Move the iTelescope network reference and campaign under itelescope/
Preparing to merge this repository into a combined astrophotography repo. The network review, the southern-target guide, the drain campaign and the observing plans all belong together under one directory; the Default Workflow files (CLAUDE.md, docs/, state/) stay at the top level because they will govern the combined repository rather than just this part of it.
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itelescope/CAMPAIGN.md
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itelescope/CAMPAIGN.md
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# Drain campaign: spend 2,638 points, then close the account
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Decision (2026-07-18): use the full points balance on southern imaging, then cancel
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the membership. Constraints and policy facts that shape the plan:
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- Balance 2,638 points; Plan-40 renews 12 Aug 2026 (GBP 32). Cancel BEFORE renewal.
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- Points cannot be refunded, and cannot be used without an active subscription
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(support article 142963). So: drain first, cancel last, in that order.
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- **Cancellation target: 10 Aug 2026**, two days before renewal. Cancellation is
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submitted via MyAccount/Cancel.aspx and requires explicit user confirmation on the
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day; Claude must not submit it unprompted.
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- Rates: see the rate card in state/NOTES.md. Billing is per minute of imaging time.
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- Moon: bright nights roughly 24 Jul - 2 Aug (full ~29 Jul); dark again 5-12 Aug.
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Full-moon week includes free access promotions; paid draining focuses on dark and
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grey nights, narrowband carries the bright week.
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- Scope availability is volatile (much of Chile offline as of 18 Jul); re-check the
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status line on go.itelescope.net before every session and substitute freely.
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## Session ledger
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Update after every run: date, scope, target, imaging minutes, points charged
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(from account/history.aspx), cumulative spend.
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| Date | Scope | Target | Plan file | Imaging | Est. pts | Actual pts | Notes |
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|---|---|---|---|---|---|---|---|
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| 2026-07-19 | T33 | 47 Tuc | ngc104-test.txt | 17 min | 0 (free) | DID NOT RUN | reservation 749228 expired unused: no images, no logs on T33 (checked 20 Jul); grid shows reschedule=No despite the flag being set at booking |
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| 2026-07-19 | T59 | NGC 6744 | ngc6744-t59.txt | 180 min | ~240 (0% moon disc. until 21 Jul) | **381** | SUCCESS (txn 851148): ran 00:05:22-03:29:56 SSO, Time Used 3h24m32s, 0% moon disc. Full dataset on scope server: L 15x300s BIN1, RGB 7x300s each BIN2; previews checked, round stars, galaxy clean: no refund case. Effective rate ~112 pts/hr of WALL time (not the 80/hr imaging-time estimate: see NOTES rate correction) |
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| 2026-07-20 | T33 | NGC 6752 | ngc6752.txt | 17 min | 0 (free) | DID NOT RUN | reservation 749229 expired unused: no images, no logs (checked 20 Jul 20:30 UTC, after window) |
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| 2026-07-21 | T32 | Centaurus A | cena-t32.txt | 120 min | ~350 (x1.6 model) | **160** | SUCCESS (txn 851344): ran 18:50:24-21:16:19 SSO local (08:50-11:16 UTC), Time Used 2h25m55s, 25% moon discount. Images present: /images/qisback/T32/NGC5128 on t32.itelescope.net:8032. Came in at 0.46x the x1.6 model, i.e. LESS than the original estimate: see the rate correction below |
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Cumulative spend: 541. Balance after (verified GetAccountStatus 2026-07-21
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11:40 UTC): **2,097**.
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**Rate correction (2026-07-21, supersedes the 2026-07-20 x1.6 warning).** Two
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paid runs now bracket the question, and both bill EXACTLY the plan's imaging
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minutes, not wall-clock:
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| Scope | Plan imaging | Wall (Time Used) | Billed | Points per imaging hour |
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|---|---|---|---|---|
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| T59 | 180 min (36x300s) | 3h24m32s | 381 | **127** (0% moon) |
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| T32 | 120 min (24x300s) | 2h25m55s | 160 | **80** (25% moon) |
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381 = 3.00 h x 127 and 160 = 2.00 h x 80, both to the point. So billing is on
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imaging time as originally documented, and the wall-clock theory is dead. What
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is wrong is the rate card in NOTES.md: it lists T59 at 80/hr (actual 127) and
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T32 at 146/hr (actual 80 even after the 25% moon discount, so a base near
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107/hr). The two look transposed, but two samples cannot prove that. **Do not
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apply a blanket multiplier.** Derive each scope's effective rate from its first
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actual bill, and treat any not-yet-observed scope's card rate as +/-60%.
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## Planned allocation (~2,600 points, adapt as scopes/weather allow)
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**Phase 1, dark nights now - 23 Jul (~1,030 pts):**
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- T59 NGC 6744 LRGB, 3 h, ~240 (scheduled 19 Jul)
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- T32 Centaurus A LRGB, 2 h, ~292: early UK-afternoon window while it is high
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- T8 Corona Australis dust complex LRGB, 2 h, ~260
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- T70 (Chile) Scorpius tail / Prawn super-wide LRGB, 2 h, ~238
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**Phase 2, bright nights 24 Jul - 2 Aug (~440 pts, narrowband only):**
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- T59 NGC 6188 in Ha/OIII/SII 5nm, 3 h total, ~240
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- T8 Ha on the Cat's Paw / War and Peace field, 1.5 h, ~195
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- Plus any full-moon free promotions for clusters (cost 0, not part of the drain)
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**Phase 3, dark nights 3 - 10 Aug (~1,130 pts):**
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- T8 SMC + 47 Tucanae in one frame, 3 h LRGB, ~390: the signature shot, SMC well
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placed in the second half of the SSO night by August
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- T8 or T59 Large Magellanic Cloud attempt if it clears the elevation limits late
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in the window; otherwise Tarantula on T32, 2 h, ~292
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- Remainder (~450): best-of list: repeat the strongest target for more depth, or
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Chile scopes (T71 106/hr, T73 224/hr) if they return from maintenance: Tarantula
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and NGC 1313 preferred. Aim to land the balance under ~50 points.
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## Booked reservations (all with plan attached + reschedule flag)
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| ID | Scope | Night of (SSO/obs local) | Slot | Plan | Est. pts | Status (2026-07-20) |
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|---|---|---|---|---|---|---|
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| 749227 | T59 | 19 Jul | 00:05-03:45 | ngc6744-t59.txt | ~240 | COMPLETED, billed 381 |
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| 749228 | T33 | 19 Jul | 00:05-00:50 | ngc104-test.txt | 0 | EXPIRED unused (no run, no auto-reschedule) |
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| 749229 | T33 | 20 Jul | 00:05-00:50 | ngc6752.txt | 0 | EXPIRED unused (no run, no auto-reschedule) |
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| 749230 | T8 | 26 Jul | 21:35-23:55 | catspaw-t8.txt | ~146 (25% moon disc.) | still booked |
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| 749302 | T32 | 21 Jul | 18:50-21:50 | cena-t32.txt | ~350 (x1.6 rate, 25% moon disc.) | COMPLETED, billed 160. EVENING slot: T32 has a 35 deg elevation floor and Cen A culminates ~17:10 before dark, sinking to 11 deg by the old 00:35 slot (which could never have run). Ran 18:50-21:16, finishing 34 min early (plan complete, not a fault); images landed under /images/qisback/T32/NGC5128 |
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| (id not captured) | T8 | 22 Jul | 21:45-00:45 | cra-t8.txt | ~250 | booked + MySummary-verified 2026-07-21 11:45 UTC. This is queue #2 finally placed: see the resolution note below. Runs 11:45-14:45 UTC 22 Jul |
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| (id not captured) | T32 | 22 Jul | 18:50-19:50 | hdrcore-t32.txt | ~25 | **CANCELLED 2026-07-21 ~15:00 UTC, never ran, 0 points spent.** Booked to fix a saturated Cen A nucleus; the nucleus is not saturated (see the correction below). Deleted from MySummary with the other three reservations verified intact afterwards; quota back to 6:05/8:00 |
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| 749314 | T33 | 21 Jul | 00:05-00:50 | ngc104-test.txt | 0 (free) | booked + grid-verified 2026-07-21 08:55 UTC. 47 Tuc first-light retry, third attempt. Runs 14:05-14:50 UTC 21 Jul. Reschedule flag again No (free scopes never rebook) |
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The T33 first-light test is now on its THIRD booking (749314); the two prior free
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reservations expired unused. If this one also fails to run, the problem is not the
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booking but the auto-start on free scopes: escalate to walk-in (POST plan.asp per
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plans/README.md) or drop the free-imaging objective.
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## Booking queue (blocked by the rolling 8-hour reservation allowance)
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Book in order as quota frees (a session completing releases its hours). Exact
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New.aspx parameters; all plans already uploaded and verified on their scopes.
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Verify every booking via Edit.aspx?id= probing (sequential ids), NOT the grid.
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| # | Scope id | start | end | start sel | end sel | Plan | Est. pts |
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|---|---|---|---|---|---|---|---|
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| 1 | BOOKED as 749302 (see table above); the original 00:35 slot was an error, Cen A is an EVENING target (35 deg floor on T32) | | | | | cena-t32.txt | ~350 |
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| 2 | BOOKED 2026-07-21 for the night of 22 Jul, 21:45-00:45 (see table above); the 01:35 slot was blocked by hajo and low anyway | | | | | cra-t8.txt | ~250 |
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| 3 | GRAS059 | 2026-07-25T20:35:00 | 2026-07-25T23:55:00 | 8:35 PM | 11:55 PM | ngc6188-haoiii-t59.txt | ~120 (disc.) |
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| 4 | GRAS059 | 2026-07-27T20:35:00 | 2026-07-27T23:05:00 | 8:35 PM | 11:05 PM | ngc6188-sii-t59.txt | ~90 (disc.) |
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| 5 | GRAS008 | 2026-08-08T02:35:00 | 2026-08-08T06:05:00 | 2:35 AM | 6:05 AM | smc47tuc-t8.txt | ~390 |
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| 6 | GRAS032 | 2026-08-09T03:05:00 | 2026-08-09T06:05:00 | 3:05 AM | 6:05 AM | tarantula-t32.txt | ~365 |
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| 7 | (T70, blocked: server unreachable) | night TBD before 5 Aug | ~2.5h | | | scorpius-t70.txt (in scratch, re-upload needed) | ~238 |
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| 8 | WITHDRAWN: booked then cancelled 2026-07-21, premise was wrong (see below) | | | | | hdrcore-t32.txt | 0 |
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### CORRECTION (2026-07-21): the Cen A nucleus was never saturated
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An earlier entry here claimed the 21 Jul Cen A data came back with a saturated
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nucleus, and booked a short-exposure core set on that basis. **The claim was
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wrong and the booking has been cancelled without running, at a cost of zero
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points.**
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The 65313 ADU figure came from taking the maximum pixel inside a 300 x 300 px
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box centred on the frame. That measures the brightest thing near the middle of
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the image, which is not the same as measuring the galaxy: it was a foreground
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star 128 px (69 arcsec) from the nucleus, sitting inside the box. Median
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filtering the inner 800 x 800 px to remove stars leaves the galaxy peaking at
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**1944 ADU**, about a thirtieth of the clip level, with **not one star-free
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pixel above 30000 ADU**. The core looked blown in the first processed image
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because of the display stretch, whose white point was set by field stars, and
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re-rendering the same data with a second tone curve scaled to the galaxy
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recovered it fully.
