How can I observe Sgr A* with itelescope.netCan redshift be measured using fourier?How to find which part of the sky a photo contains?How do I know what I'll be able to see?How do I align my finder scope National Geographic 76/700 EQWhat is it exactly about these flares of infrared light from Sgr A* that “confirms” it is a supermassive black hole?I've seen some stars tonight. What could I possibly have been looking at with these pictures?How did they measure the distance to the center of our galaxy to 0.3% accuracy?Meade ETX-90 with computerized mount slews too far during auto-alignmentHow did they estimate the mass of Sgr A*'s companion G2 without knowing what it was?
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How can I observe Sgr A* with itelescope.net
Can redshift be measured using fourier?How to find which part of the sky a photo contains?How do I know what I'll be able to see?How do I align my finder scope National Geographic 76/700 EQWhat is it exactly about these flares of infrared light from Sgr A* that “confirms” it is a supermassive black hole?I've seen some stars tonight. What could I possibly have been looking at with these pictures?How did they measure the distance to the center of our galaxy to 0.3% accuracy?Meade ETX-90 with computerized mount slews too far during auto-alignmentHow did they estimate the mass of Sgr A*'s companion G2 without knowing what it was?
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$begingroup$
I've been experimenting with itelescope.net and tried to observe Sgr A*.
I was wondering if there are any suggestions how I can best observe the surrounding stars.
telescope photography sgr-a
$endgroup$
add a comment |
$begingroup$
I've been experimenting with itelescope.net and tried to observe Sgr A*.
I was wondering if there are any suggestions how I can best observe the surrounding stars.
telescope photography sgr-a
$endgroup$
add a comment |
$begingroup$
I've been experimenting with itelescope.net and tried to observe Sgr A*.
I was wondering if there are any suggestions how I can best observe the surrounding stars.
telescope photography sgr-a
$endgroup$
I've been experimenting with itelescope.net and tried to observe Sgr A*.
I was wondering if there are any suggestions how I can best observe the surrounding stars.
telescope photography sgr-a
telescope photography sgr-a
asked 8 hours ago
NickpickNickpick
1204 bronze badges
1204 bronze badges
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1 Answer
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$begingroup$
I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.
The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.
$endgroup$
add a comment |
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1 Answer
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$begingroup$
I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.
The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.
$endgroup$
add a comment |
$begingroup$
I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.
The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.
$endgroup$
add a comment |
$begingroup$
I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.
The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.
$endgroup$
I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.
The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.
edited 7 hours ago
answered 8 hours ago
Rob JeffriesRob Jeffries
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59.2k4 gold badges123 silver badges194 bronze badges
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