Observing session

Andromeda from both sides of the sky, the Pleiades and Saturn

The polar alignment I thought was 0.2 degrees was really 3, the camera's short exposures got fixed, and an hour and a half of Andromeda came out of two runs stitched across the meridian.

Andromeda Galaxy Pleiades Saturn Polar alignment Stacking Hardware telescopeyoke

The Andromeda Galaxy's bright core with dark dust lanes sweeping across below it, and the companion M32 at top left (opens larger)

The Andromeda Galaxy, M31. 358 frames of 16 seconds, an hour and 35 minutes in all, from two runs either side of the meridian. M32 is at top left this time because the picture is the other way up from the last one.

Andromeda Galaxy (M31), from 23:26

Night
13 October: 23:26 to 00:48
Exposure
16 s each, gain 1,500
Frames
202 kept of 256Left out: 36 left out when stacked; 18 cloud
Integration
54 min
Star size FWHM
5.87 px median per frame (half of frames 5.81 to 5.93); 6.37″ across in the stack
Sky brightness
19.12 magnitudes per square arcsecond
Depth
stars to magnitude 17.915σ limit on open sky, inferred, Gaia G (camera unfiltered) band; 1,998 stars detected
Plate scale
1.32″ a pixel
Polar alignment
About 3° out, corrected to 0.1°noted
The night, frame by frame
00:00star size, 4.5 to 6.5 pxsky background, 103 to 162ticks: upper row kept, lower row left out
Each quarter hour of the night
FromFramesKeptStar size, px (median of kept)Sky background
23:2644335.91124
23:4148425.83114
23:5647425.88104
00:1148395.87104
00:2648395.86109
00:412175.78152
Where these numbers come from

Imported from telescopeyoke's session folder frames/M31/20261013-232632 on 2026-10-17. Values marked logged are read from these files and nothing else:

  • session.json sha256 d275115b2f615bd1…
  • frames.json sha256 f586f3b343264130…
  • restack.json sha256 e3154b2646fdcab1…
  • depth.json sha256 07985c7db38d6564…
  • final.jpg sha256 3a780c41db7baa38…

Frame counts and integration are telescopeyoke's restack record; the reasons are its own words for each frame it left out, grouped. Depth and sky brightness are from its photometry of the stack (depth.json). Times are local, start of the first frame to end of the last.

Pleiades (M45), from 01:23

Night
13 October: 01:23 to 02:00
Exposure
16 s each, gain 1,500
Frames
77 kept of 116Left out: 39 left out when stacked
Integration
21 min
Star size FWHM
5.48 px median per frame (half of frames 5.39 to 5.6)
The night, frame by frame
02:00star size, 5.2 to 6.2 pxsky background, 95 to 253ticks: upper row kept, lower row left out
Each quarter hour of the night
FromFramesKeptStar size, px (median of kept)Sky background
01:2346205.35115
01:3847375.60136
01:5323205.45130
Where these numbers come from

Imported from telescopeyoke's session folder frames/M45/20261014-012245 on 2026-10-17. Values marked logged are read from these files and nothing else:

  • session.json sha256 ecf2509716a6abcb…
  • frames.json sha256 9c9fc0dc7f89f2d8…
  • restack.json sha256 c465bc4e9965e98e…
  • final.jpg sha256 9e060e69ae991ab4…

Frame counts and integration are telescopeyoke's restack record; the reasons are its own words for each frame it left out, grouped. Depth and sky brightness are from its photometry of the stack (depth.json). Times are local, start of the first frame to end of the last.

Andromeda Galaxy (M31), from 02:11

Night
13 October: 02:11 to 03:43
Exposure
16 s each, gain 1,500
Frames
164 kept of 226Left out: 30 left out when stacked; 21 cloud; 6 sky brightened (cloud or a light); 5 stars trailed (wind or a knock)
Integration
44 min
Star size FWHM
5.85 px median per frame (half of frames 5.73 to 5.98); 6.6″ across in the stack
Sky brightness
18.72 magnitudes per square arcsecond
Depth
stars to magnitude 17.715σ limit on open sky, inferred, Gaia G (camera unfiltered) band; 1,761 stars detected
Plate scale
1.32″ a pixel
The night, frame by frame
03:00star size, 4.7 to 7.5 pxsky background, 68 to 340ticks: upper row kept, lower row left out
Each quarter hour of the night
FromFramesKeptStar size, px (median of kept)Sky background
02:1145395.84146
02:2638345.76152
02:4120186.01113
02:561996.00122
03:1148375.81126
03:2649275.83122
03:4170none kept79
Where these numbers come from

Imported from telescopeyoke's session folder frames/M31/20261014-021118 on 2026-10-17. Values marked logged are read from these files and nothing else:

  • session.json sha256 d275115b2f615bd1…
  • frames.json sha256 f240e7b119759e30…
  • restack.json sha256 87072c80c78211a4…
  • depth.json sha256 35eed0e8d18e10ff…
  • final.jpg sha256 4d0839041cb3478a…

Frame counts and integration are telescopeyoke's restack record; the reasons are its own words for each frame it left out, grouped. Depth and sky brightness are from its photometry of the stack (depth.json). Times are local, start of the first frame to end of the last.

