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 AAVSO. Show all posts
Showing posts with label AAVSO. 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.
Monday, July 29, 2013
Cool data...
Here is a cool light curve that jumped out at me.
The target is PNV J19150199+0719471 which is a newly discovered cataclysmic variable in Aquila. This is about a 4 hr. run, each dot is a 60 second observation with a CCD camera and yes, those are error bars! The precursor object was about 20th mag, here you can see it's varying around 15.8 The target is showing a 87 minute period. This sawtooth pattern is referred to as 'superhumps'. The model says this is oscillations in the accretion disk swirling around the white dwarf as the matter pours on to it. It's pretty dramatic…
Monday, April 22, 2013
Confirmed a new supernova in NGC 7331 with this image.
Position
22 37 2.07 +34 24 2.92
It's the upper of the close pair.
Position
22 37 2.07 +34 24 2.92
It's the upper of the close pair.
Tuesday, January 15, 2013
W30 has a new home
W30 is a 12" Meade SCT donated to the AAVSONet by the estate of Paul Wright, a former AAVSO member. The telescope is equipped with an SBIG STL-1001 camera and photometric filters. It runs a nightly program of variable star imagining gathering hundreds of images.
A new steel pier was added to the observing floor to support the telescope. Several nights of work were required to get the polar alignment right and the focusing system working properly.
Thursday, November 15, 2012
W30 arrives at Sutter Creek Observatory
Mike Simonsen and Bill Goff with telescope referred to as W30
W30 is a Meade 12" SCT telescope owned by the AAVSO as a part of their AAVSONet of telescopes. In November, it was moved to Sutter Creek Observatory and I became the new host. The scope is shown there temporarily on a tripod mounting.
Subscribe to:
Posts (Atom)



