I was lucky enough to be named as a co-author to an article about this target published in the scientific journal Nature, January 7, 2016. Here's a link:
Nature article about V404 Cygni
There was also a article published by my variable star astronomy group, AAVSO at:
AAVSO article about observers helping with the science
Very cool...
Sutter Creek Observatory conducts astronomical photometry of variable stars. It is associated with the American Association of Variable Star Observers and the Center for Backyard Astrophysics.
Showing posts with label V404 Cygni. Show all posts
Showing posts with label V404 Cygni. Show all posts
Saturday, January 9, 2016
Saturday, June 20, 2015
V404 Cyg in outburst!
This target in the constellation of Cygnus, V404, is known to be a black hole binary paired with a near solar mass companion. On June 15, 2015 it went into outburst rising from magnitude 19 to about magnitude 12.
I first observed the target on June 19 and the outburst was continuing. Here is a light curve of it's activity.

This chart contains observations over about a four hour period. The dark dots show the changes in brightness over the period, the red dots show a nearby comparison star which as you can see, is unchanging. Each dark dot is a 30 second exposure, measured with photometric software. Since each dot is 30 seconds, changes in brightness at the two or three minute level can be seen. Very exiting.
I first observed the target on June 19 and the outburst was continuing. Here is a light curve of it's activity.

This chart contains observations over about a four hour period. The dark dots show the changes in brightness over the period, the red dots show a nearby comparison star which as you can see, is unchanging. Each dark dot is a 30 second exposure, measured with photometric software. Since each dot is 30 seconds, changes in brightness at the two or three minute level can be seen. Very exiting.
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