Andromeda Galaxy (M31), both runs stacked

Stacked from
2 runs, starting 23:26, 02:11
Night
13 October: 23:26 to 03:43
Exposure
16 s each, gain 1,500
Frames
358 kept of 482
Integration
1 h 35 min
Star size FWHM
6.36″ across in the stack
Sky brightness
18.98 magnitudes per square arcsecond
Depth
stars to magnitude 17.925σ limit on open sky, inferred, Gaia G (camera unfiltered) band; 1,906 stars detected
Plate scale
1.32″ a pixel
Where these numbers come from

Imported from telescopeyoke's session folder frames/M31/combined on 2026-10-17. Values marked logged are read from these files and nothing else:

  • restack.json sha256 95d5e48dffcb7e71…
  • depth.json sha256 12193f90ab32b1b1…
  • final.jpg sha256 dfb254a5aae959f8…

Frame counts and integration are telescopeyoke's restack record; the reasons are its own words for each frame it left out, grouped. Depth and sky brightness are from its photometry of the stack (depth.json). Times are local, start of the first frame to end of the last.

The polar alignment was never 0.2°

On 6 October the software said the polar axis was 0.2° from the pole, but the mount still drifted badly. This time we found out why. Every time the handset does a GoTo, it nudges the other axis a little too, by a tenth of a degree or so. The software assumed only one axis had turned, and that tiny error threw its answer right off. Measured from the east side of the sky it said one thing, and from the west side something completely different.

Once Claude allowed for the nudge, both sides agreed: the axis was about 3° out, too high and too far east. A drift test, which just watches how fast the stars wander, said 3.2°. So every polar figure before tonight was wrong.

With the corrected measurement I got it down to 0.1°, and the stars’ drift across the picture fell to under a quarter of what it had been. One thing I learned about the mount: the rear altitude bolt is stiff. It will push the axis down, but to bring it back up I have to help it by hand. One full turn is about 2°.

The camera’s exposures, fixed

Since the first night the camera has been giving short exposures. Ask for 10 seconds and you get about 6.4. It turns out to depend on a “speed” setting in the camera’s driver, which sets how fast the picture is read off over USB. At the default speed it gives 0.63 of what is asked. Claude measured this with star trails: with the tracking off, a star draws a line whose length tells you exactly how long the shutter was open. The software now asks for the longer time that gives the exposure I want. A 10 second test came out at 9.6.

How long each picture

A friend who has been doing this for years said to go to 16 seconds. Claude checked first, with test frames from 2 to 16 seconds, and the stars stayed round all the way up. They get a bit bigger with longer exposures, but the gain in faint detail is worth it. All tonight’s runs were at 16 seconds.

Alerts in the living room

I don’t want to keep checking a laptop screen from the sofa, so the living room light now tells me how things are going:

The Google speaker says it out loud as well, when it can be found on the network, which is about half the time so far.

The targets

The bright stars of the Pleiades with long diffraction spikes and a faint blue haze around them (opens larger)

The Pleiades, M45. 113 frames, half an hour. The blue haze is dust the cluster is passing through, lit by its stars. The dark ring below the middle is dust on the camera.

Saturn with its rings tilted, small and soft (opens larger)

Saturn, at 750 mm with no Barlow lens, so it is tiny. The rings are clear, and the gap between them and the planet shows on both sides. A 2× Barlow and a faster way of capturing are next for planets.

Putting the two Andromeda runs together

When a mount like mine passes the meridian, the tube swings over to the other side and everything comes out upside down. The software is meant to spot those frames and turn them round. The first time we stacked the two runs, the galaxy came out twice, side by side. Only 8 of the 226 upside-down frames had been turned. In a field this full of stars, an upside-down frame still lines up with enough stars by chance to pass the check. Claude changed it to try the other way up whenever the fit is poor. The second time, all 228 were turned and the galaxy came out once, lined up to under a third of a pixel.

The two runs weren’t framed quite the same, so the edges only one of them covered came out as a lighter strip. The stacker now trims those edges off by itself.

The laptop went to sleep on battery at half five in the morning, partway through the first combining run. The PC in the house is far faster and is the right place for this kind of job, so that is next.

The bright core of the Andromeda Galaxy with dark dust lanes, and a small companion galaxy below
6 October 2026
The Andromeda Galaxy's bright core with dark dust lanes sweeping across below it, and the companion M32 at top left
13 October 2026
Andromeda Galaxy (M31) on two nights. Shown side by side because the two aren't on the same pixel grid; a slider between them would make the difference look like movement.