Observation by David Swan: BL Lacertae: prototypic blazar
Uploaded by
David Swan
Observer
David Swan
Observed
2018 Aug 23 - 20:45
Uploaded
2018 Aug 23 - 22:38
Objects
Variable star
Planetarium overlay
Constellation
Lacerta
Field centre
RA: 22h02m
Dec: +42°18'
Position angle: -52°26'
Field size
0°27' × 0°18'
Equipment
- 200mm SCT @ f/7
- ASI183MM
- Baader UV+IR cut
- FireCapture, DeepSkyStacker and Maxim DL
Exposure
14 x 20s
Location
Tynemouth, UK
Target name
BL Lac
Title
BL Lacertae: prototypic blazar
About this image
BL Lac is left of the red line. I estimate its brightness at 13.7 CV
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Comments
A good image of a fascinating object. This is one of the active galactic nuclei that got me interested in variable star astronomy. If you interested in contributing observations to the Variable Star Section, then please get in touch with me or Roger Pickard the Director :-)
Cheers,
Andy
I do plan to get into variables Andy, and I look forward to getting yours and other's guidance at the upcoming workshop. I am currently doing a little project comparing my CV and V photometric estimates (versus published V mags) when I have my Baader luminance UV+IR cut filter in place versus my Baader photometric V filter in place. The results - so far - are I think interesting. I plan on capturing several fields containing stars with a range of B-V ratios and perhaps prepping a little letter. Something on experience with a CMOS camera, photometry and spectral sensitivity?
It will be great to meet you at the workshop David. It sounds like you are doing very good prep work. Understanding how your system works with different filters will be useful and I look forward to hearing about your findings. Typically a V filter is used when accurate results are needed and when results will be combined with other observers, and unfiltered is used when monitoring objects for outbursts. Though there are no hard and fast rules as scientifically useful observations can be obtained with just about any setup.
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