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**The habit that IS worth keeping, in corrected form:** before booking extra
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time to fix a saturated core, *measure whether it is saturated* - median-filter
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the inner region to remove stars first, and check where the frame's bright
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pixels actually are. The check costs a minute. 47 Tuc and the SMC (queue #5)
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may still genuinely saturate, a dense cluster core being the fastest thing there
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is to clip, so run the same measurement on their data before assuming either
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way. plans/hdrcore-t32.txt stays in the repo (and on T32) as a ready-made
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ladder if one of them turns out to need it.
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### Session 2026-07-21 ~08:55 UTC (booking round run early, before Cen A ran)
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Done this session: free T33 47 Tuc retry booked as 749314 (grid-verified). NOT
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done, both correctly deferred:
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- **Cen A verify**: 749302 had not run yet (starts 08:50 UTC, this session ran at
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08:48). Verify after 11:50 UTC.
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- **cra-t8 (#2)**: blocked twice over. (1) Quota: Cen A holds 3h until it
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completes ~11:50 UTC; with Cat's Paw (2h20m) + Cen A (3h) + T33 (45m) held,
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under ~1h55m is free, not enough for a 3h slot. (2) Conflict: user hajo holds
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T8 00:25-02:25 SSO local (res 749207), overlapping our planned 01:35-04:35.
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**cra-t8 resolution options** (pick with a live grid re-check when quota frees):
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- (a) Shift to 02:25-05:25 after hajo. Downside: Corona Australis culminates
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~22:30 SSO local, so by 02:25-05:25 it is 4-6.5h past meridian and low; poor.
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- (b) PREFERRED: move cra-t8 to the NEXT night, 2026-07-23T01:35-04:35 (night of
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22 Jul SSO), same clock time, avoids hajo, keeps decent altitude. Re-check that
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night's T8 grid first. One night's slip is fine inside the drain window.
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- (c) Earlier slot 21:25-00:25 (before hajo) is astronomically best but starts
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11:25 UTC, before Cen A releases quota at 11:50; not bookable in time.
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The scheduled 12:13 UTC job (ae3af497) fires after Cen A completes: it should
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verify Cen A + bill, then book cra-t8 by option (b) unless the grid has changed
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(hajo may cancel, opening option (a)/original). At corrected (x1.6) rates the
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full remaining queue runs ~2,530 vs 2,257 balance (~270 over): once actual bills
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for Cen A and CrA land, trim Phase 3 (shorten Tarantula #6 or the SMC slot)
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to land the balance near zero.
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### Session 2026-07-21 ~11:40 UTC (Cen A verify + cra-t8 booked)
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Ran ahead of the 12:13 UTC scheduled job, after Cen A had finished at 11:16 UTC.
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- **Cen A verified**: completed, billed 160, NGC5128 images on the scope server.
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Ledger and rate model updated (the x1.6 model is withdrawn: see the rate
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correction above).
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- **cra-t8 booked**, but on a better slot than the deferred option (b). Probing
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New.aspx for the original 01:35-04:35 returned "Conflicting reservation. Start
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time must be later than 2:25 AM" (hajo, as predicted), confirming that option
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(a) was all that remained on the night of 21 Jul, and it puts Corona Australis
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3.5-6.5 h past the meridian. Instead the run went to the EVENING of the next
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night: **2026-07-22T21:45 - 2026-07-23T00:45 SSO local**, which brackets the
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~22:30 culmination, so the whole 115 min of imaging happens near the zenith.
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This is option (c)'s geometry on option (b)'s night; the reason (c) was
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unbookable earlier (quota held by Cen A) had expired by the time Cen A
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completed. Grid probing showed no conflict on either side of the slot.
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Verified in Reservation/MySummary.aspx; quota now 6:50 / 8:00.
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- Moon on the night of 22 Jul is ~57% illuminated, the last usable night before
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the bright-week narrowband phase. LRGB on a dust complex under a half moon is
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a compromise, but the alternative is slipping a Phase 1 broadband target into
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the bright week, which is worse.
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- Reservation id NOT captured: the confirm response carries only
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`ModalStatic.result("OK")` and MySummary does not print ids. Nothing depends
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on the id unless the booking must be edited or deleted, in which case find it
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by probing Edit.aspx?id= around the current sequence (749314 was issued
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~08:55 UTC on 21 Jul).
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- Budget: 2,097 left, 19 nights to 10 Aug. Remaining queue at card rates is
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roughly 1,300, which UNDER-spends by ~800. With the x1.6 model withdrawn, the
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next planning session should add work rather than trim it: candidates are a
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second narrowband night on T59 (observed 127/hr, the only scope with a
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trustworthy rate), or extending the Phase 3 SMC and Tarantula runs, both of
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which have the sky time to absorb longer plans.
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Substitution rules: if T71 returns to service, move #2 and #7 to T71 (faster
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f/2.8 optics, cheaper 106 pts/hr; re-cut the plans for 1.55"/px). If T70's
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server returns, book #7 as-is. Check the go.itelescope.net status line before
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each booking round. After #6, allocate the remaining balance (~450 pts) to a
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final deep session on the best-performing scope, sized to land under 50 pts.
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**10 Aug: verify balance is near zero, download ALL data from data.itelescope.net,
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then (with explicit user confirmation) cancel via MyAccount/Cancel.aspx.**
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## Operational notes
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- Sessions are now RESERVED, not walk-in: upload the plan to the scope, then book
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it at reservations.itelescope.net with the plan attached (procedure in
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plans/README.md); iTelescope auto-starts the plan at reservation start and the
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reschedule flag retries weather losses. Claude sessions monitor rather than
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drive. T59 moon discount correction: 0% until 21 Jul, 25% from 22 Jul.
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- Cron jobs live only in an open Claude session; if a day's session has no live
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session to fire it, the user prompts "run today's drain session" and any session
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picks it up from this file plus state/TODO.md.
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- Bad-data protection: iTelescope refunds points for weather-ruined runs on
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request; check each session's images before marking the ledger final.
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- Final data sweep before cancellation: everything on data.itelescope.net AND the
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per-scope /images/qisback/ folders.
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18
itelescope/README.md
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itelescope/README.md
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# itelescope
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Reference and review of the [iTelescope.net](https://www.itelescope.net/) remote
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telescope network: every telescope, its specs, what it is good at, and which one to
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book for a given target.
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- **[TELESCOPES.md](TELESCOPES.md)**: the full review, grouped by observatory, with a
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"choosing a telescope" guide at the end.
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- **[TARGETS.md](TARGETS.md)**: southern-sky targets invisible from the UK, matched
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to scopes and to the time of year to book them.
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- **[data/itelescope-telescopes.csv](data/itelescope-telescopes.csv)**: snapshot of
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the network's maintained specs sheet (source of truth for the numbers).
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- **state/**: project state under the Default Workflow.
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Sources: the iTelescope support article
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([telescope summary](https://support.itelescope.net/support/solutions/articles/247371))
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and the network's maintained Google Sheet. The launchpad at
|
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[go.itelescope.net](https://go.itelescope.net/) is login-only.
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155
itelescope/TARGETS.md
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155
itelescope/TARGETS.md
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@ -0,0 +1,155 @@
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# Southern targets: what the UK can never show you
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A target guide for imaging objects that are invisible (or hopeless) from the UK,
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using the southern half of the iTelescope network: Siding Spring, Australia (Q62)
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and Deep Sky Chile (X07). Companion to [TELESCOPES.md](TELESCOPES.md).
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## The visibility rule from the UK
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From latitude 51.5°N (southern England), an object's maximum altitude is
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`90° - 51.5° + declination`:
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- **Dec below about -38°: never rises.** These objects cannot be imaged from the UK
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at all, ever.
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- **Dec -25° to -38°: technically rises, practically hopeless.** Culminates under
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~15° altitude, buried in atmosphere and murk.
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- Dec -10° to -25°: imageable from the UK but always low and compromised; far better
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from the southern sites.
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Everything below is grouped by those tiers, then matched to scopes and to the time
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of year when it is best placed from the southern sites.
