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Hello all!
I recently got one of those led light boards to start taking flats with.
The first time I used it I didn't have camera connected to my computer so there was no way to monitor them. They turned out too bright with an exposure time of 1/4000...
This time I have my camera connected and APT running a flat plan. I dimmed the light board quite a bit and I'm using the white T-shirt method and my exposure time is now 1/125...
Attached is a screen shot of APT with the histogram. This histogram is similar to my light frames from last night. Are these good flats?
Thanks!
Larry
Attachments
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C
Thanks Tom!
I certainly can upload one but what exactly would you be looking for?
I thought you would judge the frame by the exposure time and histogram.
Larry
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C
Well we can look to see if any dust motes, vigenetting, etc. that should be in the image. Also inspect it for shutter shadows, light leaks, that sort of thing.
Cant really see that sort of thing with a snapshot of a screen display
Tom
Current Equipment:
Mount: Celestron CGX-L
Scope: 130mm f7 APO
Cam: ASI071mc-pro
I can pretty much guarantee that at 1/4000 and 1/125 of a second your flats are too dark. Don't measure your flats with the Backyard EOS histogram. Get another program that can measure the ADU of the flat--you're looking for 40% of your max ADU.
Personal equipment: TEC 140 F7 on Astro-Physics Mach 1 mount. Camera QSI 683ws7. Guide with Vario guiding scope
Shared equipment through Star Shadows Remote Observatory through PROMPT/ CTIO/Chile 16" RCOS 16803 chip
Shared equipment through San Diego Astronomy Society 14" RC with 16803 chip on a paramount
Software (for my stuff) PemPRO, SGP, PHD, Focus Boss, ASCOM, and Pixinsight on the other end.
Scopes: Explore Scientific ED102 APO, Sharpstar 61 EDPH II APO, Samyang 135 F2 (still on the Nikon).
Mount: Skywatcher HEQ5 Pro with Rowan Belt Mod
Stuff: ASI EAF Focus Motor (x2), ZWO OAG, ZWO 30 mm Guide Scope, ASI 220mm min, ASI 120mm mini, Stellarview 0.8 FR/FF, Sharpstar 0.8 FR/FF, Mele Overloock 3C.
Camera/Filters/Software: ASI 533 mc pro, ASI 120mm mini, ASI 220mm mini , IDAS LPS D-1, Optolong L-Enhance, ZWO UV/IR Cut, N.I.N.A., Green Swamp Server, PHD2, Adobe Photoshop CC, Pixinsight.
Dog and best bud: Jack
Sky: Bortle 6-7
My Astrobin: https://www.astrobin.com/users/Juno16/
I can easily delete these and take more once I know what I'm doing.
Larry
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C
Juno16 wrote: ↑Sat Feb 22, 2020 5:44 pm
AP Lab works great to measure flats ADU.
Thanks!
A search for AP lab didn't yield any useful results. Can you give me a link?
Larry
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C
Scopes: Explore Scientific ED102 APO, Sharpstar 61 EDPH II APO, Samyang 135 F2 (still on the Nikon).
Mount: Skywatcher HEQ5 Pro with Rowan Belt Mod
Stuff: ASI EAF Focus Motor (x2), ZWO OAG, ZWO 30 mm Guide Scope, ASI 220mm min, ASI 120mm mini, Stellarview 0.8 FR/FF, Sharpstar 0.8 FR/FF, Mele Overloock 3C.
Camera/Filters/Software: ASI 533 mc pro, ASI 120mm mini, ASI 220mm mini , IDAS LPS D-1, Optolong L-Enhance, ZWO UV/IR Cut, N.I.N.A., Green Swamp Server, PHD2, Adobe Photoshop CC, Pixinsight.
Dog and best bud: Jack
Sky: Bortle 6-7
My Astrobin: https://www.astrobin.com/users/Juno16/
Just got back from shopping with my wife.
Thanks Jim!
Larry
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C
ADU is Analog to Digital Units.
When a photon hits a photosite, depending on your quantum efficiency an electron will be produced and will be placed in the photosite. The number of electrons that each photosite can hold is called the Full Well Depth.
Once the shutter closes, and the well dumps its electrons, it gets converted into digital signal by an analog to digital converter. The output of the converter will be a number, called the ADU. Each camera has a bit depth by which the maximum ADU is expressed and because of how they are manufactured will be in some factorial of 2. So a regular CCD camera has a bit depth of 16 which is 2^16 with a max of 65,536. DSLRs generally have a bit depth of 14 which is 2^14 to a bit depth of 16,384. Ultimately it doesn't really matter as programs will rescale to whatever bit depth you want.
