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J/ApJ/562/368 UV photometry in NGC 2808 (Brown+, 2001)
Flash mixing on the white dwarf cooling curve: understanding hot horizontal branch anomalies in NGC 2808. Brown T.M., Sweigart A.V., Lanz T., Landsman W.B., Hubeny I. <Astrophys. J. 562, 368 (2001)> =2001ApJ...562..368B
ADC_Keywords: Clusters, globular ; Photometry, ultraviolet Keywords: globular clusters: individual (NGC 2808) - stars: atmospheres - stars: evolution - stars: horizontal-branch - ultraviolet: stars Description: We examine new observations of NGC 2808, taken with the far-UV and near-UV cameras on the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope (HST). Images were obtained in the far-UV crystal quartz (FUV/F25QTZ; pivot wavelength 1600Å), near-UV 2700Å continuum (NUV/F25CN270), and clear CCD (CCD/50CCD; pivot wavelength 5850Å) modes, employing a cross-shaped dither pattern. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 48 295 Photometric catalog
See also: J/A+AS/84/59 : BV photometry of NGC 2808 (Ferraro+, 1990) Table 1: UV Imaging -------------------------------------------------------------------------------- STIS Band Exposure Observation Dates (2000) Coverage (s) (arcmin2) -------------------------------------------------------------------------------- FUV/F25QTZ 8916 Jan 18, Feb 16 1744 NUV/F25CN270 8906 Jan 19, Feb 20 1752 Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1 I1 h RAh Right Ascension (J2000) (1) 3- 4 I2 min RAm Right Ascension (J2000) (1) 6- 12 F7.4 s RAs Right Ascension (J2000) (1) 14 A1 --- DE- Declination (J2000) (1) 15- 16 I2 deg DEd Declination (J2000) (1) 18- 19 I2 arcmin DEm Declination (J2000) (1) 21- 26 F6.3 arcsec DEs Declination (J2000) (1) 28- 32 F5.2 mag FUVmag The Far-UV STMAG magnitude (1600Å) 34- 37 F4.2 mag e_FUVmag The error in FUVmag 39- 43 F5.2 mag NUVmag The Near-UV STMAG magnitude (2700Å) 45- 48 F4.2 mag e_NUVmag The error in NUVmag
Note (1): The relative astrometry is very accurate (tenths of a 0.025arcsec STIS pixel), but the absolute astrometry is subject to a 1-2 arcsec uncertainty (associated with the position of the guide stars). Objects identified as [BSL2001] JHHMMSS.ssss+DDMMSS.sss in Simbad
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 29-Jan-2002
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