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ASTRO: ML4022 first light and some "interesting objects" in the image
A consulting project I have been involved in for some time recently needed a
KAI4022 based camera for some quantitative optical studies so we ended up purchasing an FLI Microline 4022 camera This past weekend I decided to use the camera for astronomy, not having used the KAI series very much in the past. I picked the AP180EDT f/9 for using it, since it was set up in the backyard with the Proline 9000 and filters already. I just replaced the camera with the Microline and shot I ended up imaging vdB142, a familiar object I have imaged many times using emission line filters and an object in a good part of the sky at sundown. the 7.4 micron pixels of the microline give me 0.94 arc-sec/pixel at the 1620 mm focal length and that's a nice image scale for the seeing conditions. They are a bit slow in the red filters due to the lower QE of the sensor compared to the KAF9000 or KAF6303 so after 10 hours of exposure things are a bit noisier than I would like. Still the camera is a lot of fun to use and the antiblooming makes for much easier shooting. The 12MHz download speed makes for easy flat shooting: those flats come down really fast: I can get a set of all three filters really fast compared to some of my older and slower cameras all in all I like the little Microline ML4022. It is pretty basic in terms of functionality but works well and I was able to operate at -30C with a 75F ambient. here's the first real image: http://www.narrowbandimaging.com/vdb...2hao3_page.htm I think I will do a Photon Transfer plot soon to see what the read noise, camera gain, PRNU, DSNU and full well parameters measure out to be. But here is why I posted this he there are three interesting objects in the image besides the "proplyds" i had previously noted back in 2006 Have a look at the image at the bottom of the page linked above: Liebrecht Venter, Dana Patchick and I have been examining them. The noted objects appear as stars in the red, blue and IR plates from ESO so that probably means they aren't planetaries, but the strong Ha signature (green channel) makes me wonder if there's potentially a nebula in at least one of them. (upper left candidate perhaps) I'll toss them out for the group to examine. |
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ASTRO: ML4022 first light and some "interesting objects" in the image
Richard,
very good picture and interesting to see that you found something that deserves closer inspection. Something slightly lower than 1 arcsecond/pixel is indeed a good scale as it allows for sharp pictures without too much processing. Going too much below 1"/pixel can get frustrating if the seeing doesn't cooperate... The 30% QE of this chip at Halpha is probably not the optimum for narrow band, but your picture shows that it still allows for good Halpha shots. I will probably buy a camera with the KAF 8300 chip, which has a QE of 48% at Halpha. Still not as good as my SXV-H9 camera, but at least the larger chip will finally give me the chance to go for the larger objects. Stefan "Richard Crisp" schrieb im Newsbeitrag m... A consulting project I have been involved in for some time recently needed a KAI4022 based camera for some quantitative optical studies so we ended up purchasing an FLI Microline 4022 camera This past weekend I decided to use the camera for astronomy, not having used the KAI series very much in the past. I picked the AP180EDT f/9 for using it, since it was set up in the backyard with the Proline 9000 and filters already. I just replaced the camera with the Microline and shot I ended up imaging vdB142, a familiar object I have imaged many times using emission line filters and an object in a good part of the sky at sundown. the 7.4 micron pixels of the microline give me 0.94 arc-sec/pixel at the 1620 mm focal length and that's a nice image scale for the seeing conditions. They are a bit slow in the red filters due to the lower QE of the sensor compared to the KAF9000 or KAF6303 so after 10 hours of exposure things are a bit noisier than I would like. Still the camera is a lot of fun to use and the antiblooming makes for much easier shooting. The 12MHz download speed makes for easy flat shooting: those flats come down really fast: I can get a set of all three filters really fast compared to some of my older and slower cameras all in all I like the little Microline ML4022. It is pretty basic in terms of functionality but works well and I was able to operate at -30C with a 75F ambient. here's the first real image: http://www.narrowbandimaging.com/vdb...2hao3_page.htm I think I will do a Photon Transfer plot soon to see what the read noise, camera gain, PRNU, DSNU and full well parameters measure out to be. But here is why I posted this he there are three interesting objects in the image besides the "proplyds" i had previously noted back in 2006 Have a look at the image at the bottom of the page linked above: Liebrecht Venter, Dana Patchick and I have been examining them. The noted objects appear as stars in the red, blue and IR plates from ESO so that probably means they aren't planetaries, but the strong Ha signature (green channel) makes me wonder if there's potentially a nebula in at least one of them. (upper left candidate perhaps) I'll toss them out for the group to examine. |
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