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Re: Nova Del 2013 = V339 Del

Posted: Fri Aug 01, 2014 12:33 pm
by Terry Bohlsen
David Boyd wrote:Robin,

That's an interesting question. I use an Astrodon V filter which has a significantly higher transmission at the [OIII] wavelength than the Bessel V which is used in ISIS for the V mag-based flux calculation. The Bessel filter transmission at the [OIII] wavelength is only 65% of the transmission of the Astrodon filter. When I convolve my recent spectra of V339 Del with the Astrodon filter profile, it reduces the intensity of the [OIII] line to 70% of it's original level but that wavelength is right on the edge of the filter profile where the gradient is large. A small change in the profile of the filter being used will potentially make a large change in the contribution of the [OIII] line to the overall magnitude being measured.

For this reason I am using the actual profile of my Astrodon filter, which I use to measure the V mag at the same time as taking the spectrum, to flux calibrate my spectra rather than the Bessel profile in ISIS.

David
David
I also use Astrodon filters so maybe my flux calibration will be out. Where did you get a transmission profile for the astrodon filter?
Terry

Re: Nova Del 2013 = V339 Del

Posted: Fri Aug 01, 2014 7:33 pm
by David Boyd
Terry,

I asked Don Goldman. He sent me a spreadsheet with transmission profiles for several of their filters including the Johnson V. I'll send you a copy.

David

Nova Del 2013 one year

Posted: Fri Aug 29, 2014 11:22 pm
by Francois Teyssier
A spectrum this night
Only 1200 secondes exposure before clouds arrive.
_novadel2013_20140829_943_fteyssier.png
_novadel2013_20140829_943_fteyssier.png (3.37 KiB) Viewed 6036 times
One year and a few years after the outburst

François

Re: Nova Del 2013 = V339 Del

Posted: Mon Oct 06, 2014 3:30 pm
by Olivier GARDE
Evolution de la Nova du Dauphin entre le 24 juillet et le 3 octobre.
Image

Re: Nova Del 2013 = V339 Del

Posted: Wed Oct 22, 2014 4:59 pm
by Paolo Berardi
New observations with Lhires III 1200.

H-beta and [O III] doublet (18 october):

Image

The complex H-Alpha line profile (19 october):

Image

Paolo