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 | 1 | X092919.16-312244.3 | chandra | ccd7 | 284.381 | 345.656 | 42.3907 | 6.87313 | 0.00173406 | 0.000281156 | 21.2169 | 1 | 0.346354 | 0.346354 | 0 | 0.961859 | F | F | 1.21e+21 | 0 | 1 | ds | |||||
| Report | 2 | X092920.19-312303.3 | chandra | ccd7 | 257.645 | 307.097 | 21.835 | 4.82451 | 0.000893198 | 0.000197355 | 10.9286 | 1 | 0.449477 | 0.254162 | 74.6384 | 0.581246 | F | F | 1.21e+21 | 0 | 1 | ds | |||||
| Report | 3 | X092912.48-312042.6 | chandra | ccd7 | 457.944 | 592.5 | 7.87418 | 3.00002 | 0.000322106 | 0.000122721 | 3.9411 | 0.9991 | 0.498857 | 0.492 | 65.8168 | 3.4374 | F | F | 1.21e+21 | 0 | 1 | d | |||||
| Report | 4 | X092915.95-312144.4 | chandra | ccd7 | 367.5 | 467 | 5.18551 | 2.44951 | 0.000212121 | 0.000100201 | 2.59539 | 0.991975 | 0.613698 | 0.492 | 168.76 | 2.17084 | F | F | 1.21e+21 | 0 | 1 | d | |||||
| Report | 5 | X092924.49-312420.8 | chandra | ccd7 | 145.81 | 149.604 | 37.9931 | 6.4941 | 0.00155417 | 0.000265652 | 19.0159 | 1 | 0.44621 | 0.44621 | 0 | 1.01992 | F | F | 1.21e+21 | 0 | 1 | ds |
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