Flats should be taken so that about half the well depth is full of electrons. So assuming a 16 bit scale, with a max of 65,536, you should aim for a mean flat ADU of about 20,000-35,000. Anywhere in there is fine.
Many programs will measure your ADU on the fly--SGP does this and will tell you immediately without the need to export the file to another program. Backyard EOS (to my knowledge) does not and instead people rely on the histogram. For whatever reason this ALWAYS leads to flats that are way too dark.
Once you figure out how to measure a flat I recommend that you measure the mean ADU of a bias frame, and the mean ADU of a saturated frame. Your goal is about half way in between.
Personal equipment: TEC 140 F7 on Astro-Physics Mach 1 mount. Camera QSI 683ws7. Guide with Vario guiding scope
Shared equipment through Star Shadows Remote Observatory through PROMPT/ CTIO/Chile 16" RCOS 16803 chip
Shared equipment through San Diego Astronomy Society 14" RC with 16803 chip on a paramount
Software (for my stuff) PemPRO, SGP, PHD, Focus Boss, ASCOM, and Pixinsight on the other end.
Stuart wrote: ↑Sun Feb 23, 2020 12:15 am
ADU is Analog to Digital Units.
When a photon hits a photosite, depending on your quantum efficiency an electron will be produced and will be placed in the photosite. The number of electrons that each photosite can hold is called the Full Well Depth.
Once the shutter closes, and the well dumps its electrons, it gets converted into digital signal by an analog to digital converter. The output of the converter will be a number, called the ADU. Each camera has a bit depth by which the maximum ADU is expressed and because of how they are manufactured will be in some factorial of 2. So a regular CCD camera has a bit depth of 16 which is 2^16 with a max of 65,536. DSLRs generally have a bit depth of 14 which is 2^14 to a bit depth of 16,384. Ultimately it doesn't really matter as programs will rescale to whatever bit depth you want.
Flats should be taken so that about half the well depth is full of electrons. So assuming a 16 bit scale, with a max of 65,536, you should aim for a mean flat ADU of about 20,000-35,000. Anywhere in there is fine.
Many programs will measure your ADU on the fly--SGP does this and will tell you immediately without the need to export the file to another program. Backyard EOS (to my knowledge) does not and instead people rely on the histogram. For whatever reason this ALWAYS leads to flats that are way too dark.
Once you figure out how to measure a flat I recommend that you measure the mean ADU of a bias frame, and the mean ADU of a saturated frame. Your goal is about half way in between.
Thanks Stuart!
That's a lot to process. I'll get on it!
Larry
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C
I use an EL panel for my flats. I processed 3 of my flat frames (with 3 different exposure times 1/30, 1/15, 1/8) through AP Lab. It gave me the ADU level for each of these flat frames. All three did not measure up to half of my ADU full well depth. But I could see how much more signal each longer exposure gave. It was then easy to extrapolate a new exposure time which, as it turned out, put me right in the ballpark for the correct ADU reading for my flats (1/2 second). So as long as I use this camera through this telescope using my EL panel at the same illumination level I know the correct exposure time to use for my flats.
Hey,
I extracted the lightness and measured the mean ADU. It's 5324. Way too dark. It should be 25,000-30,000
Attachments
Personal equipment: TEC 140 F7 on Astro-Physics Mach 1 mount. Camera QSI 683ws7. Guide with Vario guiding scope
Shared equipment through Star Shadows Remote Observatory through PROMPT/ CTIO/Chile 16" RCOS 16803 chip
Shared equipment through San Diego Astronomy Society 14" RC with 16803 chip on a paramount
Software (for my stuff) PemPRO, SGP, PHD, Focus Boss, ASCOM, and Pixinsight on the other end.
Thanks!
I'll work on it tomorrow.
I shot M44 and M86 last night and I had a tough time processing them. I suspected the flat frames. I'm shooting them again tonight and will try to get the flats sorted and reprocess it all.
Larry
For visual:
10" Skywatcher collapsible goto dob, various EP's and a Celestron StarSense auto align.
For imaging:
Orion 8" astrograph 800mm @ F3.9
Eq6-R Pro controlled by APT via EQmod with an OTA mounted mini PC
Tele Vue Paracorr Type 2 coma corrector
Altair Hypercam 26C