Compare commits
No commits in common. "main" and "campaign-ledger-2026-07-21" have entirely different histories.
main
...
campaign-l
5 changed files with 0 additions and 86 deletions
29
CAMPAIGN.md
29
CAMPAIGN.md
|
|
@ -80,7 +80,6 @@ actual bill, and treat any not-yet-observed scope's card rate as +/-60%.
|
||||||
| 749230 | T8 | 26 Jul | 21:35-23:55 | catspaw-t8.txt | ~146 (25% moon disc.) | still booked |
|
| 749230 | T8 | 26 Jul | 21:35-23:55 | catspaw-t8.txt | ~146 (25% moon disc.) | still booked |
|
||||||
| 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 |
|
| 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 |
|
||||||
| (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 |
|
| (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 |
|
||||||
| (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 |
|
|
||||||
| 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) |
|
| 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) |
|
||||||
|
|
||||||
The T33 first-light test is now on its THIRD booking (749314); the two prior free
|
The T33 first-light test is now on its THIRD booking (749314); the two prior free
|
||||||
|
|
@ -103,34 +102,6 @@ Verify every booking via Edit.aspx?id= probing (sequential ids), NOT the grid.
|
||||||
| 5 | GRAS008 | 2026-08-08T02:35:00 | 2026-08-08T06:05:00 | 2:35 AM | 6:05 AM | smc47tuc-t8.txt | ~390 |
|
| 5 | GRAS008 | 2026-08-08T02:35:00 | 2026-08-08T06:05:00 | 2:35 AM | 6:05 AM | smc47tuc-t8.txt | ~390 |
|
||||||
| 6 | GRAS032 | 2026-08-09T03:05:00 | 2026-08-09T06:05:00 | 3:05 AM | 6:05 AM | tarantula-t32.txt | ~365 |
|
| 6 | GRAS032 | 2026-08-09T03:05:00 | 2026-08-09T06:05:00 | 3:05 AM | 6:05 AM | tarantula-t32.txt | ~365 |
|
||||||
| 7 | (T70, blocked: server unreachable) | night TBD before 5 Aug | ~2.5h | | | scorpius-t70.txt (in scratch, re-upload needed) | ~238 |
|
| 7 | (T70, blocked: server unreachable) | night TBD before 5 Aug | ~2.5h | | | scorpius-t70.txt (in scratch, re-upload needed) | ~238 |
|
||||||
| 8 | WITHDRAWN: booked then cancelled 2026-07-21, premise was wrong (see below) | | | | | hdrcore-t32.txt | 0 |
|
|
||||||
|
|
||||||
### CORRECTION (2026-07-21): the Cen A nucleus was never saturated
|
|
||||||
|
|
||||||
An earlier entry here claimed the 21 Jul Cen A data came back with a saturated
|
|
||||||
nucleus, and booked a short-exposure core set on that basis. **The claim was
|
|
||||||
wrong and the booking has been cancelled without running, at a cost of zero
|
|
||||||
points.**
|
|
||||||
|
|
||||||
The 65313 ADU figure came from taking the maximum pixel inside a 300 x 300 px
|
|
||||||
box centred on the frame. That measures the brightest thing near the middle of
|
|
||||||
the image, which is not the same as measuring the galaxy: it was a foreground
|
|
||||||
star 128 px (69 arcsec) from the nucleus, sitting inside the box. Median
|
|
||||||
filtering the inner 800 x 800 px to remove stars leaves the galaxy peaking at
|
|
||||||
**1944 ADU**, about a thirtieth of the clip level, with **not one star-free
|
|
||||||
pixel above 30000 ADU**. The core looked blown in the first processed image
|
|
||||||
because of the display stretch, whose white point was set by field stars, and
|
|
||||||
re-rendering the same data with a second tone curve scaled to the galaxy
|
|
||||||
recovered it fully.
|
|
||||||
|
|
||||||
**The habit that IS worth keeping, in corrected form:** before booking extra
|
|
||||||
time to fix a saturated core, *measure whether it is saturated* - median-filter
|
|
||||||
the inner region to remove stars first, and check where the frame's bright
|
|
||||||
pixels actually are. The check costs a minute. 47 Tuc and the SMC (queue #5)
|
|
||||||
may still genuinely saturate, a dense cluster core being the fastest thing there
|
|
||||||
is to clip, so run the same measurement on their data before assuming either
|
|
||||||
way. plans/hdrcore-t32.txt stays in the repo (and on T32) as a ready-made
|
|
||||||
ladder if one of them turns out to need it.
|
|
||||||
|
|
||||||
### Session 2026-07-21 ~08:55 UTC (booking round run early, before Cen A ran)
|
### Session 2026-07-21 ~08:55 UTC (booking round run early, before Cen A ran)
|
||||||
|
|
||||||
|
|
|
||||||
11
CLAUDE.md
11
CLAUDE.md
|
|
@ -1,14 +1,3 @@
|
||||||
> [!IMPORTANT]
|
|
||||||
> **This repository has moved.** Since 2026-07-21 it lives on as the
|
|
||||||
> `itelescope/` directory of
|
|
||||||
> **[astrophotography](https://git.discworld.casa/laurence/astrophotography)**,
|
|
||||||
> merged with the processing pipeline. Both histories were preserved.
