From CBAT:
TCP J18154219+3515598
http://www.cbat.eps.harvard.edu/unconf/ ... 15598.html
Possible dwarf nova mag 11.8 unfiltered
Paolo
Transient in Lyra
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Re: Transient in Lyra
Dwarf nova!
Guiding camera view:


I updated the CBAT TOCP follow up with mine and Umberto's observation.
Paolo
Guiding camera view:


I updated the CBAT TOCP follow up with mine and Umberto's observation.
Paolo
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Re: Transient in Lyra
Excellent!
fits welcome for inclusion in the letter
François
fits welcome for inclusion in the letter
François
François Teyssier
http://www.astronomie-amateur.fr
http://www.astronomie-amateur.fr
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Re: Transient in Lyra
Sent you, François. Thanks.
A missing information, the spectrum is composed by 4 x 960s exposure frames.
Paolo
A missing information, the spectrum is composed by 4 x 960s exposure frames.
Paolo
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Re: Transient in Lyra
Bonjour à tous, voici mon profil. Umberto
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Re: Transient in Lyra
Bonjour à tous, placez un nouveau profil de la nova, observé hier soir.
Umberto
Umberto
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Re: Transient in Lyra
Salut, placé le profil d'observation du 06/12/2017.Umberto
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Re: Transient in Lyra
Bonjour, placé le profil d'observation de cette nuit.
Umberto
Umberto
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Re: Transient in Lyra
Well done Umberto. I also observed the DN on June 12. An important rebrightening helped us to continue the observations. Rebrightenings are also indicators of the WZ Sge membership (but there was no doubt considering the high amplitude outburst).
I performed a relatively long session to try and follow with photometry the small flux oscillations (superhumps) typical of this class stars. I covered about two cycles.
The DN lightcurve (SXV-H9, Mak 90 scope, V band filter Baader, 88 x 120s frames):

The flux oscillates about 0.07 mag around mean value 12.49. I used the latter value to calibrate the spectrum in absolute flux. On the top of graph I reported the spectroscopic coverage (11 x 960s frames).

In addition to h-beta and h-gamma, the profile show the He I 4471 broad absorption line.
Paolo
I performed a relatively long session to try and follow with photometry the small flux oscillations (superhumps) typical of this class stars. I covered about two cycles.
The DN lightcurve (SXV-H9, Mak 90 scope, V band filter Baader, 88 x 120s frames):
The flux oscillates about 0.07 mag around mean value 12.49. I used the latter value to calibrate the spectrum in absolute flux. On the top of graph I reported the spectroscopic coverage (11 x 960s frames).

In addition to h-beta and h-gamma, the profile show the He I 4471 broad absorption line.
Paolo