Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf | 3 | X211727.96-101712.3 | chandra | ccd7 | 793.781 | 937.458 | 61.5104 | 7.89791 | 0.0291802 | 0.00374673 | 74.6597 | 1 | 0.504696 | 0.504696 | 0 | 0.335697 | F | F | 4.94e+20 | 2.16673e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X211752.12-102029.7 | chandra | ccd7 | 68.55 | 535.6 | 18.7965 | 4.47215 | 0.00891677 | 0.00212152 | 22.8147 | 1 | 1.73865 | 1.20345 | 19.2216 | 7.12911 | F | F | 4.71e+20 | 8.38089e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X211723.47-102330.9 | chandra | ccd7 | 927.912 | 167.5 | 15.7366 | 4.12312 | 0.00746521 | 0.00195595 | 19.1007 | 1 | 1.65182 | 1.3791 | 170.968 | 6.52451 | F | F | 4.84e+20 | 6.95054e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X211730.99-101846.4 | chandra | ccd7 | 702.5 | 745.7 | 4.95358 | 2.23607 | 0.0023499 | 0.00106076 | 6.01252 | 0.999924 | 0.492 | 0.492 | 150.482 | 2.01943 | F | F | 4.87e+20 | 1.75819e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X211734.70-101148.9 | chandra | ccd6 | 119.167 | 635.167 | 2.92989 | 1.73205 | 0.0013899 | 0.00082166 | 6.41976 | 0.999934 | 0.678773 | 0.492 | 155.994 | 5.57688 | F | F | 5.01e+20 | 1.78314e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X211708.25-101533.6 | chandra | ccd6 | 912.5 | 178.5 | 0.983885 | 1 | 0.00046674 | 0.000474385 | 2.15582 | 0.981097 | 0.492 | 0.492 | 90 | 4.78953 | F | F | 5.12e+20 | 5.53433e-15 | 1 | dx |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest