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Originally posted by alfa1
Originally posted by abeverage
Anyone come up with any good explanation of this? To me an exposure is set and goes for how many seconds is requested and then a new image is created.
It is actually extraordinarily common in astronomical images to "stack" multiple frames on top of each other.
Actually more than normal, its standard practise.
Originally posted by nataylor
reply to post by abeverage
I posted this information earlier in the thread, but the three exposures with the F606W filter were combined into a single data set. Similarly, the two exposures with the F814W filter were combined into a single data set. You can see that in the first two lines of the table here: archive.stsci.edu...
The F606W data set has an exposure time of 1320 seconds, which is 3 exposures of 440 seconds. The F814W data set has an exposure time of 980 seconds, which is 2 exposures of 490 seconds.
hlsp_ison_hst_wfc3_130430_f606w-f814w_v1 is a combination of all 5 exposures. (You can tell because it has both the F606W and F814W filters in the name, so it must contain exposures taken with both those filters). The reason it is not a continuous streak of light is that the 5 exposures totaling 2300 seconds (38 minutes and 20 seconds) was actually taken over a period of 48 minutes and 24 seconds. You can see that on the page I linked to above that the start and stop times for the observations were 3:35:43 and 4:24:07, which is a duration of 48 minutes nd 24 seconds. So there was a total of 10 minutes and 4 seconds where imaging wasn't occurring, which is why you have breaks in the streak of light in that image.
Originally posted by abeverage
Originally posted by nataylor
reply to post by abeverage
I posted this information earlier in the thread, but the three exposures with the F606W filter were combined into a single data set. Similarly, the two exposures with the F814W filter were combined into a single data set. You can see that in the first two lines of the table here: archive.stsci.edu...
The F606W data set has an exposure time of 1320 seconds, which is 3 exposures of 440 seconds. The F814W data set has an exposure time of 980 seconds, which is 2 exposures of 490 seconds.
Ok, we are having some miscommunication here. I erroneously linked that data earlier and the images are not the same as on this page. or it is possible they were used in the 2 1320 and 980 exposures that doesn't matter.
Please show me the data for image below (hlsp_ison_hst_wfc3_130430_f606w-f814w_v1), it is not a multi-exposure image and still where some confusion is. I realize the curve is from the movement of the HST that was cleared up by you.
But what about the break up or dashes of light? Wouldn't a long exposure regardless of movement create a continuous blur of light?
This is the same image only with darkening the exposure. I am looking for a explanation in the drop of light in this image.
labeled hlsp_ison_hst_wfc3_130430_f606w-f814w_v1
Or explain the double dashes in image labeled hlsp_ison_hst_wfc3_130430_f814w_v1
And for comparison This is the 1320 second exposure stacked image you referenced known as IC7I11010 Found here
And this is the 980 exposure image known as IC7I11020 found here
You can tell those are multiple exposures because they (or the software) did a crappy stack overlay and you see ghosting...
Thank you.edit on 20-8-2013 by abeverage because: grammatical and frustration lol
Originally posted by abeverage
reply to post by nataylor
I'll ask again. Please link me to the data showing me the exposure times for lsp_ison_hst_wfc3_130430_f606w-f814w_v1
Thank you.edit on 20-8-2013 by abeverage because: (no reason given)
Originally posted by nataylor
reply to post by abeverage
I posted this information earlier in the thread, but the three exposures with the F606W filter were combined into a single data set. Similarly, the two exposures with the F814W filter were combined into a single data set. You can see that in the first two lines of the table here: archive.stsci.edu...
The F606W data set has an exposure time of 1320 seconds, which is 3 exposures of 440 seconds. The F814W data set has an exposure time of 980 seconds, which is 2 exposures of 490 seconds.
(Update: An earlier version of this story referred to this representation of Comet ISON as a color image assembled from subsequent exposures. This was erroneous: although the background is in color, ISON itself is taken from only one exposure and is therefore monochromatic.)
Originally posted by nataylor
Originally posted by abeverage
reply to post by nataylor
I'll ask again. Please link me to the data showing me the exposure times for lsp_ison_hst_wfc3_130430_f606w-f814w_v1
Thank you.edit on 20-8-2013 by abeverage because: (no reason given)
archive.stsci.edu...
