DeepSkyHosting

M101

Ananas
8100
Category:Deep Sky
Published:
536
M101NGC 5447NGC 5449NGC 5450NGC 5453NGC 5458NGC 5451NGC 5455NGC 5457NGC 5461NGC 5462NGC 5471NGC 5477
Resolution:
2817x2848 px
File size:
4585 KB

Technical information

Telescope/Lens
Sky-Watcher 150/750
Camera
ZWO ASI533MC Pro
Mount
Juwei 17
Guide Scope
ZWO Off-Axis Guider (OAG)
Guide Camera
ZWO ASI220MM
Accessories
Baader MPCC
Software
Siril
Location
Tokyo

Light pollution

White, Bortle 8/9 zone

Date taken

Exposure

  • 134 × 90″ · ISO/Gain: 101 · SVBONY UV/IR Cut ·

Total exposure: 3 h 21 m

Comments

yas
Are 90-second sub-exposures too long for this level of light pollution?
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AnanasReply to yas
It's hard to say. For bright objects, like Orion or Andromeda, 60 is definitely the upper limit. For fainter ones, like this, it looks optimal.
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yasReply to Ananas
The issue isn't overexposure of bright objects, but rather that under such conditions the sky background will be very high, causing faint objects to be lost.
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AnanasReply to yas
Makes sense, I'll have to experiment with it.
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yasReply to Ananas
If you use NINA, you can immediately determine the maximum exposure time for your conditions.
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AnanasReply to yas
I checked the histogram of the raw frames: in the evening, the exposure was clearly too long, yes. But by midnight, it already looks reasonable—10–15% from the left edge.
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yasReply to Ananas
The histogram doesn't tell you much. If you're comfortable with math, check out https://forums.sharpcap.co.uk/viewtopic.php?t=456. If not, here's a quick summary: you need to know: 1. The average bias for your camera settings, 2. The average background level for a given sub-exposure, 3. The camera read noise, 4. The conversion factor for your camera settings in e-/ADU. Recommended Exposure Time = 10 × (read noise)² / light pollution rate where light pollution rate is defined as: (median ADU of a subframe − median bias) × electrons per ADU / exposure length
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