Astro Spectroscopy workflow

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  • เผยแพร่เมื่อ 13 ก.ย. 2024

ความคิดเห็น • 14

  • @92mrkite
    @92mrkite 2 หลายเดือนก่อน +1

    Amazing tutorial! I’m about to set a SA200 in my EFW, and now in the best position to process my first data. If only the weather agrees, in the French southwest… Thanks again!

  • @johnfisher2495
    @johnfisher2495 4 หลายเดือนก่อน +3

    Excellent presentation. BASS also has all this step by step and more under help, for new viewers,but I like starting with the video first for an overview. I was completely unaware of siril and imagej.so thanks. I used the pixel tool in sharpcap for focus previously. Hopefully maybe you could do one on slit spectroscopy. I’m finding guiding to be troublesome there. Much appreciated 😀

  • @burtwatson8990
    @burtwatson8990 4 หลายเดือนก่อน +3

    Outstanding presentation!

  • @bassspectro483
    @bassspectro483 4 หลายเดือนก่อน

    Many thanks for sharing this well structured presentation.
    Looking forward to the next one.

  • @powaznyszachista
    @powaznyszachista หลายเดือนก่อน

    Hi. Thanks for great video. How do you get rid of reference spectrum? I can't figure this out on my own.

  • @EGYHER0
    @EGYHER0 4 หลายเดือนก่อน

    Ty for sharing your experience

  • @astrothib
    @astrothib 4 หลายเดือนก่อน

    Very nice presentation!

  • @kai_seestar
    @kai_seestar 4 หลายเดือนก่อน +1

    Excellent! Thank you for sharing this and great timing.
    I will give a presentation of doing Spectroscopy with Seestar at TAIC tonight, and have been using BASS for processing. May i reference this video in my talk?

  • @ravnica1
    @ravnica1 4 หลายเดือนก่อน

    Nice, how would you obtain and apply instrument response for a spectrum of a star of a different type let's say Betelguese?

    • @TheAstronomicalAmateur
      @TheAstronomicalAmateur  4 หลายเดือนก่อน +1

      Thanks for the question @ravnica1 - Typically you would use the instrument response from a nearby Type A or B star (that has these Balmer lines; like Sirius or Vega) to correct the instrument response the target you are after that same night (lets say Betelgeuse or Uranus). The instrument response corrects (contains, models) the atmospheric distortions, optical efficiency and your Camera quantum efficiency. So in order to get your target identified well, you always shoot a nearby Type A,B star on the same night.

    • @ritacastil
      @ritacastil หลายเดือนก่อน

      Thanks for your video! Very usefull for a someone like me wanting an overview. I am still unsure to go down this route. I would like to know if, from the scientific point of view, this type of slitless spectroscopy has any usefulness!

  • @johnfisher2495
    @johnfisher2495 4 หลายเดือนก่อน

    Just curious why you didn’t do your preprocessing inBASS?

    • @TheAstronomicalAmateur
      @TheAstronomicalAmateur  4 หลายเดือนก่อน

      Probably my familiarity with SIRIL from Astrophotography. But I also really enjoyed the speed of working with SER files. I did not find a way to use SER files in BASS (individual FITs work great!). To make it work in BASS you could export the individual FITS subs from SER (e.g. using SIRIL), and then do the stacking in BASS instead.