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## Tier 1: never visible from the UK (dec < -38°)
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### The Magellanic Clouds (the headline act)
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| Target | Dec | Best scope | Notes |
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|---|---|---|---|
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| Large Magellanic Cloud | -69° | T8 | The whole LMC just fits T8's 4 x 4 degree field |
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| Tarantula Nebula (NGC 2070) | -69° | T73, T17 | Core detail; the finest emission nebula in either sky |
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| Small Magellanic Cloud + 47 Tucanae | -72° | T8 | Both in a single T8 frame, a unique composition |
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| 47 Tucanae (NGC 104) alone | -72° | T33 (free), T73 | Second-finest globular in the sky |
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### Carina and Crux region
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| Target | Dec | Best scope | Notes |
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|---|---|---|---|
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| Eta Carinae Nebula (NGC 3372) | -59° | T71 | Fills T71's 2.7 x 1.8 degree field perfectly; narrowband showpiece |
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| Carina to Crux widefield | -60° | T70 | The richest stretch of the Milky Way in one 8-degree frame |
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| Southern Pleiades (IC 2602) | -64° | T71, T75 | Bright open cluster |
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| Running Chicken (IC 2944) | -63° | T71, T75 | Emission nebula with Bok globules |
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| Wishing Well Cluster (NGC 3532) | -58° | T71 | Reportedly the best open cluster in the sky |
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| Coalsack + Southern Cross | -60° | T70 | Dark nebula composition |
|
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### Centaurus and the southern globulars
|
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| Target | Dec | Best scope | Notes |
|
||||
|---|---|---|---|
|
||||
| Omega Centauri (NGC 5139) | -47° | T59, T17 | The largest globular cluster known; needs the ~40 arcmin fields |
|
||||
| Centaurus A (NGC 5128) | -43° | T17, T32, T73 | Iconic dust-lane radio galaxy |
|
||||
| NGC 4945 | -49° | T73 | Big edge-on spiral, underimaged |
|
||||
| NGC 6752 (Pavo globular) | -60° | T33 (free) | Third-brightest globular |
|
||||
|
||||
### Ara, Norma and the Scorpius tail
|
||||
|
||||
| Target | Dec | Best scope | Notes |
|
||||
|---|---|---|---|
|
||||
| Fighting Dragons of Ara (NGC 6188) | -49° | T71 | Dramatic narrowband target |
|
||||
| Prawn Nebula (IC 4628) | -40° | T71, T75 | Large, faint, great in Ha |
|
||||
| NGC 6231 + Table of Scorpius | -42° | T71 | Rich cluster region |
|
||||
|
||||
### Far-southern galaxies
|
||||
|
||||
| Target | Dec | Best scope | Notes |
|
||||
|---|---|---|---|
|
||||
| NGC 6744 (Pavo) | -63° | T73, T17 | Milky Way lookalike spiral |
|
||||
| NGC 1313 (Topsy-Turvy) | -66° | T73 | Distorted starburst spiral |
|
||||
| NGC 1566 (Spanish Dancer) | -55° | T73 | Grand-design face-on spiral |
|
||||
| NGC 2070 region galaxies | -69° | T17 | See Magellanic section |
|
||||
|
||||
### Southern nebulae, supernova remnants and planetaries
|
||||
|
||||
| Target | Dec | Best scope | Notes |
|
||||
|---|---|---|---|
|
||||
| Vela SNR | -45° | T70 | Huge filamentary shell, needs the 8-degree field |
|
||||
| Gum Nebula | -43° | T70 | 36 degrees across; even T70 mosaics it |
|
||||
| Southern Ring (NGC 3132) | -40° | T73 | Small bright planetary |
|
||||
| Toby Jug Nebula (IC 2220) | -59° | T73 | Reflection nebula |
|
||||
|
||||
## Tier 2: hopeless from the UK (dec -25° to -38°), excellent from the south
|
||||
|
||||
| Target | Dec | Best scope | Notes |
|
||||
|---|---|---|---|
|
||||
| Cat's Paw (NGC 6334) | -36° | T71 | Narrowband showpiece |
|
||||
| War and Peace (NGC 6357) | -34° | T71 | Pairs with the Cat's Paw in one T75 framing |
|
||||
| NGC 1365 (Great Barred Spiral) | -36° | T73, T17 | The archetypal barred spiral, Fornax |
|
||||
| Fornax cluster core | -35° | T17, T32 | Galaxy cluster field |
|
||||
| M83 (Southern Pinwheel) | -30° | T73, T17 | Face-on spiral, superb from Q62/X07 |
|
||||
| NGC 300 and NGC 55 (Sculptor) | -37°/-39° | T17, T75 | Nearby resolved spirals |
|
||||
| NGC 253 (Sculptor Galaxy) | -25° | T17, T32 | Huge dusty starburst, low and ruined from the UK |
|
||||
| Corona Australis dust complex | -37° | T71, T75 | Reflection nebula and dust river |
|
||||
|
||||
## When to book what (from the southern sites)
|
||||
|
||||
Seasons refer to what is well placed in the evening-to-midnight sky at Siding Spring
|
||||
and Deep Sky Chile. Siding Spring scopes have 30-35 degree minimum elevation limits,
|
||||
so aim within a few hours of culmination; T70 in Chile can go to the horizon.
|
||||
|
||||
- **Jan-Mar:** Tarantula and the LMC, NGC 1313, Vela SNR and the Gum Nebula, Carina
|
||||
rising late evening.
|
||||
- **Apr-Jun:** Eta Carinae at its best, Crux and the Coalsack, Omega Centauri,
|
||||
Centaurus A, NGC 4945, the Musca dark nebulae.
|
||||
- **Jul-Sep (now):** the Scorpius tail and Ara at the zenith: Cat's Paw, War and
|
||||
Peace, Prawn, NGC 6188, NGC 6231; NGC 6744; Corona Australis; 47 Tucanae and the
|
||||
SMC in the second half of the night.
|
||||
- **Oct-Dec:** Magellanic Cloud prime time, 47 Tucanae, Sculptor galaxies (NGC 253,
|
||||
55, 300), Fornax cluster and NGC 1365, NGC 1566.
|
||||
|
||||
## A sensible first campaign (July-August)
|
||||
|
||||
1. **Free warm-up on T33** (30 min/day, Siding Spring): 47 Tucanae or NGC 6752 in
|
||||
LRGB across a few nights. Costs nothing, learns the booking system.
|
||||
2. **T71 narrowband run** (Chile, f/2.8): NGC 6188 or the Cat's Paw + War and Peace
|
||||
region. Fast optics keep the bill down; use the standard 300 s calibrated subs.
|
||||
3. **T73 galaxy shot**: NGC 6744, currently well placed, as an LRGB target.
|
||||
4. **Book ahead for October-November:** T8 for the LMC (or SMC + 47 Tuc in one
|
||||
frame): the single most "you cannot do this from the UK" image on the network.
|
||||
|
||||
## Budgeting a points balance
|
||||
|
||||
Published rate shape (from itelescope.net/standard-plans, 2026-07): affordable
|
||||
scopes roughly $19-54 per imaging hour, premium scopes roughly $54-118 per hour,
|
||||
where the range is the moon-phase discount (dark of moon at the top of the range,
|
||||
bright moon at the bottom) and the plan discount (10% on Plan-40, 20% on Plan-90).
|
||||
Exact per-scope, per-night rates are shown in the login portal's planner; treat the
|
||||
numbers below as planning estimates, not quotes.
|
||||
|
||||
What a ~2,600 point balance buys, roughly:
|
||||
|
||||
- **A strong narrowband image on a fast scope (T71, T75):** 2-3 hours of exposure
|
||||
is plenty at f/2.8-f/3.8; booked around gibbous moon the rate is at the low end,
|
||||
so call it 150-350 points per finished target.
|
||||
- **An LRGB galaxy on T73 or T17:** wants dark-of-moon time at premium-scope rates;
|
||||
3-4 hours, roughly 300-500 points per target.
|
||||
- **The T8 Magellanic Cloud shot:** 2-3 hours LRGB at a mid-range rate, roughly
|
||||
200-350 points.
|
||||
|
||||
So ~2,600 points is comfortably 8-12 finished showpiece targets, or a full year of
|
||||
the seasonal calendar above at one or two targets a month. Stretch it further with:
|
||||
|
||||
- **Full moon weeks are free** on the standard plans: use them for bright globulars
|
||||
and clusters (47 Tuc, NGC 3532, IC 2602) where moonlight matters least, and keep
|
||||
paid time for faint stuff.
|
||||
- **The daily free 30 minutes** (T33 south, T68 north) for framing tests and short
|
||||
targets, never spend points discovering a framing mistake.
|
||||
- **Moon-phase arbitrage:** book narrowband (Carina, Ara, Cat's Paw) at bright moon
|
||||
when rates bottom out; the 3 nm filters do not care about moonlight.
|
||||
|
||||
## Cost-shape notes
|
||||
|
||||
- Fast scopes (T71 f/2.8, T75 f/3.8, T70 f/3.5) reach depth in the least imaging
|
||||
time, which is what you pay for: prefer them for nebulae.
|
||||
- The two free scopes cover both hemispheres of this list poorly (T68 is northern)
|
||||
but T33 covers southern globulars and compact targets well.
|
||||
- Moonlight: narrowband targets (Carina, Ara, Scorpius nebulae) tolerate moon;
|
||||
save galaxy and globular time (T73, T17, T8 LRGB) for dark-of-moon bookings.
|
||||
377
itelescope/TELESCOPES.md
Normal file
377
itelescope/TELESCOPES.md
Normal file
|
|
@ -0,0 +1,377 @@
|
|||
# iTelescope.net telescope review
|
||||
|
||||
A review of every telescope on the iTelescope.net network, grouped by observatory.
|
||||
Compiled 2026-07-17 from the network's own sources:
|
||||
|
||||
- Support article (observatory summaries, minimum elevations):
|
||||
https://support.itelescope.net/support/solutions/articles/247371
|
||||
- Maintained specs Google Sheet (snapshotted in [data/itelescope-telescopes.csv](data/itelescope-telescopes.csv)):
|
||||
https://docs.google.com/spreadsheets/d/1jZWkkjewOuyNC9YzQ8y2d0pO1e4T7EBeysmQMPBVSOk/
|
||||
- The launchpad (https://go.itelescope.net/) is login-only and holds no public specs.
|
||||
|
||||
Note on coverage: the Google Sheet is the maintained source and is what this review
|
||||
follows. The older support article additionally lists T9, T19, T31 and T69, which no
|
||||
longer appear in the sheet (retired or rebuilt); T74 appears in the sheet with no
|
||||
specs, presumably in commissioning.
|
||||
|
||||
## The network at a glance
|
||||
|
||||
| Observatory | MPC code | Hemisphere | Telescopes |
|
||||
|---|---|---|---|
|
||||
| Utah Desert Remote Observatory, USA | U94 | North | T2, T5, T11, T14, T20, T21, T25, T26, T68 |
|
||||
| Sierra Remote Observatory, California, USA | U69 | North | T24 |
|
||||
| Siding Spring Observatory, Australia | Q62 | South | T8, T17, T30, T32, T33, T59 |
|
||||
| Deep Sky Chile | X07 | South | T70, T71, T72, T73, T74, T75 |
|
||||
| AstroCamp Observatory, Spain | I89 | North | T18 |
|
||||
| Entre Encinas y Estrellas (e-EyE), Spain | (none listed) | North | T80 |
|
||||
|
||||
Two systems are free to use (30 minutes per day): **T68** (Utah, fast colour
|
||||
widefield) and **T33** (Siding Spring, narrow deep field).
|
||||
|
||||
---
|
||||
|
||||
## Utah Desert Remote Observatory (MPC U94)
|
||||
|
||||
Dark Great Basin desert site; the largest cluster on the network and the main
|
||||
northern-hemisphere hub.
|
||||
|
||||
### T2: Takahashi TOA-150 + QHY268C (one-shot colour)
|
||||
|
||||
- 150 mm f/7.3 apochromatic refractor, 1105 mm focal length
|
||||
- QHY268C colour CMOS (Sony IMX571, APS-C), 0.69"/px, 72.6 x 48.6 arcmin
|
||||
- Paramount GTS, off-axis guided, no filters; minimum elevation 25 degrees
|
||||
|
||||
**Review:** the premium one-shot-colour option. Superb refractor optics and a modern
|
||||
back-illuminated sensor at a well-sampled 0.69"/px make it the easiest route to a
|
||||
finished colour image of medium-sized targets (galaxy groups, planetary nebulae,
|
||||
globulars) with no filter runs to plan. No narrowband, so emission nebulae under
|
||||
moonlight are off the menu. Files are large (26 MP 16-bit FITS).