The first two entires in that table show the observations made with the F606W and F814W filters.
Originally posted by nataylor
If you look up proposal 13229, which contained all the ISON data taken on April 30th, you can see if ISON-FIXED observations on page 5 you can see the alternating F606W and F814W filter exposures of 440 and 490 seconds total.There's even a nice little timeline on that page that shows the overhead time between exposures.
The reason it is not a continuous streak of light is that the 5 exposures totaling 2300 seconds
They're talking about the image on that page. This one:
Originally posted by NeoParadigm
Originally posted by nataylor
reply to post by abeverage
I posted this information earlier in the thread, but the three exposures with the F606W filter were combined into a single data set. Similarly, the two exposures with the F814W filter were combined into a single data set. You can see that in the first two lines of the table here: archive.stsci.edu...
The F606W data set has an exposure time of 1320 seconds, which is 3 exposures of 440 seconds. The F814W data set has an exposure time of 980 seconds, which is 2 exposures of 490 seconds.
We were discussing this comment,
(Update: An earlier version of this story referred to this representation of Comet ISON as a color image assembled from subsequent exposures. This was erroneous: although the background is in color, ISON itself is taken from only one exposure and is therefore monochromatic.)
hubblesite.org...
Why are they talking about only one exposure of ISON? Do they mean they only used one filter?
If this was already explained then I missed it.
Originally posted by nataylor
They're talking about the image on that page. This one:
Originally posted by NeoParadigm
Originally posted by nataylor
reply to post by abeverage
I posted this information earlier in the thread, but the three exposures with the F606W filter were combined into a single data set. Similarly, the two exposures with the F814W filter were combined into a single data set. You can see that in the first two lines of the table here: archive.stsci.edu...
The F606W data set has an exposure time of 1320 seconds, which is 3 exposures of 440 seconds. The F814W data set has an exposure time of 980 seconds, which is 2 exposures of 490 seconds.
We were discussing this comment,
(Update: An earlier version of this story referred to this representation of Comet ISON as a color image assembled from subsequent exposures. This was erroneous: although the background is in color, ISON itself is taken from only one exposure and is therefore monochromatic.)
hubblesite.org...
Why are they talking about only one exposure of ISON? Do they mean they only used one filter?
If this was already explained then I missed it.
That's a composite image where the stars are shown in color, by combining the exposure data with the various filters. The comet in that image is taken from only one of the 5 exposures taken.
Originally posted by NeoParadigm
Originally posted by nataylor
reply to post by abeverage
I posted this information earlier in the thread, but the three exposures with the F606W filter were combined into a single data set. Similarly, the two exposures with the F814W filter were combined into a single data set. You can see that in the first two lines of the table here: archive.stsci.edu...
The F606W data set has an exposure time of 1320 seconds, which is 3 exposures of 440 seconds. The F814W data set has an exposure time of 980 seconds, which is 2 exposures of 490 seconds.
We were discussing this comment,
(Update: An earlier version of this story referred to this representation of Comet ISON as a color image assembled from subsequent exposures. This was erroneous: although the background is in color, ISON itself is taken from only one exposure and is therefore monochromatic.)
hubblesite.org...
Why are they talking about only one exposure of ISON? Do they mean they only used one filter?
If this was already explained then I missed it.
Originally posted by abeverage
Even by your naming logic lsp_ison_hst_wfc3_130430_f606w-f814w_v1 would only be 2 images using the F606W filter and the F814W filter amounting to 880 seconds.edit on 20-8-2013 by abeverage because: (no reason given)
(Update: An earlier version of this story referred to this representation of Comet ISON as a color image assembled from subsequent exposures. This was erroneous: although the background is in color, ISON itself is taken from only one exposure and is therefore monochromatic.)
It's a total of 2300 seconds (three exposures of 440 seconds with the F606W filter and two exposures of 490 seconds with the F814W filter).
Originally posted by abeverage
reply to post by nataylor
So ntaylor how long was the exposure to lsp_ison_hst_wfc3_130430_f606w-f814w_v1?