Spinoffs from supernova hunting
Even I have to admit it: supernova hunting is boring. I take pictures of 10,000 galaxies per year, on average, and I'll find only 5 supernovae in that time period. Another way to look at it is that I shoot galaxies on 250+ nights per year. Thus, you could either say that I look at 9,995 galaxies per year and don't find a supernova in any of them, or you could say that I search for supernovae on 245 nights per year and don't make a discovery. That's a lot of time spent, and a lot of galaxies imaged with no discoveries made!
Now you take ol' M 95 here, for instance. I've shot this galaxy on 73 nights over the past 10 years, and I've never discovered a supernova in it. In 2012, I heard about a supernova in M 95, and I took some pictures of it. But that wasn't a "discovery" for me. And I haven't seen a supernova in it since then. So, you could also say that I've been looking at this galaxy for 13 years without finding a supernova in it.
Yeah, I think that qualifies as boring!
To mix things up a bit, I started to keep track of asteroids that I encounter in my searches. One of the benefits of supernova hunting is developing a large database of galaxy images, taken over a span of many years. So, if tonight my telescope-control software shows an asteroid in the field of view of a particular galaxy, I can blink the current image with an older image and see the asteroid (as shown above).
The other night, while shooting M 95, I saw that asteroid (1633) Chimay was in the field. Having such a low number for an asteroid, I knew it should look pretty bright in my images. So, without taking the time to figure out which "star" was the asteroid, I merely made a note of it and then searched for it in my images the following day.
While blinking the images, the asteroid was certainly obvious. But another star caught my eye. It was brightest in the reference image and dimmer in the image with the asteroid. Although sky conditions can vary, causing stars in an image to appear brighter than they do on a different night, this one star was brighter, and the rest stayed the same. Hmmm. Must be a variable star!
I used Aladin to identify the star of interest and it proved to be an RR Lyrae type of variable star, varying between 14th and 16th magnitude. I assume that the "ZTF" in the name means that it was discovered by the Zwicky Transient Facility, my competitors in supernova hunting! In any case, I just happened to choose a reference image with the star near maximum brightness and I blinked it with the current image when the star was near minimum brightness. What luck!
I've always appreciated and respected the work of variable star observers. And I think it would be fun to follow a variable star and create my own light curve. But it's terribly difficult, in my opinion. Variable star observing requires a type of patience and dedication that I don't seem to possess! I've been a backyard stargazer for 45 years and, for whatever reason, I've never been able to keep up with a variable star. If it's a short-period variable like Algol, I can't dedicate myself to get out there and get images of it through a complete cycle. And if it's a long-period variable like Mira, I tend to forget all about it after a few months. Variable star observing just doesn't fit my personality! But it's fun when I can "discover" a variable star like the one pictured above, as a spinoff to supernova hunting.
Supernova hunting has opened up a whole new dimension of imaging for me! Since I have to compare tonight's images with images from long ago to find supernovae, the dimension of time has become a huge part of my image processing. While other amateur astrophotographers may find faint new objects in their images by going deep with 50-hour exposures and using an assortment of fancy color filters (H-alpha, RGB, sodium, etc.), I am using relatively short (20 seconds), unfiltered exposures to find objects that change over time.
Perhaps I should have named this post "The Time Filter." Blinking images uses the filter of time to reveal objects that would likely go unnoticed by any other means.
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| My picture of the supernova in M 95 in 2012 |


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