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Name Last modified Size Description
Parent Directory -
2010junwifesb.log 16-Jun-2010 13:30 13K
Jul20/ 30-Jul-2010 11:12 -
Jun28/ 30-Jul-2010 11:12 -
calibjun2010.fits 16-Jun-2010 13:45 20K
sp024bf.fits 16-Jun-2010 13:37 39K
sp028bf.fits 16-Jun-2010 13:27 39K
sp036bf.fits 16-Jun-2010 13:27 39K
sp041bf.fits 16-Jun-2010 13:27 39K
sp042bf.fits 16-Jun-2010 13:27 39K
sp080bf.fits 16-Jun-2010 13:38 39K
sp087bf.fits 16-Jun-2010 13:27 39K
sp088bf.fits 16-Jun-2010 13:27 39K
sp089bf.fits 16-Jun-2010 13:27 39K
sp090bf.fits 16-Jun-2010 13:27 39K
sp143bf.fits 16-Jun-2010 13:38 39K
Blue WIFES Observations June 7,8,9 2010 ---------------------------------------- Good between 3500A and 5900A. 3400-3500 and ~5900-6000 problematic. The fluxes are on a relative absolute scale, but the absolute scale is unreliable due to cloud, seeing and so forth. But the relative fluxes are excellent except on the extreme edges of the spectra as noted above. The extreme red edge is well into the dichroic (the red side measures from 5600A to 9700A). sp024bf.fits EG131 sp028bf.fits cs22940-09 sp036bf.fits lsiv-14_116 sp041bf.fits cs22955-24 seems it was cloudy; could do repeating sp042bf.fits cs29496-10 sp080bf.fits EG131 sp087bf.fits F110 sp088bf.fits cs22956-90 sp089bf.fits cs22956-94 sp090bf.fits cs22938-44 sp143bf.fits EG131 The logfile identifies the stars as does the fits header. I used Heap-Lindler standards from the STIS archive http://archive.stsci.edu/prepds/stisngsl/index.html plus my own values for EG131. Standards used bd-122669.tab cd-3018140.tab g114-26h.tab g20-15.tab hd161770.tab hd204543.tab hd9051.tab eg131new.tab The mean flux calibration that I used (15 observations) is calibjun2010.fits sp087bf is Feige 110. It is a sdO Hamuy spectrophotomenric standard. sp024bf.fits is the smooth spectrum star (EG131) that I used for division. sp080bf.fits and sp143bf.fits are also EG131 on different nights. It will give you a feeling for the repeatability of the observations and reductions.