|
|
||||||
>
|
|
||||||
> **Do new work there, not here.** This copy is kept read-only-in-spirit until
|
|
||||||
> the drain campaign closes (10-12 Aug 2026), because sessions are running most
|
|
||||||
> nights and nothing should break mid-campaign. Anything committed here after
|
|
||||||
> the merge will be stranded.
|
|
||||||
|
|
||||||
# Default Workflow
|
# Default Workflow
|
||||||
|
|
||||||
This file is the entry point for any Claude Code session working under the Default
|
This file is the entry point for any Claude Code session working under the Default
|
||||||
|
|
|
||||||
11
README.md
11
README.md
|
|
@ -1,14 +1,3 @@
|
||||||
> [!IMPORTANT]
|
|
||||||
> **This repository has moved.** Since 2026-07-21 it lives on as the
|
|
||||||
> `itelescope/` directory of
|
|
||||||
> **[astrophotography](https://git.discworld.casa/laurence/astrophotography)**,
|
|
||||||
> merged with the processing pipeline. Both histories were preserved.
|
|
||||||
>
|
|
||||||
> **Do new work there, not here.** This copy is kept read-only-in-spirit until
|
|
||||||
> the drain campaign closes (10-12 Aug 2026), because sessions are running most
|
|
||||||
> nights and nothing should break mid-campaign. Anything committed here after
|
|
||||||
> the merge will be stranded.
|
|
||||||
|
|
||||||
# itelescope
|
# itelescope
|
||||||
|
|
||||||
Reference and review of the [iTelescope.net](https://www.itelescope.net/) remote
|
Reference and review of the [iTelescope.net](https://www.itelescope.net/) remote
|
||||||
|
|
|
||||||
|
|
@ -1,17 +0,0 @@
|
||||||
;
|
|
||||||
; 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
|
|
||||||
|
|
@ -42,24 +42,6 @@
|
||||||
two prior free reservations (749228, 749229) expired unused with reschedule=No;
|
two prior free reservations (749228, 749229) expired unused with reschedule=No;
|
||||||
if 749314 also fails to run, stop rebooking and either walk it in (POST
|
if 749314 also fails to run, stop rebooking and either walk it in (POST
|
||||||
plan.asp per plans/README.md) or drop the free objective.
|
plan.asp per plans/README.md) or drop the free objective.
|
||||||
- The T32 HDR core set (plans/hdrcore-t32.txt) was booked and then CANCELLED on
|
|
||||||
2026-07-21 without running: the Cen A nucleus is not saturated, the earlier
|
|
||||||
claim having measured a foreground star. See the correction in CAMPAIGN.md.
|
|
||||||
Zero points spent. The plan file remains available on T32 if a genuinely
|
|
||||||
saturated target turns up.
|
|
||||||
- The 21 Jul Cen A data has been fully processed off-repo, in the user's
|
|
||||||
Downloads\NGC5128\20260721\stacked folder: masters, plate solution (0.27
|
|
||||||
arcsec on 237 stars), an LRGB composite, a globular cluster survey (289
|
|
||||||
candidates, 62% catalogue-confirmed, density falling 10.5x outward), surface
|
|
||||||
photometry (Sersic n = 4.27, Re = 400 arcsec, total G = 6.56, which matches
|
|
||||||
the catalogued brightness and so validates the photometric chain), and a
|
|
||||||
transient/moving-object search (both null, with measured limits). METHODS.md
|
|
||||||
there documents the lot. Nothing from that analysis needs to come back into
|
|
||||||
this repo, but two results affect FUTURE sessions and are recorded here:
|
|
||||||
**(a)** measure saturation properly before buying short subs, and **(b)** the
|
|
||||||
faint outer halo in that stack is limited by the sky-plane subtraction
|
|
||||||
(-17.9 ADU/px of real halo light absorbed), not by exposure time, so more
|
|
||||||
integration alone would not have gone deeper.
|
|
||||||
- CrA on T8 runs 11:45-14:45 UTC 22 Jul. Verify after 14:45 UTC: images under
|
- CrA on T8 runs 11:45-14:45 UTC 22 Jul. Verify after 14:45 UTC: images under
|
||||||
/images/qisback/T8/ on t8.itelescope.net:8008, then the actual bill from
|
/images/qisback/T8/ on t8.itelescope.net:8008, then the actual bill from
|
||||||
account/history.aspx into the ledger. This is the first T8 bill, so it also
|
account/history.aspx into the ledger. This is the first T8 bill, so it also
|
||||||
|
|
|
||||||
Loading…
Add table
Add a link
Reference in a new issue