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 | X003935.52-510511.8 | chandra | ccd5 | 359.479 | 185.165 | 29.957 | 11.7359 | 0.00322118 | 0.00126192 | 2.88563 | 0.997113 | 4.57894 | 4.57894 | 0 | 11.6796 | F | F | 1.49e+20 | 0 | 1 | ds | |||||
| Report | 2 | X003923.02-511237.9 | chandra | ccd6 | 342.022 | 285.481 | 36.6546 | 6.0543 | 0.00394135 | 0.000650999 | 49.6158 | 1 | 1.0963 | 1.0963 | 0 | 3.99316 | F | F | 1.44e+20 | 0 | 1 | ds | |||||
| Report | 1 | X003928.20-511036.0 | chandra | ccd6 | 242.577 | 532.731 | 16.0339 | 4.12312 | 0.00172407 | 0.000443345 | 21.7035 | 1 | 1.05507 | 0.654914 | 139.676 | 6.15776 | A | F | 1.45e+20 | 0 | 1 | d | |||||
| Report | 3 | X003919.83-511758.8 | chandra | ccd7 | 130.009 | 644.32 | 14.2314 | 3.77245 | 0.00153025 | 0.000405638 | 11.6619 | 1 | 0.415872 | 0.415872 | 0 | 1.51237 | F | F | 1.4e+20 | 0 | 1 | ds | |||||
| Report | 1 | X003915.86-511701.7 | chandra | ccd7 | 205.856 | 760.305 | 10.9285 | 3.30583 | 0.00117511 | 0.000355465 | 8.95538 | 1 | 0.569171 | 0.569171 | 0 | 0.560499 | F | F | 1.41e+20 | 0 | 1 | ds | |||||
| Report | 2 | X003915.92-511615.1 | chandra | ccd7 | 204.1 | 854.6 | 9.75482 | 3.16228 | 0.0010489 | 0.000340029 | 7.9936 | 1 | 0.492 | 0.492 | 158.085 | 0.347624 | F | F | 1.41e+20 | 0 | 1 | d | |||||
| Report | 3 | X003919.69-511238.7 | chandra | ccd6 | 405.278 | 283.5 | 8.81178 | 3 | 0.000947501 | 0.00032258 | 11.9277 | 1 | 0.935137 | 0.492 | 18.0881 | 3.89182 | A | F | 1.44e+20 | 0 | 1 | d | |||||
| Report | 5 | X003912.76-511918.8 | chandra | ccd7 | 264.278 | 481.167 | 8.61228 | 3.00001 | 0.000926049 | 0.000322581 | 7.05734 | 0.999999 | 0.492 | 0.492 | 124.294 | 2.88501 | F | F | 1.39e+20 | 0 | 1 | d | |||||
| Report | 4 | X003924.04-511445.0 | chandra | ccd6 | 322.25 | 26.75 | 3.91091 | 2 | 0.000420527 | 0.000215054 | 5.29382 | 0.999743 | 0.492 | 0.492 | 45 | 2.05603 | F | F | 1.43e+20 | 0 | 1 | d |
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