|
||||
|
||||
### T5: Takahashi Epsilon 250 + SBIG ST-10XME
|
||||
|
||||
- 250 mm f/3.4 hyperbolic flat-field astrograph, 850 mm focal length
|
||||
- ST-10XME CCD (NABG), 1.66"/px, 60.6 x 40.8 arcmin
|
||||
- Paramount PME, external guiding; RGB, Ha/SII/OIII, and Johnson-Cousins B, V, I
|
||||
|
||||
**Review:** a fast classic. The f/3.4 Epsilon gathers light quickly for its class and
|
||||
the photometric filter set makes it one of the few scopes that does both pretty
|
||||
pictures and science. The small, old NABG CCD is the weak point: only 3.2 MP, and
|
||||
bright stars bloom on long exposures, so keep subs short around bright fields.
|
||||
|
||||
### T11: Planewave CDK20 + FLI ProLine PL11002M
|
||||
|
||||
- 510 mm (20") f/4.5 corrected Dall-Kirkham with 0.66x reducer, 2280 mm
|
||||
- PL11002M CCD (full frame), 0.81"/px, 54.3 x 36.2 arcmin
|
||||
- Ascension 200HR; LRGB, 3 nm narrowband, and U, B, V, R, I; minimum elevation 20 degrees
|
||||
|
||||
**Review:** big aperture at a fast reduced focal ratio with a generous field: a strong
|
||||
general-purpose deep-space scope for nebulae and larger galaxies, plus full UBVRI for
|
||||
photometry. The sensor's 51% peak QE is dated, so it needs more integration time than
|
||||
the CMOS scopes for the same depth, and it is noted as sensitive to stray-light
|
||||
gradients near full moon.
|
||||
|
||||
### T14: Takahashi FSQ-106 Fluorite + SBIG STX-16803
|
||||
|
||||
- 106 mm f/5.0 Petzval refractor, 530 mm focal length
|
||||
- STX-16803 CCD, 3.5"/px, 238.8 x 238.8 arcmin (4 x 4 degrees)
|
||||
- Paramount ME, unguided; LRGB, 5 nm Ha/SII/OIII, V; minimum elevation 25 degrees
|
||||
|
||||
**Review:** the classic mono widefield workhorse. Four square degrees on the square
|
||||
16803 sensor suits large nebula complexes (North America, Veil, Rho Ophiuchi) and
|
||||
mosaics. CCD rather than CMOS, so integration is slower than modern rivals, and
|
||||
dithering is recommended. Pick it for framed mono narrowband over T20's colour.
|
||||
|
||||
### T20: Takahashi FSQ-106ED + ZWO ASI2400C (one-shot colour)
|
||||
|
||||
- 106 mm f/5.0 Petzval refractor, 530 mm focal length
|
||||
- ASI2400C colour CMOS (Sony IMX410, full frame, 14-bit), 2.31"/px, 233.7 x 155.8 arcmin
|
||||
- Paramount ME, unguided; Optolong L-Pro and L-Ultimate (3 nm dual-band), Astrodon narrowband
|
||||
- Field rotated 90 degrees relative to T14 for alternative framing
|
||||
|
||||
**Review:** the colour twin of T14 with a modern full-frame CMOS. The L-Ultimate
|
||||
dual-band filter is the clever bit: one-shot-colour narrowband on emission nebulae,
|
||||
even with the moon up. Sensor is 14-bit, so dynamic range trails the mono 16-bit
|
||||
scopes. The best low-effort widefield choice on the network.
|
||||
|
||||
### T21: Planewave CDK17 + FLI PL6303E
|
||||
|
||||
- 431 mm (17") f/4.5 corrected Dall-Kirkham with 0.66x reducer, 1940 mm
|
||||
- PL6303E CCD (NABG), 0.96"/px, 49.2 x 32.8 arcmin
|
||||
- Ascension 200HR; Astrodon LRGB, 5 nm narrowband, and UBVRI; minimum elevation 20 degrees
|
||||
|
||||
**Review:** billed as a combined photometry and imaging system, and that is its niche:
|
||||
the sensitive NABG chip plus a full Johnson-Cousins set makes it a proper science
|
||||
scope. The same NABG sensitivity means blooming on bright subjects, so it rewards
|
||||
careful target and exposure choice rather than casual use.
|
||||
|
||||
### T25: Planewave CDK20 + Player One Zeus 455M PRO
|
||||
|
||||
- 508 mm (20") f/6.8 corrected Dall-Kirkham at native focal length, 3454 mm
|
||||
- Zeus 455M mono CMOS (Sony IMX455, full frame), 0.23"/px, 36.2 x 24.2 arcmin, 61 MP
|
||||
- Planewave L-500; Astrodon LRGB and 3 nm narrowband
|
||||
|
||||
**Review:** the resolution monster. At 0.23"/px it is oversampled for almost any
|
||||
seeing, which means you can bin or drizzle as you please and still resolve fine
|
||||
structure in small galaxies and planetary nebulae. The cost is enormous files (61 MP
|
||||
per sub) and a narrow field. Choose it when the target is small and detail is the
|
||||
point.
|
||||
|
||||
### T26: Planewave Delta Rho 500 + ZWO ASI6200MM Pro
|
||||
|
||||
- 508 mm (20") f/3.0 corrected astrograph, 1537 mm focal length
|
||||
- ASI6200MM mono CMOS (IMX455, full frame, Bin2 only), 1.01"/px, 80.4 x 54.0 arcmin
|
||||
- Planewave L-550 on equatorial wedge; Chroma LRGB and 3 nm narrowband
|
||||
- Recommended subs: LRGB 30-180 s, narrowband 180-300 s (900 s available)
|
||||
|
||||
**Review:** arguably the best imaging system on the network: half a metre of aperture
|
||||
at f/3.0 with a modern 91% QE sensor is a light bucket that reaches faint extended
|
||||
nebulosity (integrated flux nebulae, faint Ha shells) in a fraction of the usual
|
||||
integration time, over a 1.3-degree field. Bin2-only is a software limitation, not an
|
||||
optical one, and barely matters at this image scale.
|
||||
|
||||
### T68: Celestron RASA 11 + ZWO ASI2600C (free, one-shot colour)
|
||||
|
||||
- 279 mm (11") f/2.2 Rowe-Ackermann Schmidt astrograph, 620 mm focal length
|
||||
- ASI2600C colour CMOS (IMX571, APS-C), 1.25"/px, 130.2 x 87.0 arcmin
|
||||
- Paramount ME II, mount-guided, no filters; 30 minutes free per day
|
||||
|
||||
**Review:** the free taster scope, and genuinely good: f/2.2 means even short free
|
||||
sessions produce satisfying colour images of bright nebulae and comets over a
|
||||
2-degree field. No filters and modest QE cap its ceiling. Ideal for trying the
|
||||
network, time-lapse of transients, or quick-look framing before booking a paid scope.
|
||||
|
||||
---
|
||||
|
||||
## Sierra Remote Observatory, California (MPC U69)
|
||||
|
||||
High Sierra site with steady seeing; hosts the network's largest northern aperture.
|
||||
|
||||
### T24: Planewave CDK24 + Player One Zeus 455M PRO
|
||||
|
||||
- 610 mm (24") f/6.5 corrected Dall-Kirkham, 3962 mm focal length
|
||||
- Zeus 455M mono CMOS, 0.395"/px (Bin2), 31.6 x 21.1 arcmin
|
||||
- Ascension 200HR, external guiding beyond 300 s; Astrodon LRGB, 3 nm narrowband, V and Ic
|
||||
- Match subs to calibration set (60/120/180/300/600/900 s); minimum elevation 25 degrees
|
||||
|
||||
**Review:** the northern flagship. The biggest glass in the northern half of the
|
||||
network on a steady-seeing site, with a modern high-QE sensor: first choice for small
|
||||
galaxies, quasar fields and faint photometry (V and Ic fitted). The operational notes
|
||||
(RBI flush, fixed exposure ladder, dithering) show it is run seriously for calibrated
|
||||
science data. Narrow field, so not for showpiece nebulae.
|
||||
|
||||
---
|
||||
|
||||
## Siding Spring Observatory, Australia (MPC Q62)
|
||||
|
||||
The network's southern-hemisphere anchor, on the AAO site. The only access most users
|
||||
have to Magellanic Cloud and far-southern targets at serious aperture. Roof geometry
|
||||
limits northern views (horizon limits 35-75 degrees depending on scope).
|
||||
|
||||
### T8: Takahashi FSQ-106ED + FLI Microline 16803
|
||||
|
||||
- 106 mm f/5.0 Petzval refractor, 530 mm focal length
|
||||
- ML16803 CCD, 3.5"/px, 238.8 x 238.8 arcmin (4 x 4 degrees)
|
||||
- Paramount PME, external guiding; Astrodon LRGB, EXO, narrowband, NIR luminance
|
||||
- North horizon limit 75 degrees; dithering recommended (occasional dark columns)
|
||||
|
||||
**Review:** the southern widefield essential: four square degrees on the LMC, SMC,
|
||||
Eta Carinae or the Gum Nebula is something no northern scope can offer. Same era of
|
||||
CCD as T14 with the same patience requirement, and its known dark-column quirk makes
|
||||
dithering effectively mandatory. Book it for large southern showpieces.
|
||||
|
||||
### T17: Planewave CDK17 + ZWO ASI6200MM Pro
|
||||
|
||||
- 432 mm (17") f/6.8 corrected Dall-Kirkham, 2939 mm focal length
|
||||
- ASI6200MM mono CMOS (Bin2 only), 0.53"/px, 42.4 x 28.3 arcmin
|
||||
- Paramount PME, unguided; Astrodon LRGB and 5 nm narrowband; minimum elevation 35 degrees
|
||||
|
||||
**Review:** a modern deep-field machine pointed at the southern sky: 91% QE at half an
|
||||
arcsecond per pixel is a potent combination for southern galaxies (NGC 1365, Centaurus
|
||||
A) and planetary nebulae. The tight 35-degree elevation floor means plan targets near
|
||||
culmination.
|
||||
|
||||
### T30: Planewave CDK20 + FLI PL6303E
|
||||
|
||||
- 508 mm (20") f/4.4 corrected Dall-Kirkham with 0.66x reducer, 2262 mm
|
||||
- PL6303E CCD (NABG), 0.81"/px, 41.6 x 27.8 arcmin
|
||||
- Ascension 200HR; Astrodon LRGB, 5 nm narrowband, and full Johnson-Cousins UBVRcIc
|
||||
|
||||
**Review:** the southern science scope: big aperture, fast reduced optics and the
|
||||
full photometric filter set. Same NABG blooming caveat as its northern siblings, and
|
||||
the CCD needs more integration than T17's CMOS for imaging, so treat it as
|
||||
photometry-first, imaging-second.
