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 | 3 | X141206.83-030621.4 | chandra | ccd3 | 985.538 | 460.331 | 12.4124 | 3.52313 | 0.00781048 | 0.00221692 | 42.1868 | 1 | 0.517179 | 0.517179 | 0 | 2.41416 | F | F | 4.25e+20 | 0 | 1 | ds | |||||
| Report | 5 | X141204.43-030918.0 | chandra | ccd2 | 632.729 | 1086.4 | 10.8084 | 3.28761 | 0.00680119 | 0.00206873 | 35.0385 | 1 | 0.789247 | 0.381416 | 233.476 | 2.63593 | F | F | 4.19e+20 | 0 | 1 | ds | |||||
| Report | 1 | X141119.42-030838.7 | chandra | ccd0 | 967.3 | 734.5 | 4.58456 | 2.23608 | 0.00288479 | 0.00140703 | 5.21257 | 0.999846 | 1.46786 | 0.653453 | 161.601 | 9.69084 | A | F | 4.21e+20 | 0 | 1 | d | |||||
| Report | 2 | X141140.40-030823.6 | chandra | ccd0 | 329.349 | 765.89 | 14.3057 | 3.8832 | 0.00900188 | 0.00244351 | 16.2654 | 1 | 0.625398 | 0.625398 | 0 | 4.50047 | F | F | 4.22e+20 | 0 | 1 | ds | |||||
| Report | 2 | X141158.15-030849.7 | chandra | ccd2 | 823.5 | 1143.25 | 3.99649 | 2 | 0.00251475 | 0.00125848 | 12.9558 | 1 | 0.492 | 0.492 | 90 | 1.59066 | F | F | 4.2e+20 | 0 | 1 | d | |||||
| Report | 1 | X141205.15-030858.7 | chandra | ccd2 | 610.25 | 1125 | 3.98436 | 2 | 0.00250712 | 0.00125848 | 12.9164 | 1 | 0.492 | 0.492 | 160.67 | 2.52157 | F | F | 4.2e+20 | 0 | 1 | d | |||||
| Report | 4 | X141203.78-031611.2 | chandra | ccd2 | 652 | 246 | 3.60446 | 2.00001 | 0.00226807 | 0.00125849 | 11.6849 | 0.999997 | 1.39294 | 1.34318 | 180 | 9.06848 | F | F | 4.06e+20 | 0 | 1 | d | |||||
| Report | 2 | X141211.15-030422.6 | chandra | ccd3 | 853.5 | 701.167 | 2.99071 | 1.73205 | 0.00188188 | 0.00108988 | 10.1647 | 0.999998 | 0.492 | 0.492 | 130.269 | 4.38794 | F | F | 4.29e+20 | 0 | 1 | d | |||||
| Report | 1 | X141204.34-030539.5 | chandra | ccd3 | 1060.83 | 544.833 | 2.98741 | 1.73205 | 0.0018798 | 0.00108988 | 10.1535 | 0.999998 | 0.492 | 0.492 | 45 | 2.26734 | F | F | 4.27e+20 | 0 | 1 | d | |||||
| Report | 5 | X141210.67-030653.0 | chandra | ccd3 | 868.167 | 395.5 | 2.98226 | 1.73205 | 0.00187655 | 0.00108988 | 10.136 | 0.999998 | 0.492 | 0.492 | 180 | 3.22462 | F | F | 4.24e+20 | 0 | 1 | d | |||||
| Report | 3 | X141210.07-030925.0 | chandra | ccd2 | 460.5 | 1071.5 | 2.97874 | 1.73205 | 0.00187434 | 0.00108988 | 9.65644 | 0.999997 | 0.521845 | 0.492 | 90 | 3.75096 | F | F | 4.19e+20 | 0 | 1 | d | |||||
| Report | 2 | X141138.62-030524.2 | chandra | ccd1 | 843 | 188 | 1.99483 | 1.41421 | 0.00125523 | 0.00088988 | 6.97409 | 0.999914 | 0.492 | 0.492 | 45 | 5.13664 | F | F | 4.28e+20 | 0 | 1 | d | |||||
| Report | 1 | X141136.35-030113.5 | chandra | ccd1 | 912 | 697.5 | 1.97579 | 1.41421 | 0.00124325 | 0.000889881 | 6.90751 | 0.999914 | 0.492 | 0.492 | 180 | 8.0583 | F | F | 4.37e+20 | 0 | 1 | d | |||||
| Report | 4 | X141222.92-030939.0 | chandra | ccd3 | 495.5 | 58 | 1.96171 | 1.41422 | 0.00123438 | 0.000889881 | 6.66737 | 0.999899 | 0.665224 | 0.492 | 56.3099 | 6.70882 | F | F | 4.17e+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