Call for monitoring of AG Dra by R. Galis & al.
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Re: Call for monitoring of AG Dra by R. Galis & al.
Increase of He II, and Balmer lines intensities in the last spectrum obtained by Joan
Equivalent widths mesaured on Echelle spectra: New observations strongly welcome for the next days
François
Stormy weather here
Equivalent widths mesaured on Echelle spectra: New observations strongly welcome for the next days
François
Stormy weather here
François Teyssier
http://www.astronomie-amateur.fr
http://www.astronomie-amateur.fr
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Re: Call for monitoring of AG Dra by R. Galis & al.
Hello,
These graphs, are a complement of the François's anterior explanation.
This is de first service of the Linx.
Today is de second day cloud, the weather will improve on next Wednesday.
Regards, J. Guarro.
These graphs, are a complement of the François's anterior explanation.
This is de first service of the Linx.
Today is de second day cloud, the weather will improve on next Wednesday.
Regards, J. Guarro.
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Re: Call for monitoring of AG Dra by R. Galis & al.
Hi all,
According to last AAVSO observations from the previous night, there is an increase of brightness of AG Dra in all filters. Of course, it is based only on the observations by one observer, but nevertheless, also according to your last spectroscopic observation (the increase of EWs of Balmer lines and He II), it is worth monitoring the star in the next days.
We are looking forward to new observations. Have a clear sky!
Regards,
Jaroslav Merc
According to last AAVSO observations from the previous night, there is an increase of brightness of AG Dra in all filters. Of course, it is based only on the observations by one observer, but nevertheless, also according to your last spectroscopic observation (the increase of EWs of Balmer lines and He II), it is worth monitoring the star in the next days.
We are looking forward to new observations. Have a clear sky!
Regards,
Jaroslav Merc
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Re: Call for monitoring of AG Dra by R. Galis & al.
Bonjour à tous, placez le profil d'observation de la nuit 28/05/2017.
Umberto
Umberto
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Re: Call for monitoring of AG Dra by R. Galis & al.
I've been having issues processing my LISA spectra...think I just solved it with another tune-up at the scope.
Here is AG Dra on 28May17:

I labeled the probable He lines...Hope we see more "fireworks" in this system!
James
Here is AG Dra on 28May17:

I labeled the probable He lines...Hope we see more "fireworks" in this system!
James
James Foster
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
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Re: Call for monitoring of AG Dra by R. Galis & al.
Clear sky last nightAccording to last AAVSO observations from the previous night, there is an increase of brightness of AG Dra in all filters. Of course, it is based only on the observations by one observer, but nevertheless, also according to your last spectroscopic observation (the increase of EWs of Balmer lines and He II), it is worth monitoring the star in the next days.
The fit is now in the base, Jaroslav
Significant increase of Raman OVI Update of EW from echelle spectra James: the identification of He I lines is correct
Your spectrum is welcome in the base!
Umberto: excellent coverage!
François
François Teyssier
http://www.astronomie-amateur.fr
http://www.astronomie-amateur.fr
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Re: Call for monitoring of AG Dra by R. Galis & al.
This full weekend's one night result - with an experiment, tuning the Alpy 600 focus on the UV (via mercury lamp's UV lines) + scope too (in turn loosing the IR part's focus):
Also lost the H-alpha with 3 x 15 minute exposures (almost H-beta, too).
The SNR start to become good from 3650A.
However, no big change in this region.
- Peter
Looks like this tuning brought some extra (Balmer serie full).Also lost the H-alpha with 3 x 15 minute exposures (almost H-beta, too).
The SNR start to become good from 3650A.
However, no big change in this region.
- Peter
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Re: Call for monitoring of AG Dra by R. Galis & al.
Nice result Peter!
Waiting for the fit
No change since yesterday He II declining slowly
François
Waiting for the fit
No change since yesterday He II declining slowly
François
François Teyssier
http://www.astronomie-amateur.fr
http://www.astronomie-amateur.fr
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Re: Call for monitoring of AG Dra by R. Galis & al.
Bonjour, voici le profil hier soir et une comparaison des Raman OVI avec le jour 28/05/2017
Umberto
Umberto
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Re: Call for monitoring of AG Dra by R. Galis & al.
I believe (looking AG Dra in my video finder scope) that AG Dra has brightening as seen last night. I've taken BVI photometry of this object with a C-11 the last two weeks and will process that for submission to AASVO.
In addition, in support of the Solar Analog project, I'm getting a 200mm lens on a ST-8 and RVB & Stromgren V filters to mount on top of my CDK17 and spectroscope to take simultaneous specta/photometry.
James
In addition, in support of the Solar Analog project, I'm getting a 200mm lens on a ST-8 and RVB & Stromgren V filters to mount on top of my CDK17 and spectroscope to take simultaneous specta/photometry.
James
James Foster
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200