|
||||
|
||||
### T32: Planewave CDK17 + ZWO ASI6200MM Pro
|
||||
|
||||
- 431 mm (17") f/6.8 corrected Dall-Kirkham, 2912 mm focal length
|
||||
- ASI6200MM mono CMOS (Bin2 only), 0.53"/px, 42.4 x 28.3 arcmin
|
||||
- Ascension 200HR; Astrodon LRGB, 5 nm narrowband, plus V and Ic; minimum elevation 30 degrees
|
||||
|
||||
**Review:** effectively T17's twin with a slightly friendlier elevation limit and V/Ic
|
||||
photometric filters added. If T17 is booked, this is the same capability; if you need
|
||||
magnitudes as well as pictures, prefer T32 of the pair.
|
||||
|
||||
### T33: 12.5" RCOS Ritchey-Chretien + Apogee Alta U16 (free)
|
||||
|
||||
- 320 mm (12.5") f/9.0 Ritchey-Chretien, 2885 mm focal length
|
||||
- Alta U16 CCD (NABG), 0.54"/px, 37 x 37 arcmin
|
||||
- Paramount ME, external guiding; Astrodon LRGB and narrowband
|
||||
- 30 minutes free per day; north horizon limit 45 degrees
|
||||
- Recommended: LRGB 300 s; narrowband 300 s Bin2 or 600 s Bin1 on calm nights
|
||||
|
||||
**Review:** the free southern scope, and a much more serious instrument than "free"
|
||||
suggests: a proper RC with narrowband filters at 0.54"/px. The NABG CCD blooms on
|
||||
bright stars and f/9 is slow, so free 30-minute slots are best spent on compact,
|
||||
reasonably bright targets, or accumulated across nights.
|
||||
|
||||
### T59: Planewave CDK20 + FLI ProLine 16803
|
||||
|
||||
- 510 mm (20") f/6.8 corrected Dall-Kirkham, 3411 mm focal length
|
||||
- ProLine 16803 CCD, 0.54"/px, 37.2 x 37.2 arcmin
|
||||
- Ascension 200HR; Astrodon LRGB, 5 nm narrowband, Ic and Z; capable of 15-minute subs
|
||||
|
||||
**Review:** deep and square: the 16803's square field at half-arcsecond sampling with
|
||||
an ABG chip rated for very long exposures. The scope to book for faint southern
|
||||
targets that need 900-second narrowband subs without blooming worries. QE is dated
|
||||
(60%), so it trades sensor efficiency for exposure headroom.
|
||||
|
||||
---
|
||||
|
||||
## Deep Sky Chile (MPC X07)
|
||||
|
||||
Newest site, Atacama-quality southern skies; a modern all-CMOS lineup built around
|
||||
astrophotography.
|
||||
|
||||
### T70: Samyang 135 mm f/3.5 + ZWO ASI2600MM Pro
|
||||
|
||||
- 65 mm camera lens at f/3.5, 129 mm focal length
|
||||
- ASI2600MM mono CMOS (IMX571, APS-C), 4.51"/px, 469.8 x 355.2 arcmin (7.8 x 5.9 degrees)
|
||||
- Paramount ME, guided; Astrodon LRGB and narrowband; minimum elevation 0 degrees
|
||||
|
||||
**Review:** an eight-degree mono narrowband field under Atacama skies, down to the
|
||||
horizon. Made for constellation-scale mosaics, the Gum Nebula, and the Milky Way core.
|
||||
It is a camera lens, so expect corner coma and halos on bright stars; that is the
|
||||
stated trade for the field of view.
|
||||
|
||||
### T71: Takahashi Epsilon 180ED + ZWO ASI2600MM Pro
|
||||
|
||||
- 180 mm f/2.8 hyperbolic Newtonian astrograph, 500 mm focal length
|
||||
- ASI2600MM mono CMOS, 1.55"/px, 161.4 x 108.0 arcmin
|
||||
- Paramount MyT, guided; Astrodon LRGB and 5 nm narrowband
|
||||
- Electronic shutter: no user darks; calibrated data supplied for standard sub lengths
|
||||
|
||||
**Review:** the best fast-widefield system on the network: f/2.8 optics, a modern
|
||||
sensor and Chilean skies. A 2.7 x 1.8 degree field at 1.55"/px suits nearly every
|
||||
showpiece southern nebula. Subs are constrained to the standard calibration ladder
|
||||
(10-600 s) since you cannot take your own darks, and files are large (101 MiB).
|
||||
|
||||
### T72: Planewave CDK20 + FLI ML-16200
|
||||
|
||||
- 510 mm (20") f/6.8 corrected Dall-Kirkham, 3411 mm focal length
|
||||
- ML-16200 CCD, 0.359"/px, 26.9 x 21.5 arcmin
|
||||
- Planewave L-500; LRGB, narrowband, and U, B, V, R, I
|
||||
- Precision-scaled raw calibration frames published at data.itelescope.net (0-900 s)
|
||||
|
||||
**Review:** the Chilean science workhorse: full UBVRI photometry, very fine sampling,
|
||||
and a published high-precision calibration pipeline aimed squarely at photometric
|
||||
work. The 39Ke full well is modest, so watch saturation on bright comparison stars.
|
||||
For pretty pictures the CMOS scopes on site are faster; for southern photometry this
|
||||
is the one.
|
||||
|
||||
### T73: Planewave CDK14 + ZWO ASI2600MM Pro
|
||||
|
||||
- 356 mm (14") f/7.2 corrected Dall-Kirkham, 2563 mm focal length
|
||||
- ASI2600MM mono CMOS, 0.31"/px, 31.8 x 21.0 arcmin
|
||||
- Paramount ME II, guided; Chroma LRGB and 3 nm narrowband
|
||||
|
||||
**Review:** a fine-detail southern imager: 0.31"/px oversampling with a near-zero
|
||||
dark current sensor (darks essentially redundant) and tight 3 nm Chroma narrowband.
|
||||
The pick for small southern galaxies and planetaries when T25-style resolution is
|
||||
wanted below the celestial equator. Short 240 s max recommended subs keep runs simple.
|
||||
|
||||
### T74: (in commissioning)
|
||||
|
||||
Listed in the network sheet with no published specs yet.
|
||||
|
||||
### T75: ASA N250 + ZWO ASI6200MM Pro
|
||||
|
||||
- 250 mm f/3.8 Newtonian astrograph, 950 mm focal length
|
||||
- ASI6200MM mono CMOS (Bin2 only), 1.72"/px, 137.4 x 91.8 arcmin
|
||||
- Paramount MyT, guided; Chroma LRGB and 3 nm narrowband
|
||||
|
||||
**Review:** the middle option at Deep Sky Chile: faster and wider than the CDKs,
|
||||
deeper than the Epsilon. A 2.3 x 1.5 degree field at f/3.8 with 91% QE makes quick
|
||||
work of medium-large southern nebulae. Bin2-only sampling is coarse but well matched
|
||||
to the focal length.
|
||||
|
||||
---
|
||||
|
||||
## AstroCamp Observatory, Spain (MPC I89)
|
||||
|
||||
High-altitude site in the Spanish mountains; fills the European longitude gap so
|
||||
northern targets can be followed when America is in daylight.
|
||||
|
||||
### T18: Planewave CDK12 + QHY600M
|
||||
|
||||
- 318 mm (12.5") f/5.3 corrected Dall-Kirkham, 1683 mm focal length
|
||||
- QHY600M mono CMOS (IMX455, full frame, Bin2 only), 0.92"/px, 73.6 x 49.1 arcmin
|
||||
- Paramount PME, externally guided; Astrodon LRGB, 5 nm narrowband, photometric V and Ic
|
||||
- Minimum elevation 40 degrees
|
||||
|
||||
**Review:** a well-balanced all-rounder: enough aperture for galaxies, a wide enough
|
||||
field (1.2 degrees) for most nebulae, modern sensor, and V/Ic for photometry. Its real
|
||||
value is longitude coverage for time-critical work (exoplanet transits, variable
|
||||
stars, GRB follow-up) from Europe. The 40-degree elevation floor is the strictest on
|
||||
the network, so target selection matters.
|
||||
|
||||
---
|
||||
|
||||
## Entre Encinas y Estrellas (e-EyE), Spain
|
||||
|
||||
Hosting site in Extremadura; currently one iTelescope system.
|
||||
|
||||
### T80: Samyang 135 mm f/3.5 + ZWO ASI2600MM Pro
|
||||
|
||||
- 65 mm camera lens at f/3.5, 129 mm focal length
|
||||
- ASI2600MM mono CMOS, 5.98"/px, 622.2 x 415.8 arcmin (10.4 x 6.9 degrees)
|
||||
- Paramount MyT, guided; Astrodon LRGB and narrowband
|
||||
|
||||
**Review:** T70's northern sibling: a ten-degree mono field for constellation-scale
|
||||
imaging (whole of Orion's belt and sword in one frame, big Ha mosaics of Cygnus).
|
||||
Same camera-lens caveats on corner stars. Between this and T70 the entire sky is
|
||||
covered at super-wide field.
|
||||
|
||||
---
|
||||
|
||||
## Choosing a telescope
|
||||
|
||||
| Use case | First choice | Alternatives |
|
||||
|---|---|---|
|
||||
| Widefield narrowband, north | T14 (mono), T20 (colour dual-band) | T68 (free colour) |
|
||||
| Widefield narrowband, south | T71 | T8, T75 |
|
||||
| Constellation-scale mosaics | T80 (north), T70 (south) | |
|
||||
| Faint extended nebulosity | T26 | T75, T71 |
|
||||
| Small galaxies / fine detail, north | T24 | T25 |
|
||||
| Small galaxies / fine detail, south | T73 | T17, T32, T59 |
|
||||
| Photometry / science, north | T21, T24 | T5, T11, T18 |
|
||||
| Photometry / science, south | T72 | T30, T32 |
|
||||
| One-shot colour, minimum effort | T20 | T2, T68 |
|
||||
| Long (15 min) narrowband subs, south | T59 | |
|
||||
| European longitude / transit timing | T18 | |
|
||||
| Free / trying the network | T68 (north), T33 (south) | |
|
||||
|
||||
## General observations
|
||||
|
||||
- The network is mid-migration from legacy CCDs (16803, PL6303E, ST-10XME) to modern
|
||||
back-illuminated CMOS (IMX455, IMX571): the CMOS scopes reach the same depth in
|
||||
roughly half the integration time thanks to 85-91% peak QE, and several of the CCD
|
||||
systems (NABG chips especially) carry blooming caveats the CMOS ones do not.
