Документ взят из кэша поисковой машины. Адрес оригинального документа : http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_Spec_Publ_Cat.README Дата изменения: Fri Jun 14 23:45:05 2013 Дата индексирования: Fri Feb 28 09:54:48 2014 Кодировка: ISO8859-5 Поисковые слова: южная атлантическая аномалия

CHANDRAOBSID: Chandra observation identifier;
SPECOBJID: spectroscopic observation identifier;
CXOMPNAME: ChaMP identifier;
RA: optical R.A. (J2000);
DEC.: optical DECL. (J2000);
TELESCOPE: telescope used for obtaining spectrum;
SPEC: spectrograph used for obtaining spectrum;
DATE: date of spectroscopic observation;
REDSHIFT: spectroscopic redshift;
CLASS: spectroscopic classification, BLAGN (broad-line AGN), NELG (narrow emission line galaxy), ALG (absorption line galaxy);
NETB: number of counts and associated errors;
FSC: soft (0.5-2 keV) X-ray flux in units of 12-13 erg s-1 cm-2 and associated errors;
FHC: hard (2-8 keV) X-ray flux in units of 12-13 erg s-1 cm-2 and associated errors;
FUV: far-UV AB magnitude and associated errors;
NUV: near-UV AB magnitude and associated errors;
U: u-band AB magnitude and associated errors;
G: g-band AB magnitude and associated errors;
R: r-band AB magnitude and associated errors;
I: i-band AB magnitude and associated errors;
Z: z-band AB magnitude and associated errors;
Y: y-band Vega magnitude and associated errors;
J: J-band Vega magnitude and associated errors;
H: H-band Vega magnitude and associated errors;
K: K-band Vega magnitude and associated errors;
MAG34: 3.4 ЮМm Vega magnitude and associated errors;
MAG46: 4.6 ЮМm Vega magnitude and associated errors;
MAG12: 12 ЮМm Vega magnitude and associated errors;
MAG22: 22 ЮМm Vega magnitude and associated errors;
S20: 20 cm radio flux in mJy and associated errors;
LOG LX: logarithmic 2-10 keV X-ray luminosity in units of erg s-1 ;
GAMMA: power-law slope from X-ray spectral fitting and associated 90% confidence;
NHINT, NH and associated 90% confidence;
NPHOT: number of photometric bands per catalogue used for the SED fitting (X: Chandra: G: GALEX, O: Optical, N: near-infrared, W: WISE, R: radio);
AGNTEMP: AGN template used for the SED fit (0: No AGN used, 1: Elvis et al. 1994 + Richards et al. 2006, 2: Hopkins et al. 2007, 3-6: Seyfert-2 from Bianchi et al. 2006, 7: NGC 1068 by Matt et al. 1997, 8: Mrk231 by Berta et al. 2006, 9: IRAS19254- 7245 by Berta et al. 2003, 10: IRAS22491-1808 by Farrah et al. 2003;
GALTEMP: galaxy template used for the SED fit (0: No galaxy template used, 1: NGC 5253 by Beck et al. 1996, 2: NGC 7714 by Brandl et al. 2004, 3: M82 by Strickland et al. 2004, 4: IRAS12112+0305 by Imanishi et al. 2007, 5: Elliptical from Rowan-Robinson et al. 2008, 6: Young elliptical from Maraston 2005);
FSB: fraction of starburst contribution to the bolometric luminosity;
FA: fraction of AGNs contribution to the bolometric luminosity;
LBOL: bolometric luminosity (1e9-1e19 Hz) in erg s-1 ;
MBH: logarithmic estimate of black hole mass