Here spectra obtain following the call of observation from Dr Noel Richardson and Dr Anthony Moffat link here
Due to bad wheather condition, it was not possible to obtain spectra during the period of measuarements of CHANDRA satellites. But, i hope these data obtain just before can help the studies.
The spectrograph is a cross dispersed with a typical resolution of R=11000. Spectra are calibrated in wave lenght with a Argon thorium lamp. Instrumental response was removed with anly one observation of the reference star Beta eri.
The observation of beta eri was done for each night, but these spectra do not exploit these data at the time of writing of this web page. If necessary, i will exploit these data about the continium.
I did a substraction of a sythetic model of atmospheric H2O for the spectra obtain on december, 16 th. Look working very good.
Page genere automatiquement le 28/12/2012 a 13:38 par un script python a
partir des fichiers fits au format definit pour la base de donnee Bess
Auteur Thierry Lemoult, pour m ecrire: thierry dot lemoult arobase hotmail dot
fr
Objet | date | Pose | Instrument | fichier |
delta-orion | 2012-11-29T22:53:52 | 24 x 60 s | C14 eShel#TLE ST8XME | _del-ori_20121129_954_full.fits |
delta orion | 2012-12-02T22:11:42 | 3 x 120 s | C14 eShel#TLE ST8XME | _del-ori_20121202_925_full.fits |
del-ori | 2012-12-08T21:39:34 | 15 x 120 s | C14 eShel#TLE ST8XME | _del-ori_20121208_902_full.fits |
del-ori | 2012-12-11T22:58:04 | 5 x 240 s | C14 eShel#TLE ST8XME | _del-ori_20121211_957_full.fits |
del ori | 2012-12-16T21:40:24 | 9 x 120 s | C14 eShel#TLE ST8XME | _del-ori_20121216_903_full.fits |
del ori | 2012-12-16T21:40:24 | 9 x 120 s | C14 eShel#TLE ST8XME | _del_ori_20121216_903_full_H2O.fits |
delta-orion
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