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 | 1 | X123959.43-113723.6 | chandra | ccd7 | 187.545 | 578.01 | 395.808 | 20.0998 | 0.22408 | 0.0113791 | 257.368 | 1 | 0.492 | 0.492 | 174.969 | 1.6796 | F | F | 3.7e+20 | 1.23346e-12 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 2 | X124000.34-113724.0 | chandra | ccd7 | 160.233 | 577.2 | 28.5859 | 5.47724 | 0.0161834 | 0.00310085 | 18.5875 | 1 | 0.492 | 0.492 | 42.8868 | 1.61581 | F | F | 3.7e+20 | 8.92298e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 3 | X123957.36-113720.6 | chandra | ccd7 | 249.346 | 584.115 | 12.1875 | 3.60557 | 0.00689972 | 0.00204123 | 7.9247 | 1 | 0.492 | 0.492 | 106.655 | 1.88695 | F | F | 3.71e+20 | 4.43591e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 4 | X123959.87-113623.6 | chandra | ccd7 | 174.444 | 699.944 | 17.744 | 4.24264 | 0.0100454 | 0.0024019 | 11.5377 | 1 | 0.492 | 0.492 | 31.4582 | 0.762942 | F | F | 3.69e+20 | 5.52807e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 5 | X124000.66-113520.0 | chandra | ccd7 | 150.722 | 829.167 | 8.62549 | 3.00001 | 0.00488317 | 0.0016984 | 5.60858 | 0.999962 | 0.492 | 0.492 | 94.2654 | 0.598049 | F | F | 3.67e+20 | 2.64825e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X124001.02-113724.5 | chandra | ccd7 | 139.957 | 576.1 | 32.7452 | 5.91611 | 0.0185381 | 0.00334931 | 21.2921 | 1 | 0.627853 | 0.492 | 14.2573 | 1.59139 | T | F | 3.7e+20 | 1.51551e-13 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 7 | X123958.35-113718.1 | chandra | ccd7 | 219.667 | 589.167 | 5.26461 | 2.44951 | 0.00298047 | 0.00138675 | 3.42322 | 0.99694 | 0.492 | 0.492 | 132.322 | 1.71593 | F | F | 3.7e+20 | 1.64011e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X124000.06-113709.2 | chandra | ccd7 | 168.625 | 607.125 | 7.17887 | 2.82845 | 0.0040642 | 0.00160128 | 4.66795 | 0.99982 | 0.492 | 0.492 | 168.69 | 1.40125 | F | F | 3.7e+20 | 2.2362e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X124000.91-113703.2 | chandra | ccd7 | 143.3 | 619.5 | 4.19517 | 2.23609 | 0.00237502 | 0.00126593 | 2.72784 | 0.989223 | 0.492 | 0.492 | 25.6701 | 1.24617 | F | F | 3.7e+20 | 1.31045e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X123959.28-113828.9 | chandra | ccd7 | 191.875 | 445.25 | 7.68453 | 2.82844 | 0.00435047 | 0.00160127 | 4.99674 | 0.999962 | 0.492 | 0.492 | 37.9819 | 2.72837 | F | F | 3.72e+20 | 3.58458e-14 | 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