Symbiotics at the UV end

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Peter Somogyi
Posts: 420
Joined: Sun Jul 13, 2014 8:56 am

Symbiotics at the UV end

Post by Peter Somogyi »

Hello,

Let me publish a few result examples for UV end (defining a new method for myself), with my best care of response (2 ref stars where appropriate - averaging where needed), using Vega from the calspec library for IR curve + of course local ref.stars in the near. (This means ref.stars + target stars all everything divided by a Vega IR = instrumental response corrector, but used only a low order spline later "Automatic 2".) Using Vega was not extremely necessary, but I can see bad effects (minor ripples, UV end deviation) that it has removed.
I was doing exposures up to the level H-alpha allowed (ideally I'd overexpose even H-beta, but seeing no common procedure sending spectra in this way, and just overexposing H-alpha don't seem to be of much improvement).

Let me show a few interesting results:
asdb_v694mon_20170331_841.png
asdb_v694mon_20170331_841.png (7.78 KiB) Viewed 3536 times
In the above case, there's a sudden cut at Balmer end. It's not because the object was low (23 degree in my case), that drop is visible on the spectrum end itself visually! (I can see people cutting it here, I'd suggest not to do so even when noisy.)
I would also introduce the practice to send in some noise in the end till meaningful, even if speculative... it's needed at least for SNR estimate, and the definite end is hard to specify. Here in this case, for U band evaluation this hard cut at Balmer end should be something important...

AG Dra is something reproducing here to me, now showing a bit more (including noise as a watermark):
asdb_agdra_20170331_984.png
asdb_agdra_20170331_984.png (6.97 KiB) Viewed 3536 times
For fullness, a few main targets:
asdb_tcrb_20170401_018.png
asdb_tcrb_20170401_018.png (6.75 KiB) Viewed 3536 times
BF Cyg got quite bluish, and using Vega (+ ref star: 1 Sge) did make the continuum much more straight till blue end:
asdb_bfcyg_20170401_133.png
asdb_bfcyg_20170401_133.png (7 KiB) Viewed 3536 times
However, below 3650A I'm also uncertain, due to high gradients arise on the IR curve.

Cheers,
Peter

PS: all was made with a 300/1200 Newton + Alpy 600 + Atik 414 EXm + internal calibration frames.
Francois Teyssier
Posts: 1548
Joined: Fri Sep 23, 2011 1:01 pm
Location: Rouen
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Re: Symbiotics at the UV end

Post by Francois Teyssier »

Nice to see the Balmer jump!

François
Andrew Smith
Posts: 321
Joined: Fri Sep 30, 2011 12:23 pm

Re: Symbiotics at the UV end

Post by Andrew Smith »

Glad you got a satisfactory method worked out Peter, which is giving good results.

Regards Andrew
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