[Aavso-photometry] FITS and observation time
Jeff Hopkins
phxjeff at hposoft.com
Wed Aug 1 14:35:07 EDT 2007
Hello Arne,
I did more testing with the DSI Pro and AutoStar to better understand
how to get more precise timing information.
Observation Time Test
# Exp Exp Time Start Stop Info Box FITS Header
10 15 sec 05:40 08:25 10 Images 163 sec Time 05:56
10 images
16 sec from end of first frame 150 sec
20 30 sec 12:50 23:18 20 Images 627 sec Time 13:21
20 Images
31 sec from end of first frame 600 sec
10 30 sec 27:00 32:30 10 Images 328 sec Time 27:46
10 Images
46 sec from end of first frame 300 sec
20 30 sec 34:00 44:29 20 Images 627 sec Time 34:32
20 Images
32 sec from end of first frame 600 sec
Note: Start and Stop times are mm:ss.
For single exposures
Exposure Info Box
15.0 sec 17 sec
11.3 sec 13 sec
8.1 sec 10 sec
5.7 sec 7 sec
4.0 sec 6 sec
2.8 sec 4 sec
2.0 sec 3 sec
1.4 sec 3 sec
1.0 sec 2 sec
0.7071 sec 2 sec
0.5 sec 2 sec
0.3536 sec 1 or 2 sec
Same for all faster times
Times are +/- 1 second
It seems the actual times can only be known to 1 or 2 seconds and
times can vary I think due to processing activities of the computer.
For stacked images it appears the best time estimate would be to take
the time reported in the FITS header, subtract the individual
exposure time then add one half the total exposure time reported in
the FIS Header.
For example 20 - 30 second stacked exposures. The FITS Header time is
hh:13:21 (note the hours are not used here to simplify things). The
Total FITS Header exposure time is 600 seconds. The time of
mid-observation would be approximately
hh:13:21 (780 seconds) - 30 + 600/2 = 750 + 300 = 1050 seconds or hh:17:30
I'd be very interested in any comments or suggestions. I have sent a
request to Meade to allow more control over the time reported and to
report in hh:mm:ss.ss instead of just hh:mm:ss.
Jeff
At 09:42 -0700 07/26/2007, arne wrote:
>Jeff Hopkins wrote:
>> Normally I observe long period eclipsing binaries where precise time
>> to the second or millisecond is not a factor. Recently I have started
>> a mentor project using the fast eclipsing binary sz Herculis. I am
>> using AutoStar and found the FITS time indication is off. It seems to
>> be the time the file is saved. I started a one-shot 15 second
>> exposure at 05:02:30. The end time should have been 05:02:45 or
>> close. The FITS Header indicated 05:02:57.
>>
>> If the difference is fairly constant, it could be compensated for.
>> However, things get more complex when images are stacked and during
>> the stacking when some images are not stacked due to poor quality.
>>
>> How has this been handled by the AAVSO?
>>
>The AAVSO assumes that the submitted time is for the midpoint of
>the exposure. Calculating this correctly is left up to the observer.
>
>Not quite sure how you would get 05:02:57 from your above example.
>Does Autostar take 12 seconds to download the image? Certainly
>the written time cannot reflect the end-time of writing an image
>since the header gets written first.
>
>Most software packages modify the header time when stacking
>images. There was an extensive discussion about this a couple
>of years ago on this list, but I'd presume that each software
>package writes things differently today.
>Arne
>_______________________________________________
--
Jeff Hopkins
HPO SOFT
Counting Photons
http://www.hposoft.com/Astro/astro.html
Hopkins Phoenix Observatory
7812 West Clayton Drive
Phoenix, Arizona 85033-2439 U.S.A.
(623)849-5889
(623) 247-1190 (Fax)
www.hposoft.com
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