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
Andy Wilson
Andy Wilson, 2018 Aug 25 - 09:06 UTC

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

David Swan
David Swan, 2018 Aug 25 - 10:26 UTC

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?

Andy Wilson
Andy Wilson, 2018 Aug 25 - 12:20 UTC

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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