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 | X212845.34-132434.5 | chandra | ccd3 | 517.935 | 402.343 | 16.5682 | 4.07041 | 0.00265047 | 0.000651157 | 24.4361 | 1 | 0.60967 | 0.60967 | 0 | 3.87225 | F | F | 4.94e+20 | 0 | 1 | ds | |||||
| Report | 4 | X212851.26-132453.1 | chandra | ccd3 | 342.217 | 364.538 | 11.9887 | 3.46247 | 0.00191788 | 0.000553906 | 17.6819 | 1 | 0.574202 | 0.574202 | 0 | 3.33124 | F | F | 4.93e+20 | 0 | 1 | ds | |||||
| Report | 1 | X212916.43-131832.4 | chandra | ccd0 | 440.751 | 321.222 | 25.5962 | 5.05927 | 0.00409472 | 0.00080935 | 36.5432 | 1 | 2.34998 | 1.09496 | 30.7866 | 5.86555 | F | F | 4.86e+20 | 0 | 1 | ds | |||||
| Report | 1 | X212923.53-132234.9 | chandra | ccd1 | 391.341 | 339.265 | 11.5295 | 3.73067 | 0.00184442 | 0.00059681 | 7.46026 | 1 | 1.92349 | 0.729385 | 40.899 | 6.63033 | F | F | 4.9e+20 | 0 | 1 | ds | |||||
| Report | 1 | X212835.93-132244.3 | chandra | ccd2 | 658.6 | 113.9 | 9.76908 | 3.16228 | 0.00156278 | 0.000505878 | 14.4067 | 1 | 1.12358 | 0.492 | 40.7279 | 5.07747 | A | F | 4.92e+20 | 0 | 1 | d | |||||
| Report | 3 | X212853.87-132041.5 | chandra | ccd2 | 126.5 | 363.5 | 6.87884 | 2.64575 | 0.00110043 | 0.000423248 | 10.1444 | 1 | 0.521845 | 0.492 | 45 | 1.27595 | F | T | 4.89e+20 | 0 | 1 | d | |||||
| Report | 2 | X212925.44-132327.8 | chandra | ccd1 | 334.214 | 231.357 | 6.83969 | 2.64576 | 0.00109416 | 0.000423248 | 4.42568 | 0.999806 | 0.492 | 0.492 | 120.473 | 7.24342 | F | F | 4.9e+20 | 0 | 1 | d | |||||
| Report | 2 | X212830.57-132552.1 | chandra | ccd3 | 955.5 | 244.072 | 6.63182 | 2.64576 | 0.00106091 | 0.000423249 | 9.78111 | 1 | 0.82287 | 0.492 | 102.364 | 7.49303 | A | F | 4.96e+20 | 0 | 1 | d | |||||
| Report | 3 | X212847.83-132449.2 | chandra | ccd3 | 443.5 | 372 | 5.90759 | 2.44949 | 0.000945051 | 0.000391851 | 8.71296 | 0.999999 | 0.544143 | 0.492 | 54.645 | 3.6736 | F | T | 4.94e+20 | 0 | 1 | d | |||||
| Report | 2 | X212859.30-131948.5 | chandra | ccd0 | 948.5 | 166.25 | 3.9371 | 2 | 0.000629827 | 0.000319945 | 5.62092 | 0.999842 | 0.492 | 0.492 | 90 | 2.11157 | F | F | 4.88e+20 | 0 | 1 | d | |||||
| Report | 3 | X212914.30-131722.2 | chandra | ccd0 | 503.167 | 463.5 | 2.73941 | 1.73206 | 0.00043823 | 0.000277082 | 3.911 | 0.998364 | 0.492 | 0.492 | 90 | 6.2064 | F | T | 4.84e+20 | 0 | 1 | d | |||||
| Report | 4 | X212909.04-131641.2 | chandra | ccd0 | 659.5 | 546.833 | 5.1329 | 2.44951 | 0.000821123 | 0.000391855 | 7.32814 | 0.999987 | 1.61853 | 0.795665 | 88.0349 | 5.9622 | A | F | 4.84e+20 | 0 | 1 | d | |||||
| Report | 5 | X212909.29-131952.7 | chandra | ccd0 | 652.072 | 157.643 | 6.88484 | 2.64575 | 0.00110138 | 0.000423248 | 9.82935 | 1 | 0.596477 | 0.492 | 117.588 | 3.66865 | F | F | 4.87e+20 | 0 | 1 | d | |||||
| Report | 2 | X212836.85-131947.3 | chandra | ccd2 | 631.5 | 473.5 | 1.93778 | 1.41422 | 0.000309992 | 0.000226236 | 2.8577 | 0.988477 | 0.492 | 0.492 | 90 | 5.17583 | F | F | 4.89e+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