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 | 3 | X153658.65-510221.4 | chandra | ccd3 | 1152.96 | 674.35 | 74.5969 | 8.7018 | 0.0158891 | 0.00185348 | 70.3463 | 1 | 0.454527 | 0.454527 | 0 | 1.97218 | 27.8306 | 46 | 0.246096 | 0.134747 | F | T | 4.02e+21 | 1.93192e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X153750.07-510933.4 | chandra | ccd7 | 1109.79 | 814.864 | 74.1439 | 10.4207 | 0.0157925 | 0.00221959 | 19.9184 | 1 | 4.82745 | 3.54246 | 114.211 | 11.9056 | 68.6564 | 6.47 | -0.827757 | 0.178452 | F | F | 4.32e+21 | 1.94092e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X153653.02-505901.7 | chandra | ccd1 | 447.671 | 389.467 | 31.1118 | 5.72836 | 0.00662692 | 0.00122016 | 23.8457 | 1 | 0.650693 | 0.650693 | 0 | 4.09002 | 18.9153 | 11.9153 | -0.227047 | 0.221412 | F | T | 3.94e+21 | 8.33368e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X153652.15-505525.8 | chandra | ccd1 | 463.75 | 827.667 | 11.753 | 4.57071 | 0.00250343 | 0.000973578 | 23.6475 | 1 | 1.44281 | 0.841815 | 45.3354 | 7.61309 | 8.9506 | 2.90119 | -0.510421 | 0.436289 | A | F | 3.86e+21 | 3.51797e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X153718.86-505813.6 | chandra | ccd3 | 764.083 | 1177.08 | 11.3909 | 4.57071 | 0.00242626 | 0.000973561 | 14.5951 | 1 | 1.57836 | 1.26163 | 95.147 | 6.94348 | 7.59392 | 3.79696 | -0.333333 | 0.42619 | F | F | 4.01e+21 | 3.26243e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X153726.42-505844.4 | chandra | ccd3 | 619.1 | 1114.2 | 9.61616 | 4.27872 | 0.00204824 | 0.000911367 | 15.5213 | 1 | 1.00486 | 0.759298 | 48.3391 | 7.5489 | 9.74411 | -0.127946 | -1 | 0.626494 | F | F | 4.05e+21 | 2.82312e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X153555.36-510052.2 | chandra | ccd0 | 876.278 | 959.833 | 9.09204 | 4.27872 | 0.00193665 | 0.00091139 | 9.54175 | 1 | 2.54987 | 1.13931 | 108.257 | 8.35926 | 6.69735 | 2.39469 | -0.473233 | 0.525248 | A | F | 3.77e+21 | 2.8353e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X153634.73-510928.6 | chandra | ccd2 | 931.357 | 598.643 | 6.69855 | 3.78388 | 0.0014268 | 0.000805973 | 12.2003 | 1 | 1.38192 | 0.492 | 173.069 | 6.75059 | 2.87942 | 3.84927 | 0.144137 | 0.57485 | A | F | 4.08e+21 | 1.97202e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X153638.43-510401.9 | chandra | ccd2 | 860.833 | 1262.67 | 5.91531 | 3.59808 | 0.00125997 | 0.000766396 | 20.326 | 1 | 0.492 | 0.492 | 153.435 | 1.6706 | 5.91531 | 0 | -1 | 0.871615 | F | F | 3.98e+21 | 1.90927e-14 | 1 | dx |
| Report | 5 | X153658.42-511018.8 | chandra | ccd2 | 478.333 | 496.667 | 5.85833 | 2.44949 | 0.00124783 | 0.000521746 | 10.4545 | 1 | 0.492 | 0.492 | 74.8718 | 7.5415 | F | F | 4.17e+21 | 0 | 1 | d | |||||
| Report | 7 | X153649.83-510301.6 | chandra | ccd3 | 1321.5 | 592.25 | 3.97961 | 2 | 0.000847657 | 0.000426 | 3.75285 | 0.998918 | 0.492 | 0.492 | 90 | 0.480685 | F | F | 4e+21 | 0 | 1 | d | |||||
| Report | 1 | X153658.77-505917.6 | chandra | ccd1 | 336.75 | 356.5 | 3.97449 | 2 | 0.000846581 | 0.000426007 | 3.04625 | 0.991951 | 0.492 | 0.492 | 39.6902 | 4.15593 | F | F | 3.97e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X153654.00-510122.3 | chandra | ccd3 | 1241.5 | 794 | 3.91531 | 3.17945 | 0.00083396 | 0.000677222 | 13.4537 | 1 | 0.492 | 0.492 | 52.0181 | 1.98139 | 0.915307 | 3 | 0.532447 | 0.936375 | F | F | 3.99e+21 | 1.00364e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X153707.96-510604.4 | chandra | ccd2 | 295.5 | 1013.5 | 4.78698 | 3.39792 | 0.00101964 | 0.000723762 | 10.3718 | 1 | 0.587021 | 0.492 | 97.0181 | 4.53179 | 1.85799 | 2.92899 | 0.223733 | 0.738413 | F | F | 4.12e+21 | 2.00735e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X153714.31-505739.8 | chandra | ccd3 | 851.25 | 1246 | 3.91739 | 3.17945 | 0.000834404 | 0.000677222 | 13.6298 | 1 | 0.504692 | 0.492 | 142.018 | 6.87078 | 1 | 0.917393 | -0.0430828 | 1.4262 | F | F | 3.99e+21 | 1.11297e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X153600.60-505746.0 | chandra | ccd0 | 776.75 | 1338.5 | 3.7742 | 3.17945 | 0.000803926 | 0.00067724 | 7.94267 | 0.999996 | 1.38853 | 0.740549 | 113.875 | 8.95062 | 2.86452 | 1.90968 | -0.2 | 0.736836 | A | F | 3.71e+21 | 1.53803e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X153603.43-510537.9 | chandra | ccd0 | 720 | 379.5 | 5.74452 | 3.59808 | 0.00122361 | 0.00076641 | 11.3652 | 1 | 1.68849 | 0.636813 | 171.918 | 7.30171 | 4.87226 | 0.872262 | -0.696315 | 0.773348 | A | T | 3.91e+21 | 1.68059e-14 | 1 | dx |
| Report | 5 | X153724.32-510304.9 | chandra | ccd3 | 660.5 | 584.833 | 2.94277 | 1.73205 | 0.00062681 | 0.000368927 | 2.77509 | 0.994051 | 0.529672 | 0.492 | 169.722 | 5.90061 | F | F | 4.12e+21 | 0 | 1 | d | |||||
| Report | 3 | X153654.74-510619.9 | chandra | ccd2 | 548.5 | 982.167 | 2.93958 | 1.73205 | 0.000626136 | 0.00036893 | 5.24584 | 0.999684 | 0.492 | 0.492 | 28.155 | 3.5627 | F | T | 4.08e+21 | 0 | 1 | d | |||||
| Report | 4 | X153628.43-510340.6 | chandra | ccd0 | 241.5 | 618.833 | 2.93935 | 1.73205 | 0.000626097 | 0.000368937 | 5.2744 | 0.999697 | 0.621484 | 0.492 | 14.3052 | 2.96188 | F | F | 3.94e+21 | 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