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 | X235839.16-552937.4 | chandra | ccd7 | 783.902 | 588.438 | 121.781 | 60.7586 | 0.00610495 | 0.00304586 | 3.47959 | 0.999691 | 1.18272 | 1.18272 | 0 | 3.6771 | T | T | 1.33e+20 | 3.95644e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X235859.83-552730.1 | chandra | ccd7 | 426.902 | 847.438 | 121.776 | 14.94 | 0.00610469 | 0.00074895 | 3.47945 | 0.999691 | 1.18267 | 1.18267 | 0 | 0.113097 | T | F | 1.33e+20 | 4.38836e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X235914.62-552425.6 | chandra | ccd6 | 1082.43 | 730.926 | 76.6349 | 8.83177 | 0.00384175 | 0.000442741 | 61.6215 | 1 | 0.654638 | 0.514664 | 176.636 | 3.70753 | F | T | 1.33e+20 | 4.11622e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 1 | X000047.88-551940.9 | chandra | ccd5 | 408.47 | 841.606 | 61.9225 | 13.6022 | 0.00310421 | 0.000681886 | 25.935 | 1 | 2.88528 | 2.74147 | 64.0777 | 17.1509 | F | F | 1.29e+20 | 3.15891e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X000004.53-552604.3 | chandra | ccd6 | 219.186 | 528.186 | 34.9338 | 7.14157 | 0.00175125 | 0.000358011 | 28.09 | 1 | 3.59014 | 3.43996 | 83.7227 | 9.19273 | F | F | 1.26e+20 | 2.17232e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X235902.26-553903.8 | chandra | ccd3 | 832.417 | 729.944 | 20.6018 | 6.00018 | 0.0010331 | 0.000300886 | 3.10053 | 0.998055 | 5.62693 | 3.28915 | 100.826 | 11.5158 | A | F | 1.34e+20 | 1.49177e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X235934.44-552937.1 | chandra | ccd6 | 740.548 | 97.1667 | 20.3149 | 4.58259 | 0.0010184 | 0.000229728 | 16.335 | 1 | 0.688685 | 0.548913 | 16.6749 | 5.22925 | F | F | 1.33e+20 | 1.2523e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X235917.61-553617.7 | chandra | ccd3 | 568 | 1067.45 | 15.3961 | 4.69051 | 0.000772053 | 0.000235211 | 2.31708 | 0.986667 | 2.62982 | 2.07403 | 176.122 | 9.07187 | F | F | 1.34e+20 | 1.05357e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X235923.71-553523.4 | chandra | ccd3 | 463.389 | 1178.16 | 26.3196 | 6.35469 | 0.00131984 | 0.000318666 | 3.96105 | 0.999878 | 3.16942 | 3.16942 | 0 | 8.50837 | F | T | 1.34e+20 | 1.78776e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X235926.79-554212.3 | chandra | ccd3 | 411.183 | 346.452 | 42.8506 | 9.38122 | 0.00214879 | 0.000470432 | 6.44894 | 1 | 5.0697 | 4.2878 | 133.381 | 15.1169 | F | F | 1.35e+20 | 3.18054e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X235907.73-554058.7 | chandra | ccd3 | 738.984 | 496.998 | 14.0402 | 8.67276 | 0.000704068 | 0.000434909 | 2.11302 | 0.981236 | 3.28903 | 2.30908 | 6.94395 | 13.4934 | F | F | 1.34e+20 | 1.04015e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X235927.29-553734.6 | chandra | ccd3 | 402.148 | 911.339 | 22.1346 | 7.39889 | 0.00110997 | 0.000371028 | 3.33122 | 0.999184 | 5.2372 | 5.2372 | 0 | 10.7246 | F | F | 1.34e+20 | 1.52439e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X235850.62-553854.2 | chandra | ccd3 | 1033.19 | 749.985 | 77.6989 | 12.1018 | 0.00389633 | 0.000606864 | 11.6935 | 1 | 4.2085 | 4.2085 | 0 | 11.4382 | F | F | 1.34e+20 | 5.81466e-14 | 1 | dsx |
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