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 | 2 | X010511.29-061207.0 | chandra | ccd7 | 618.716 | 1027.46 | 176.926 | 13.5472 | 0.0180222 | 0.00137996 | 143.388 | 1 | 0.443496 | 0.336947 | 7.69736 | 1.89335 | 124.807 | 51.9357 | -0.412302 | 0.0877707 | F | F | 5.34e+20 | 1.43349e-13 | 1 | dsxf |
| Report | srcpi bgdpi arf | 1 | X010516.11-061748.7 | chandra | ccd7 | 472.574 | 333.12 | 46.4431 | 6.81538 | 0.00473084 | 0.000694236 | 37.6393 | 1 | 1.92383 | 1.01925 | 347.551 | 6.0389 | 33.4018 | 13.6656 | -0.419318 | 0.185944 | F | F | 5.39e+20 | 3.81076e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X010442.21-060712.3 | chandra | ccd6 | 1031.29 | 657.443 | 33.5504 | 5.79227 | 0.00341755 | 0.000590019 | 41.6119 | 1 | 4.17921 | 2.52514 | 71.3822 | 7.61472 | 22.702 | 10.054 | -0.386128 | 0.237097 | F | F | 5.36e+20 | 4.11747e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X010509.03-060649.6 | chandra | ccd6 | 217.7 | 703.18 | 32.7624 | 6.89491 | 0.00333728 | 0.000702338 | 29.4498 | 1 | 1.70667 | 1.38589 | 73.1236 | 5.89702 | 23.8625 | 8.96865 | -0.45365 | 0.231319 | F | F | 5.31e+20 | 4.03967e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X010506.49-061509.4 | chandra | ccd7 | 764.145 | 656.762 | 20.0974 | 4.48301 | 0.00204718 | 0.000456653 | 16.2877 | 1 | 0.340928 | 0.340928 | 0 | 2.65168 | 15 | 5.91516 | -0.434366 | 0.296629 | F | F | 5.37e+20 | 1.7516e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 15 | X010502.83-061535.6 | chandra | ccd7 | 875.128 | 603.489 | 19.2119 | 4.38314 | 0.00195698 | 0.00044648 | 15.5701 | 1 | 0.598909 | 0.342092 | 149.908 | 3.02179 | 13.9032 | 6.9032 | -0.336435 | 0.288557 | F | F | 5.38e+20 | 1.623e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X010502.63-061509.1 | chandra | ccd7 | 881.002 | 657.468 | 12.9856 | 3.7228 | 0.00132275 | 0.000379215 | 10.524 | 1 | 0.372356 | 0.372356 | 0 | 2.58805 | 9 | 3.91526 | -0.3937 | 0.394565 | F | F | 5.37e+20 | 1.01377e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 7 | X010513.97-061028.3 | chandra | ccd7 | 536.9 | 1227.6 | 9.70594 | 4.27872 | 0.000988674 | 0.000435842 | 17.8985 | 1 | 0.566578 | 0.492 | 79.3673 | 3.27429 | 8 | 1.85297 | -0.623876 | 0.516372 | F | F | 5.33e+20 | 8.38632e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 13 | X010514.06-061750.4 | chandra | ccd7 | 534.136 | 329.136 | 9.0132 | 4.42783 | 0.00091811 | 0.000451031 | 6.39443 | 0.999999 | 1.95153 | 0.926957 | 15.5531 | 5.83 | 8.71026 | 0.716858 | -0.847916 | 0.620852 | A | F | 5.39e+20 | 7.36876e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 11 | X010522.41-061252.3 | chandra | ccd7 | 281.214 | 934.928 | 6.04099 | 3.78388 | 0.000615353 | 0.000385437 | 6.16876 | 0.999992 | 0.521455 | 0.492 | 16.5119 | 4.60743 | 4.60041 | 1.60041 | -0.483806 | 0.685868 | F | F | 5.34e+20 | 5.63986e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 8 | X010515.49-061640.3 | chandra | ccd7 | 490.833 | 471.5 | 6.32794 | 3.78388 | 0.000644582 | 0.000385437 | 7.71898 | 0.999999 | 0.743977 | 0.492 | 82.5868 | 5.00012 | 4.71998 | 0.775981 | -0.717617 | 0.816481 | A | F | 5.38e+20 | 5.35038e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X010504.51-061322.9 | chandra | ccd7 | 823.7 | 872.9 | 4.57653 | 3.39792 | 0.000466179 | 0.000346121 | 7.03278 | 0.999994 | 0.492 | 0.492 | 18.4349 | 0.810238 | 4.91531 | -0.25408 | -1 | 0.992474 | F | F | 5.36e+20 | 3.50324e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 14 | X010505.27-061147.7 | chandra | ccd7 | 800.7 | 1066.3 | 4.40715 | 3.39792 | 0.000448924 | 0.000346121 | 5.72379 | 0.999964 | 0.492 | 0.492 | 45 | 0.859216 | 3 | 1.74592 | -0.264244 | 0.75178 | F | T | 5.34e+20 | 3.40038e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X010454.30-060622.4 | chandra | ccd6 | 664.3 | 758.5 | 4.70362 | 3.39792 | 0.000479126 | 0.000346123 | 8.63986 | 0.999999 | 1.26493 | 0.492 | 110.573 | 6.65495 | 1.90121 | 2.80241 | 0.191598 | 0.746709 | A | F | 5.33e+20 | 5.53761e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X010443.59-060807.2 | chandra | ccd6 | 988.667 | 545.367 | 33.6401 | 6.97913 | 0.00342669 | 0.000710917 | 28.8469 | 1 | 1.95257 | 1.36352 | 67.5926 | 6.73889 | 23.5861 | 10.1131 | -0.399802 | 0.223706 | F | F | 5.36e+20 | 4.06042e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 12 | X010510.01-061843.8 | chandra | ccd7 | 657.1 | 220.5 | 5.49571 | 3.59808 | 0.000559808 | 0.00036651 | 7.73898 | 0.999999 | 0.965354 | 0.638683 | 156.658 | 6.33016 | 3.88794 | 1.88794 | -0.346268 | 0.667974 | A | F | 5.4e+20 | 4.55763e-15 | 1 | dx |
| Report | 9 | X010500.19-061540.2 | chandra | ccd7 | 954.5 | 593.75 | 3.77404 | 2.00001 | 0.000384435 | 0.000203726 | 3.05863 | 0.995218 | 0.492 | 0.492 | 50.3098 | 3.22021 | F | F | 5.38e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 10 | X010457.52-061402.9 | chandra | ccd7 | 1035.5 | 791.5 | 4.91531 | 3.39792 | 0.000500687 | 0.000346121 | 16.8899 | 1 | 0.492 | 0.492 | 90 | 2.15871 | 2 | 2.91531 | 0.186216 | 0.713849 | F | T | 5.37e+20 | 4.02957e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X010516.57-061245.5 | chandra | ccd7 | 458.167 | 948.833 | 2.83061 | 2.93649 | 0.000288334 | 0.000299119 | 6.87766 | 0.99997 | 0.492 | 0.492 | 90 | 3.15221 | 0.915307 | 2 | 0.372068 | 1.09797 | F | F | 5.34e+20 | 2.25668e-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