spectro-aras.com

Super manip Olivier. La cave est resté a une température supérieur a l'extérieur car tu as des sources de chaleur dans la cave: * compression du gaz * fonctionnent de la caméra. Les variations que tu observes sont typiques d'une régulation dite en fourchette. C'est ce qui est fait de base par la cav...

Hello Francois.

Your perfectly right ! The algorithm of guiding put the wrong star is ne slit.
I need to improve my program to manage this kind of situation. Today i need no brighter star close to 15 arcsec of the target.

Thierry

A emission star. H gamma, H beta, Ha. And the line are really broad.
Any idea ?

Yes Andrew, i keep the list of observed stars updated.

A new emitting star.

A new emitting star. Mag 9.6

I continue the survey tonight, and re discovered the emission of this star.
Spectrum look similar.
Francois (LISA) & Christian (VHIRES), can you send me your spectrum ? I will update the ARAS web page with these spectrum.

With the help of Andrew, i integrate the plot in Galactic coordinate here: http://www.astrosurf.com/aras/be_candidate/auto-be-candidate.html#GalacticPlot And just below a html, csv full list of already observed star from Andrew and me, in the same format. http://www.astrosurf.com/aras/be_candidate/r...

Vmag=6.3 so a esay target for HighResolution spectrum. But that's a morning star in the Gemini.

Hello Tonight, I capture BD+03 3861. High resolution spectrum are welcome. The star is not present in Bess, nor Catalogue of Stellar Spectral Classifications (Skiff, 2009-2014) nor http://arxiv.org/abs/1409.4668 19 00 05.95543 +03 19 05.8433 Vmag=8.6 H-K=-0.02 i just updated the list of Be candidate...