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 rmf | 3 | X231823.63-422213.7 | chandra | ccd7 | 538.09 | 598.038 | 726.57 | 33.1382 | 0.132165 | 0.00602793 | 81.3599 | 1 | 0.483924 | 0.483924 | 0 | 0.585741 | F | T | 1.33e+20 | 4.90979e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X231822.43-422212.4 | chandra | ccd7 | 565.119 | 600.771 | 38.3389 | 7.57137 | 0.00697394 | 0.00137725 | 4.29312 | 0.999976 | 1.5 | 1.5 | 0 | 0.728448 | T | T | 1.33e+20 | 3.95591e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X231822.34-421809.3 | chandra | ccd7 | 567.336 | 1094.81 | 29.8149 | 5.4603 | 0.00542341 | 0.000993243 | 3.33862 | 0.999234 | 1.21321 | 1.21321 | 0 | 4.60197 | F | F | 1.35e+20 | 3.43266e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 21 | X231823.94-422355.1 | chandra | ccd7 | 531.139 | 391.971 | 23.9811 | 5.32186 | 0.00436223 | 0.00096806 | 2.68536 | 0.994757 | 0.347444 | 0.347444 | 0 | 1.2196 | F | F | 1.32e+20 | 2.48668e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 13 | X231830.00-422042.0 | chandra | ccd7 | 394.032 | 784.011 | 43.6987 | 7.00004 | 0.00325052 | 0.000520698 | 4.89329 | 0.999997 | 0.49639 | 0.492 | 47.7188 | 2.20401 | F | F | 1.34e+20 | 1.88523e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 15 | X231753.21-422202.4 | chandra | ccd7 | 1222.94 | 619.976 | 39.3308 | 7.81041 | 0.00292561 | 0.000580977 | 4.40418 | 0.999984 | 2.23024 | 1.48199 | 124.888 | 5.96705 | A | F | 1.32e+20 | 1.8878e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X231849.46-422411.8 | chandra | ccd6 | 742.57 | 999.754 | 39.1464 | 6.57756 | 0.00291191 | 0.000489273 | 19.2911 | 1 | 1.39128 | 1.39128 | 0 | 4.69835 | F | F | 1.33e+20 | 2.89014e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X231758.58-423010.5 | chandra | ccd2 | 906.973 | 1203.61 | 13.7807 | 6.08423 | 0.00102508 | 0.000452575 | 2.85878 | 0.996987 | 2.76722 | 2.76722 | 0 | 8.92144 | F | F | 1.28e+20 | 1.25872e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X231840.99-422301.0 | chandra | ccd6 | 932.7 | 1143.3 | 9.62554 | 3.16228 | 0.000715995 | 0.000235226 | 4.7434 | 0.999897 | 0.492 | 0.492 | 66.1368 | 2.91181 | F | F | 1.33e+20 | 6.72256e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X231854.44-422525.2 | chandra | ccd6 | 630.167 | 849.944 | 7.40907 | 3.00003 | 0.000551123 | 0.000223157 | 3.65115 | 0.998833 | 1.35553 | 0.822988 | 33.5751 | 6.01678 | A | F | 1.33e+20 | 5.50985e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X231848.90-422424.9 | chandra | ccd6 | 754.833 | 972.667 | 5.51312 | 2.4495 | 0.000410093 | 0.000182206 | 2.71683 | 0.99019 | 0.591583 | 0.492 | 77.5598 | 4.67264 | F | T | 1.33e+20 | 4.11755e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X231853.08-422404.5 | chandra | ccd6 | 660.5 | 1014.1 | 4.64535 | 2.23608 | 0.000345544 | 0.00016633 | 2.2892 | 0.974918 | 0.492 | 0.492 | 126.65 | 5.30434 | F | T | 1.33e+20 | 3.41052e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X231749.93-422727.0 | chandra | ccd3 | 289.5 | 904.1 | 4.38861 | 2.23608 | 0.000326524 | 0.000166371 | 4.0559 | 0.998674 | 0.814691 | 0.492 | 57.1139 | 8.05787 | A | F | 1.29e+20 | 3.85562e-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