|
||||
- Several CMOS systems are Bin2-only due to software limitations (T17, T18, T26, T32,
|
||||
T75). At their focal lengths this costs little real resolution.
|
||||
- Minimum elevation limits vary widely (0 degrees at T70 up to 40 degrees at T18) and
|
||||
are a real planning constraint, especially at Siding Spring where the roof blocks
|
||||
much of the northern sky.
|
||||
- Calibration is handled network-side on several scopes (T71's electronic shutter
|
||||
disallows user darks; T72 publishes precision-scaled calibration frames; T24 wants
|
||||
subs matched to its calibration ladder). Check the per-scope notes before planning
|
||||
exposures.
|
||||
78
itelescope/data/itelescope-telescopes.csv
Normal file
78
itelescope/data/itelescope-telescopes.csv
Normal file
|
|
@ -0,0 +1,78 @@
|
|||
Telescope,Platform,Aperture (in),Aperature (mm),Focal Length (mm),F-Ratio,Optical Tube Assembly,Optical Design,Camera,Sensor Type,CMOS Sensor Model,Sensor Size / Format (mm),"Camera Angle
|
||||
(""Up"" = Deg. East of N)",FOV X (arcmins),FOV Y (arcmins),Pixel Size (µm),Resolution (arcsec / pixel),Sensor Megapixels,Array X,Array Y,Peak QE,Full Well,N/ABG,Recommended Max Exposure (seconds),Guiding,Mount,Filters,Notes,"Additional System Specifications
|
||||
(e.g. horizon limits, special notes)"
|
||||
,Utah Desert Remote Observatory (MPC U94),,,,,,,,Note: Sensors generally have 16-bit ADCs unless other values are provided,,,,,,,,,,,,,,,,,,,
|
||||
T2,One Shot Color,5.9,150,1105.1,f/7.3,Takahashi TOA-150,Apochromatic Refractor,QHY268C,"Color CMOS
|
||||
(RGGB Bayer)",Sony IMX571,"23.5 x 15.7
|
||||
(APS-C)",178.683º,72.6,48.6,3.76,"0.69""",26.4,6280,4210,90%,51Ke,—,300,MOAG with Loadstar SX2,Paramount GTS,None,"Large (26 MP, 16-bit) FITS files",Telescope System Information and Specs
|
||||
T5,Medium Deep Space,9.8,250,850,f/3.4,Takahashi Epsilon 250,Hyperbolic Flat-Field,SBIG ST-10XME,CCD,—,14.9 x 10.0,177º,60.6,40.8,6.8,"1.66""",3.2,2184,1472,85%,100Ke,NABG,300,External Guiding,Paramount PME,"Red Green Blue, Ha, SII, OIII, Clear and Johnson's Cousin's Photometric B,V, and I filters.",Non Anti Bloom Gate (NABG) CCD. Bright stars will bloom or bleed in long exposures. Keep your exposures short if very bright stars are in your target FoV.,Telescope System Information and Specs
|
||||
T11,Deep Space,20.1,510,"2280
|
||||
(0.66 reducer)",f/4.5,Planewave CDK20,Corrected Dall-Kirkham,FLI ProLine PL11002M,CCD,—,"36 x 24
|
||||
(Full Format)",186.9º,54.3,36.2,9,"0.81""",10.7,4008,2672,51%,60Ke,ABG,600,Active Guiding Disabled,Planewave Ascension 200HR,"AstroDon - Luminance, Red, Green, Blue. 3nm Ha3_50R, Sii3_50R, Oiii_50R. U, B, V, R, I",Optics more sensitive to stray light gradients (e.g. during full moon),Telescope System Information and Specs
|
||||
T14,Wide Field,4.2,106,530,f/5.0,Takahashi FSQ Fluorite,Petzval Apochromatic Refractor,SBIG STX-16803,CCD,—,36.8 x 36.8,90º,238.8,238.8,9,"3.5""",16.8,4096,4096,60%,100Ke,ABG,600,Unguided,Paramount ME,"LRGB, Ha (5nm), SII(5nm), OIII(5nm), V Filters",Dithering recommended,Telescope System Information and Specs
|
||||
T20,Wide Field,4.2,106,530,f/5.0,Takahashi FSQ-ED,Petzval Apochromatic Refractor,ZWO ASI2400C,"Color CMOS
|
||||
(14-bit ADC)
|
||||
(RGGB Bayer)",Sony IMX410,"36 x 24
|
||||
(Full Format)",358.4º,233.7,155.8,5.94,"2.31""",24.5,6072,4042,>80%,50Ke,ABG,300,Unguided,Paramount ME,"Optolong Lpro, Optolong LUltimate (Ha/OIII 3nm dual band), Astrodon Ha (3nm), SII (3nm) & OIII (5nm)",FoV Rotated 90° relative to T14 for different framing opportunities.,Telescope System Information and Specs
|
||||
T21,Deep Space,17.0,431,"1940
|
||||
(0.66 reducer)",f/4.5,Planewave CDK17,Corrected Dall-Kirkham,FLI-PL6303E,CCD,—,27.6 x 18.4,359º,49.2,32.8,9,"0.96""",6.3,3072,2048,68%,100Ke,NABG,600,Active Guiding Disabled,Planewave Ascension 200HR,"Astrodon LRGB 50mm unmounted, Astrodon Ha, SII, OIII, 5nm, 50 mm unmounted, Astrodon UBVRI John/Cousins",Photometry and Imaging system. Sensitive NABG CCD - susceptible to blooming artifacts from bright subjects,Telescope System Information and Specs
|
||||
T25,Deep Space,20.0,508,3454,f/6.8,Planewave CDK20,Corrected Dall-Kirkham,Player One Zeus 455M PRO,Mono CMOS,Sony IMX455,"36 x 24
|
||||
(Full Format)",251.9º,36.2,24.2,3.76,"0.23""",61.2,9576,6388,91%,71.6Ke,—,600,None,Planewave L-500,"Astrodon LRGB Gen2 I-Series Tru-Balance filters, Astrodon 3nm SII,Ha,OIII",Produces very large files,Telescope System Information and Specs
|
||||
T26,Deep Space,20.0,508,1537,f/3.0,Planewave Delta Rho 500,Advanced Corrected Cassegrain Focus,ASI6200MM Pro (mono),Mono CMOS,Sony IMX455,"36 x 24
|
||||
(Full Format)",181º,80.4,54,7.52 (Bin2),"1.01""",15.3,4788,3194,91%,51.4Ke,—,300,None,Planewave L-550 on Equatorial Wedge,"Chroma Filters:
|
||||
Wideband: Luminance, Red, Green & Blue
|
||||
Narrowband: SII, Ha & OIII with a 3nm optimise passband","Bin2 only due to current software limitations
|
||||
Recommended Exposures: LRGB: 30s-180s.
|
||||
Narrowband: 180s-300s. 900s Available",Telescope System Information and Specs
|
||||
T68,"One Shot Color
|
||||
(30 min free / day)",11.0,279,620,f/2.2,"Celestron RASA 11""",Rowe Ackerman Schmidt Astrograph,ZWO ASI2600 Color,"Color CMOS
|
||||
(RGGB Bayer)",Sony IMX571,"23.6 x 15.6
|
||||
(APS-C)",277º,130.2,87,3.76,"1.25""",26.1,6248,4176,>50%,—,—,240,Via Mount,Paramount ME II,None,"Full-Time Free Telescope System
|
||||
Large (26 MP, 16-bit) FITS files",Telescope System Information and Specs
|
||||
,Sierra Remote Observatory (MPC U69),,,,,,,,,,,,,,,,,,,,,,,,,,,
|
||||
T24,Deep Space,24.0,610,3962,f/6.5,Planewave CDK24,Corrected Dall-Kirkham ,Player One Zeus 455M PRO,Mono CMOS,—,36 x 24,90.7º,31.6,21.1,7.52 (Bin2),"0.395""",15.3,4788,3194,91%,71.6Ke,—,600,External Guiding (300s+),Planewave Ascension 200HR,"Astrodon LRGB2-E50S
|
||||
Astrodon HA3_50S, OIII3_50S, SII3_50S.Astrodon V, I (V*-50S, Ic*-50S)","Best results on Bin1. Dithering highly recommended. Uses RBI Flush to prevent ghosting. Best to use 60, 120, 180, 300, 600 and 900s exposures to match with calibraiton data.",Telescope System Information and Specs
|
||||
,"Siding Springs Observatory, Australia (MPC Q62)",,,,,,,,,,,,,,,,,,,,,,,,,,,
|
||||
T8,Wide Field,4.2,106,530,f/5.0,Takahashi FSQ ED,Petzval Apochromatic Refractor,FLI Microline 16803,CCD,—,36.8 x 36.8,358º,238.8,238.8,9,"3.5""",16.8,4096,4096,60%,100Ke,ABG,600,External ,Paramount PME,"AstroDon Series 2
|
||||
Luminance, Red, Green, Blue, EXO, Ha, SII, OIII, NIR Luminance",Northern view is restricted by observatory roof. N Horizon limit is 75°. Dithering is recommended because T8's CCD sometimes produces dark columns. ,Telescope System Information and Specs
|
||||
T17,Deep Field Astrophotography,17.0,432,2939,f/6.8,Planewave CDK17,Corrected Dall-Kirkham ,ASI6200MM Pro (mono),Mono CMOS,Sony IMX455,"36 x 24
|
||||
(Full Format)",84.2º,42.4,28.3,7.52 (Bin2),"0.531""",15.3,4788,3194,91% (475nm),51.4Ke,—,240,Unguided,Paramount PME,"Astrodon: Luminance, Clear
|
||||
Astrodon: Red-E. Green-E. Blue-E
|
||||
Astrodon: Ha 5nm, 5nm OIII, 5nm, SII","NEW CMOS Camera for astrophotography
|
||||
Bin2 only due to software limitations",Telescope System Information and Specs
|
||||
T30,Deep Space,20.0,508,"2262
|
||||
(0.66 reducer)",f/4.4,Planewave CDK20,Corrected Dall-Kirkham ,FLI-PL6303E,CCD,—,27.6 x 18.4,270º,41.6,27.8,9,"0.81""",6.3,3072,2048,68%,100Ke,NABG,300,Active Guiding Disabled,Planewave Ascension 200HR,"AstroDon Tru-Balance Gen 2 E series Luminance, Red, Green, Blue, 5nm Ha, 5nm SII, 5nm OIII, and AstroDon Johnson/Cousins UvBVRcIc",Very sensitive NABG CCD - susceptible to blooming artifacts from bright subjects,Telescope System Information and Specs
|
||||
