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 | 6 | X125250.77-423935.3 | chandra | ccd7 | 353.587 | 551.446 | 52.9689 | 8.89155 | 0.00710387 | 0.00119248 | 14.6653 | 1 | 0.931765 | 0.556188 | 95.1098 | 0.285786 | 54.9273 | 7.44392 | -0.761303 | 0.183854 | T | F | 7.55e+20 | 5.36769e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X125430.14-424317.4 | chandra | ccd5 | 127.389 | 687.167 | 38.5774 | 8.05337 | 0.00517374 | 0.00108007 | 11.9493 | 1 | 3.84806 | 2.97913 | 48.4135 | 18.3727 | 23.378 | 7.69036 | -0.504939 | 0.264107 | F | F | 7.58e+20 | 5.9468e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X125351.13-424250.0 | chandra | ccd5 | 1000.89 | 746.318 | 21.8854 | 6.97913 | 0.00293513 | 0.000935995 | 6.04334 | 1 | 4.12987 | 1.9622 | 167.592 | 11.3112 | 15.0288 | 9.23584 | -0.23874 | 0.293038 | A | F | 7.6e+20 | 2.90508e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X125312.97-424007.7 | chandra | ccd6 | 842.946 | 782.321 | 19.4112 | 4.40581 | 0.00260331 | 0.00059088 | 26.2995 | 1 | 1.54943 | 0.781829 | 316.654 | 3.84946 | 13.8291 | 8.57275 | -0.234639 | 0.270477 | F | F | 7.59e+20 | 2.94312e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X125218.31-424004.4 | chandra | ccd7 | 1080.76 | 491.132 | 17.5153 | 5.4441 | 0.00234904 | 0.000730127 | 14.3749 | 1 | 1.36529 | 0.854963 | 177.038 | 6.27193 | 11.7879 | 6.25767 | -0.306459 | 0.31716 | A | F | 7.47e+20 | 1.92985e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X125228.18-424657.3 | chandra | ccd3 | 271.389 | 881.278 | 15.4341 | 5.33013 | 0.00206992 | 0.000714842 | 9.63511 | 1 | 2.55158 | 1.88599 | 54.5165 | 8.65828 | 7.24899 | 8.24765 | 0.0644434 | 0.346528 | F | F | 7.37e+20 | 2.76907e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X125232.91-424242.0 | chandra | ccd7 | 753.619 | 171.719 | 51.86 | 7.20139 | 0.00695514 | 0.000965806 | 14.3583 | 1 | 1.65942 | 0.70282 | 75.6307 | 4.79038 | 31.749 | 15.6414 | -0.339891 | 0.178295 | A | F | 7.46e+20 | 6.94757e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X125212.50-424652.9 | chandra | ccd3 | 622.333 | 889.5 | 13.1599 | 4.96863 | 0.00176492 | 0.00066636 | 9.70131 | 1 | 2.6098 | 1.13435 | 11.8697 | 10.3781 | 7.37436 | 5.82233 | -0.117608 | 0.381494 | A | F | 7.34e+20 | 2.55223e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X125212.35-424700.8 | chandra | ccd3 | 625.611 | 873.556 | 21.3867 | 5.7697 | 0.00286824 | 0.000773794 | 27.308 | 1 | 1.21506 | 0.693358 | 145.889 | 10.4902 | 11.7547 | 9.63199 | -0.099252 | 0.272334 | A | F | 7.34e+20 | 4.19526e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X125250.99-423908.9 | chandra | ccd7 | 348.167 | 604.611 | 8.74592 | 4.1225 | 0.00117295 | 0.000552883 | 17.3508 | 1 | 0.492 | 0.492 | 3.7157 | 0.437057 | 5.83061 | 2 | -0.489184 | 0.56866 | F | F | 7.56e+20 | 8.88621e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X125227.21-423747.1 | chandra | ccd7 | 881.5 | 770.389 | 11.6598 | 4.57071 | 0.00156373 | 0.000612994 | 19.9901 | 1 | 0.734929 | 0.492 | 101.477 | 4.92457 | 7.9433 | 3.9433 | -0.336514 | 0.408807 | F | F | 7.54e+20 | 1.23932e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X125238.60-423635.7 | chandra | ccd7 | 626.25 | 915.75 | 7.7611 | 3.95804 | 0.00104087 | 0.000530827 | 15.8786 | 1 | 0.523313 | 0.492 | 166.717 | 3.85453 | 3.92037 | 2.84073 | -0.159683 | 0.573417 | F | F | 7.58e+20 | 8.25876e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 13 | X125253.77-424139.0 | chandra | ccd7 | 285.75 | 299.375 | 7.49184 | 3.95804 | 0.00100476 | 0.000530827 | 10.5097 | 1 | 0.492 | 0.492 | 21.8014 | 2.15445 | 6.91531 | 0.661227 | -0.825454 | 0.684576 | F | F | 7.53e+20 | 7.76405e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 10 | X125227.11-424204.3 | chandra | ccd7 | 883.25 | 247.75 | 8.49184 | 4.1225 | 0.00113887 | 0.000552883 | 11.9125 | 1 | 0.492 | 0.492 | 115.67 | 5.28807 | 3.83061 | 4.74592 | 0.106722 | 0.488066 | F | F | 7.45e+20 | 1.00265e-14 | 1 | dx |
| Report | 6 | X125302.24-424302.1 | chandra | ccd6 | 1083.17 | 427.5 | 5.88281 | 2.44949 | 0.000788964 | 0.00032851 | 7.97038 | 0.999998 | 0.492 | 0.492 | 101.599 | 3.96769 | F | F | 7.52e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X125310.04-424039.0 | chandra | ccd6 | 908.1 | 718.3 | 4.61696 | 3.39792 | 0.000619197 | 0.000455706 | 7.45996 | 0.999997 | 0.543911 | 0.492 | 83.9526 | 3.45532 | 1.92339 | 2.69357 | 0.166815 | 0.757458 | F | F | 7.57e+20 | 6.65277e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X125341.40-424423.3 | chandra | ccd6 | 206.25 | 261.25 | 5.62278 | 3.59808 | 0.000754091 | 0.000482551 | 9.15494 | 1 | 1.55865 | 0.867967 | 152.329 | 10.2561 | 3.81139 | 1.81139 | -0.355696 | 0.688185 | A | F | 7.56e+20 | 1.89724e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X125258.45-424350.8 | chandra | ccd6 | 1168 | 328.5 | 2.91531 | 2.93649 | 0.000390982 | 0.000393823 | 10.0175 | 0.999998 | 0.492 | 0.492 | 180 | 4.479 | 1.91531 | 1 | -0.313966 | 1.07858 | F | F | 7.5e+20 | 4.58936e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X125308.83-424355.2 | chandra | ccd6 | 935.5 | 319.5 | 1.66123 | 2.65831 | 0.000222793 | 0.000356516 | 2.85413 | 0.994963 | 0.492 | 0.492 | 90 | 5.35314 | 1.91531 | -0.25408 | -1 | 2.01728 | F | F | 7.52e+20 | 2.65606e-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