T32,Wide Deep Field,17.0,431,2912,f/6.8,Planewave CDK17,Corrected Dall-Kirkham ,ASI6200MM Pro (mono),Mono CMOS,Sony IMX455,"36 x 24
|
||||
(Full Format)",90º,42.4,28.3,7.52 (Bin2),"0.53""",15.3,4788,3194,91% (475nm),51.4Ke,—,300,Active Guiding Disabled,Planewave Ascension 200HR,"Astrodon E-Series Luminance Red, Green, Blue
|
||||
Astrodon 5nm Ha, SII, OIII
|
||||
Astrodon Johnson/Couisins V, Ic","NEW CMOS Camera for astrophotography
|
||||
Bin2 only due to software limitations",Telescope System Information and Specs
|
||||
T33,"Narrow Deep Field
|
||||
(30 min free / day)",12.6,320,2885,f/9.0,"Star Instruments 12.5"" RCOS",Ritchey-Chrétien - Closed Carbon Tube,Apogee Alta U16,CCD,—,36.8 x 36.8,359º,37,37,9,"0.54""",16.8,4096,4096,69%,100Ke,NABG,300,External Guiding,Paramount ME,"Astrodon Series II: Luminance, Red, Green, Blue
|
||||
Astrodon Ha (5nm), SII, OIII (3nm)
|
||||
","Full-Time Free Telescope System
|
||||
North Horizon limit is 45°
|
||||
Rec. exposures: LRGB at 300s. Narrowband at 300s Bin2, or 600s Bin1 on calm nights. ",Telescope System Information and Specs
|
||||
T59,Wide Deep Field,20.1,510,3411,f/6.8,Planewave CDK20,Corrected Dall-Kirkham ,FLI Proline 16803,CCD,—,36.8 x 36.8,90º,37.2,37.2,9,"0.54""",16.8,4096,4096,60%,> 100X Saturation Exposure,ABG,900,Active Guiding Disabled,Planewave Ascension 200HR,"Astrodon E-Series Luminance Red, Green, Blue
|
||||
Astrodon 5nm Ha, SII, OIII
|
||||
Astrodon Johnson/Couisins, IcZ",Capable of very long (15 min) exposures,Telescope System Information and Specs
|
||||
,Deep Sky Chile (MPC X07),,,,,,,,,,,,,,,,,,,,,,,,,,,
|
||||
T70,Super Wide Field,2.6,65,129,f/3.5,Samyang 135 mm @ f/3.5,Camera Lens,ASI2600MM Pro (mono),Mono CMOS,Sony IMX571,"23.5 x 15.7
|
||||
(APS-C)",314º,469.8,355.2,3.76,"4.51""",26.1,6248,4176,60%,50Ke,—,300,ZWO 30 F/4 guidescope with Loadstar SX2,Paramount ME,"Astrodon Gen 2 E-Series LRGB, Ha, OIII, SII","Note: Camera lens. Some residual coma occurs in the corners, and bright stars develop halos. This is normal and expected on this system. ",Telescope System Information and Specs
|
||||
T71,Wide Field Astrophotography,7.1,180,500,f/2.8,Takahashi Epsilon 180ED,Hyperbolic Corrected Newtonian Astrograph,ASI2600MM Pro (mono),Mono CMOS,Sony IMX571,"23.5 x 15.7
|
||||
(APS-C)",342.5º,161.4,108,3.76,"1.55""",26.1,6248,4176,60%,50Ke,—,600,QHY miniguidescope f4.3 with Loadstar Pro,Paramount MyT,"Astrodon Gen 2 I-Series LRGB, Ha (5nm), OIII (5nm), SII (5nm)","Electronic shutter. No user dark frames can be taken. Calibrated data available for 10, 30, 60, 120 180, 300, 600s.
|
||||
|
||||
Generates very large (26 MP, 101 MiB) FITS files",Telescope System Information and Specs
|
||||
T72,Deep Space,20.1,510,3411,F/6.8,Planewave CDK20,Corrected Dall-Kirkham,FLI ML-16200,CCD,—,27 x 21.6,176º,26.93,21.53,6,"0.359""",16.2,4500,3600,60%,39Ke,ABG,600,None,PlaneWave L-500,"L,R,G,B,SII,Ha,OIII,U,V,B,R,I filters",Raw calibration frames can be found at data.itelescope.net. (Bias Bin1 & Bin2 and Darks 900s Bin1 & 2 are scaled with high precision for photometry calibrated image data from 0 to 900 seconds).,Telescope System Information and Specs
|
||||
T73,Deep Field Astrophotography,14.0,356,2563,f/7.2,Planewave CDK14,Corrected Dall-Kirkham,ASI2600MM Pro (mono),Mono CMOS,Sony IMX571,"23.5 x 15.7
|
||||
(APS-C)",179.6º,31.8,21,3.76,"0.31""",26.1,6248,4176,60%,50Ke,—,240,WO Guide Star 61 f5.9 guide scope with Starlight Xpress Ultrastar Pro (mono) guide camera,Paramount MEII,"Chroma LRGB, Chroma 3nm Ha, OIII, SII",(the ASI2600MM has an extremely low dark current making darks virtually redundant),Telescope System Information and Specs
|
||||
T74,,,,,,,,,,,,,,,,,,,,,,,,,,,,
|
||||
T75,Medium Deep Space,9.8,250,950,f/3.8,ASA N250,Newtownian Astrograph,ASI6200MM Pro (mono),Mono CMOS,Sony IMX455,"36 x 24
|
||||
(Full Format)",88.3º,137.4,91.8,7.52 (Bin2),"1.722""",15.3,4788,3194,91%,50Ke,—,600,ZWO 30 F/4 guide scope with ASI290MM mini,Paramount MyT,"Chroma LRGB, Chroma 3nm Ha, OIII, SII",Bin2 only due to current software limitations.,Telescope System Information and Specs
|
||||
,"AstroCamp Observatory, Spain (MPC I89)",,,,,,,,,,,,,,,,,,,,,,,,,,,
|
||||
T18,Medium Deep Space,12.5,318,1683,f/5.3,Planewave CDK12,Corrected Dall-Kirkham ,QHY600M-PH-US Mono,Mono CMOS,Sony IMX455,"36 x 24
|
||||
(Full Format)",150º,73.6,49.1,7.52 (Bin2),"0.92"" (Bin2)",15.3,4788,3194,87%,> 38Ke,—,300,External via Lodestar SX and 300mm guidescope,Paramount PME,"Astrodon Series E LRGB. Astrodon 5nm Ha, SII, OIII. Photometric V (Custom Scientific Bessell) and Ic (Astrodon John/Cousins)","Bin2 only due to current software limitations.
|
||||
SONY Full Frame BSI CMOS Sensor IMX455",Telescope System Information and Specs
|
||||
,"Entre Encinas y Estrellas, Spain",,,,,,,,,,,,,,,,,,,,,,,,,,,
|
||||
T80,Super Wide Field,2.6,65,129,f/3.5,Samyang 135 mm @ f/3.5,Camera Lens,ASI2600MM Pro P25 (mono),Mono CMOS,Sony IMX571,"23.5 x 15.7
|
||||
(APS-C)",268º,622.2,415.8,3.76,"5.98""",26.1,6248,4176,60%,50Ke,—,300,ZWO 30 F/4 guidescope with Loadstar SX2 ,Paramount MyT,"Astrodon Gen 2 E-Series LRGB, Ha, OIII, SII",Note: Camera lens. Some residual coma occurs in the corners,Telescope System Information and Specs
|
||||
|
100
itelescope/plans/README.md
Normal file
100
itelescope/plans/README.md
Normal file
|
|
@ -0,0 +1,100 @@
|
|||
# Observing plans and the T33 session runbook
|
||||
|
||||
ACP observing plans for iTelescope scopes, plus the procedure to run one on T33
|
||||
(the free Siding Spring scope). Credentials are NOT in this repo: they live in
|
||||
the local claudetemp itelescope folder (creds.txt, `username=`/`password=` lines).
|
||||
|
||||
## Plan format (ACP)
|
||||
|
||||
See [ngc104-test.txt](ngc104-test.txt). Directives, then a target line:
|
||||
`Name<TAB>RA_decimal_hours<TAB>Dec_decimal_degrees`. Counts, intervals, binning
|
||||
and filters are parallel comma-separated lists. `#shutdown` parks safely at the
|
||||
end (iTelescope's own one-click plans do the same).
|
||||
|
||||
## T33 endpoints (base http://t33.itelescope.net:8033, HTTP auth = iTelescope creds)
|
||||
|
||||
| Purpose | Path |
|
||||
|---|---|
|
||||
| Status JSON (times, obsStat, obsOwner) | /ac/SystemStatus/asystemstatus.asp |
|
||||
| Console text | /ac/SystemStatus/aconsread.asp |
|
||||
| Scope connect control | /ac/SystemStatus/ascopeconn.asp |
|
||||
| Shutter/roof status | /ac/SystemStatus/ashutterctl.asp |
|
||||
| My plan folder (list/upload/delete) | /plans/qisback/aindex.asp, aupload.asp, adelfile.asp |
|
||||
| Run a plan ("Acquire Images") | POST /ac/Plans/plan.asp |
|
||||
| My logs | /logs/qisback/aindex.asp |
|
||||
| Finished data | data.itelescope.net |
|
||||
|
||||
Upload: multipart POST to `/plans/qisback/aupload.asp`, fields `File1` (the file)
|
||||
and `DestPath=/plans/qisback`. Verified working 2026-07-18; content round-trips
|
||||
exactly.
|
||||
|
||||
Run: the web UI posts the plan select to `/ac/Plans/plan.asp`; the select's value
|
||||
is the WINDOWS path `C:\ProgramData\ACP\ACP Web Data\Doc Root\plans\qisback\<file>`.
|
||||
Field names seen: `plan`, optional `VPhot`, `AutoLogoff`. NOT yet exercised live
|
||||
(observatory was closed, daytime); the first live session must confirm whether a
|
||||
scope-connect POST (ascopeconn.asp) is required first, and capture the exact
|
||||
response shape.
|
||||
|
||||
## The 47 Tuc free-session test (ngc104-test.txt)
|
||||
|
||||
- Target: NGC 104 / 47 Tucanae, RA 0.4015 h, Dec -72.0814 deg (circumpolar at SSO).
|
||||
- L 4x120 s, RGB 2x90 s each, Bin2: about 17 min exposure, about 24 min with
|
||||
overhead, inside the daily free 30 minutes.
|
||||
- Uploaded to /plans/qisback/ on 2026-07-18 and verified.
|
||||
|
||||
### When to run
|
||||
|
||||
47 Tuc clears T33's 20 degree minimum elevation in the second half of the SSO
|
||||
night. SSO local = UTC+10; the good window is roughly 14:00-19:30 UTC (UK
|
||||
afternoon/evening). Sunrise at SSO was 06:14 local (20:14 UTC) at recon time;
|
||||
stop well before dawn.
|
||||
|
||||
### Procedure
|
||||
|
||||
1. GET asystemstatus.asp: confirm observatory open (obsStat) and no other user
|
||||
(obsOwner n/a). If someone is on, wait and retry; T33 is first-come.
|
||||
2. Confirm the plan file is still in /plans/qisback/ (aindex.asp).
|
||||
3. POST plan.asp with the plan's Windows path to start acquisition.
|
||||
4. Poll aconsread.asp (console) every minute or two: slew, centering, filter
|
||||
changes, exposures. The run self-terminates via #shutdown.
|
||||
5. Images land in /images/qisback/ on the scope server and then on
|
||||
data.itelescope.net; logs in /logs/qisback/.
|
||||
6. Record the session outcome in state/NOTES.md.
|
||||
|
||||
Abort path if something looks wrong: the web UI exposes an abort on the console
|
||||
page; locate it live before starting exposures (not yet mapped).
|
||||
|
||||
## Reservations (verified working 2026-07-18)
|
||||
|
||||
Reservations live at http://reservations.itelescope.net ("Reservations Pilot"),
|
||||
reached from each scope's /ac/MenuItems/reservation-edit.asp iframe as
|
||||
`?t=<scope-id>&u=<username>` (scope ids look like GRAS059 for T59, GRAS033 for
|
||||
T33; full list in the resources JSON on go.itelescope.net/Reservation/Overview.aspx,
|
||||
whose embedded DayPilot events also show everyone's bookings, roof/sun times, and
|
||||
the moon discount per night). No separate login: it trusts the u= parameter once a
|
||||
session cookie exists.
|
||||
|
||||
Creating one is a three-step WebForms dance against
|
||||
`New.aspx?start=<ISO local>&end=<ISO local>&r=<scope-id>` (times are OBSERVATORY
|
||||
LOCAL): (1) GET the form, (2) POST tokens + DropDownStartTime/DropDownEndTime
|
||||
(e.g. "12:05 AM"/"3:45 AM") + PlanToRunListBox=<plan file> + RescheduleCheckbox
|
||||
+ ButtonRefreshPlans=Refresh Plans, which re-renders with Confirm enabled,
|
||||
(3) re-POST the fresh tokens with the same fields + ReservationOKButton=Confirm
|
||||
Reservation. Success = response script `ModalStatic.result("OK")` AND the booking
|
||||
appearing in the grid: the modal also says "OK" on silent failure, so ALWAYS
|
||||
re-fetch the grid and look for the reservation id + username.
|
||||
|
||||
Availability probing (2026-07-21): a plain GET of
|
||||
`New.aspx?start=...&end=...&r=...` is a cheap, side-effect-free conflict check.
|
||||
The form comes back with the two time dropdowns populated for +/-60 min around
|
||||
the requested times, and if the slot collides with someone else's booking it
|
||||
also renders "Conflicting reservation. Start time must be later than H:MM AM".
|
||||
No message plus a full pair of dropdowns means the window is clear. This beats
|
||||
reading the DayPilot grid, whose event divs do not survive a plain
|
||||
Invoke-WebRequest fetch (they are rendered client-side).
|
||||
|
||||
Rules learned: maximum reservation length 4:00; recommended duration 1.5x total
|
||||
imaging time; the attached plan is auto-started by iTelescope at reservation
|
||||
start (no walk-in POST needed); RescheduleCheckbox auto-rebooks the identical
|
||||
timeslot on the first available night of the next 30 if the run does not happen.
|
||||
Delete/edit via Edit.aspx?id=<reservation id> from the grid.
|
||||
12
itelescope/plans/catspaw-t8.txt
Normal file
12
itelescope/plans/catspaw-t8.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; Cat Paw NGC 6334 in Ha on T8 - phase 2 narrowband
|
||||
; Ha 9x600s Bin1. 90 min imaging. Bright moon OK.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 9
|
||||
#interval 600
|
||||
#binning 1
|
||||
#filter Ha
|
||||
NGC6334 17.340000 -36.116667
|
||||
#shutdown
|
||||
12
itelescope/plans/cena-t32.txt
Normal file
12
itelescope/plans/cena-t32.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; Centaurus A (NGC 5128) on T32 for qisback - drain campaign phase 1
|
||||
; L 12x300s, RGB 4x300s each. 120 min imaging.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 12,4,4,4
|
||||
#interval 300,300,300,300
|
||||
#binning 2,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
NGC5128 13.424333 -43.019139
|
||||
#shutdown
|
||||
12
itelescope/plans/cra-t8.txt
Normal file
12
itelescope/plans/cra-t8.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; Corona Australis dust complex on T8 for qisback - drain campaign phase 1
|
||||
; L 8x300s Bin1, RGB 5x300s each Bin2. 115 min imaging.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 8,5,5,5
|
||||
#interval 300,300,300,300
|
||||
#binning 1,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
CrA-complex 19.030000 -36.955000
|
||||
#shutdown
|
||||
17
itelescope/plans/hdrcore-t32.txt
Normal file
17
itelescope/plans/hdrcore-t32.txt
Normal file
|
|
@ -0,0 +1,17 @@
|
|||
;
|
||||
; Centaurus A (NGC 5128) HDR core set on T32 for qisback - drain campaign
|
||||
; Companion to cena-t32.txt (2026-07-21, 24x300s LRGB BIN2), whose nucleus is
|
||||
; saturated: the core reaches 65313 ADU in a single 300s luminance sub.
|
||||
; This is the short-exposure ladder to blend under that core.
|
||||
; L 8x60s, 8x15s, 8x5s spans a 60x range below 300s; RGB 5x30s gives the
|
||||
; nucleus colour. BIN2 throughout so the frames register to the deep stack
|
||||
; without rescaling. 18.2 min imaging total.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 8,8,8,5,5,5
|
||||
#interval 60,15,5,30,30,30
|
||||
#binning 2,2,2,2,2,2
|
||||
#filter Luminance,Luminance,Luminance,Red,Green,Blue
|
||||
NGC5128 13.424333 -43.019139
|
||||
#shutdown
|
||||
12
itelescope/plans/ngc104-test.txt
Normal file
12
itelescope/plans/ngc104-test.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; 47 Tucanae (NGC 104) free-session test plan for qisback
|
||||
; L 4x120s, RGB 2x90s each, Bin2. ~17 min exposure, ~24 min with overhead.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 4,2,2,2
|
||||
#interval 120,90,90,90
|
||||
#binning 2,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
NGC104 0.401500 -72.081389
|
||||
#shutdown
|
||||
12
itelescope/plans/ngc6188-haoiii-t59.txt
Normal file
12
itelescope/plans/ngc6188-haoiii-t59.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; NGC 6188 Fighting Dragons on T59, session A: Ha + OIII - phase 2 narrowband
|
||||
; Ha 6x600s, OIII 6x600s. 120 min imaging. Bright moon OK.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 6,6
|
||||
#interval 600,600
|
||||
#binning 1,1
|
||||
#filter Ha,OIII
|
||||
NGC6188 16.669167 -48.796667
|
||||
#shutdown
|
||||
12
itelescope/plans/ngc6188-sii-t59.txt
Normal file
12
itelescope/plans/ngc6188-sii-t59.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; NGC 6188 on T59, session B: SII + extra Ha - phase 2 narrowband
|
||||
; SII 6x600s, Ha 3x600s. 90 min imaging. Bright moon OK.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 6,3
|
||||
#interval 600,600
|
||||
#binning 1,1
|
||||
#filter SII,Ha
|
||||
NGC6188 16.669167 -48.796667
|
||||
#shutdown
|
||||
13
itelescope/plans/ngc6744-t59.txt
Normal file
13
itelescope/plans/ngc6744-t59.txt
Normal file
|
|
@ -0,0 +1,13 @@
|
|||
;
|
||||
; NGC 6744 paid session on T59 for qisback
|
||||
; L 15x300s Bin1, RGB 7x300s each Bin2.
|
||||
; 180 min imaging = ~240 pts at Plan-40 rate 80/hr before moon discount.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 15,7,7,7
|
||||
#interval 300,300,300,300
|
||||
#binning 1,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
NGC6744 19.162833 -63.857500
|
||||
#shutdown
|
||||
12
itelescope/plans/ngc6752.txt
Normal file
12
itelescope/plans/ngc6752.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; NGC 6752 (Pavo globular) free-session plan for qisback
|
||||
; L 4x120s, RGB 2x90s each, Bin2. ~17 min exposure, ~24 min with overhead.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 4,2,2,2
|
||||
#interval 120,90,90,90
|
||||
#binning 2,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
NGC6752 19.181111 -59.984444
|
||||
#shutdown
|
||||
12
itelescope/plans/scorpius-t70.txt
Normal file
12
itelescope/plans/scorpius-t70.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; Scorpius tail super-wide (Prawn/Cat Paw region) on T70 for qisback - phase 1
|
||||
; L 10x300s, RGB 4x300s each. 110 min imaging.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 10,4,4,4
|
||||
#interval 300,300,300,300
|
||||
#binning 1,1,1,1
|
||||
#filter Luminance,Red,Green,Blue
|
||||
Scorpius-tail 16.916667 -40.000000
|
||||
#shutdown
|
||||
12
itelescope/plans/smc47tuc-t8.txt
Normal file
12
itelescope/plans/smc47tuc-t8.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; SMC + 47 Tucanae in one T8 frame - phase 3 signature shot
|
||||
; L 8x300s Bin1, RGB 6x300s each Bin2. 130 min imaging. Dark of moon.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 8,6,6,6
|
||||
#interval 300,300,300,300
|
||||
#binning 1,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
SMC-47Tuc 0.650000 -72.500000
|
||||
#shutdown
|
||||
12
itelescope/plans/tarantula-t32.txt
Normal file
12
itelescope/plans/tarantula-t32.txt
Normal file
|
|
@ -0,0 +1,12 @@
|
|||
;
|
||||
; Tarantula Nebula NGC 2070 on T32 - phase 3
|
||||
; L 10x300s, RGB 5x300s each. 125 min imaging. Pre-dawn rising target.
|
||||
;
|
||||
#largepreviews
|
||||
#tiff
|
||||
#count 10,5,5,5
|
||||
#interval 300,300,300,300
|
||||
#binning 2,2,2,2
|
||||
#filter Luminance,Red,Green,Blue
|
||||
NGC2070 5.643333 -69.100000
|
||||
#shutdown
|
||||
Loading…
Add table
Add a link
Reference in a new issue