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 | X042706.27-594857.0 | chandra | ccd7 | 835.187 | 443.229 | 260.695 | 16.4575 | 0.0814928 | 0.00514458 | 111.156 | 1 | 1.21019 | 0.564754 | 310.369 | 4.06554 | 165.802 | 53.7629 | -0.510279 | 0.0811254 | A | F | 1.41e+20 | 6.13209e-13 | 1 | dsxf |
| Report | srcpi bgdpi arf | 7 | X042715.62-594941.4 | chandra | ccd7 | 691.789 | 353.196 | 9.92184 | 3.28163 | 0.00310155 | 0.00102583 | 4.23049 | 0.9998 | 0.391834 | 0.391834 | 0 | 4.33606 | 6.91528 | 1.83056 | -0.581388 | 0.550503 | F | F | 1.41e+20 | 2.41924e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X042700.77-595012.4 | chandra | ccd7 | 918.8 | 289.4 | 10.6977 | 4.42783 | 0.00334408 | 0.00138413 | 19.4561 | 1 | 0.827997 | 0.492 | 22.2219 | 5.49878 | 4.89923 | 0.84884 | -0.704652 | 0.775905 | A | F | 1.41e+20 | 2.87245e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X042837.26-594942.6 | chandra | ccd3 | 803.3 | 419.6 | 10.0673 | 4.42783 | 0.00314715 | 0.00138418 | 10.4245 | 1 | 2.26364 | 1.91801 | 145.114 | 10.3212 | 5.56954 | 4.4978 | -0.106457 | 0.44593 | F | F | 1.43e+20 | 4.80069e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X042654.17-594725.9 | chandra | ccd7 | 1020.5 | 627.667 | 5.83061 | 3.59808 | 0.00182264 | 0.00112475 | 14.1669 | 1 | 0.492 | 0.492 | 36.8699 | 4.09073 | 1.91531 | 3.91531 | 0.343017 | 0.66104 | F | F | 1.41e+20 | 1.70604e-14 | 1 | dx |
| Report | 1 | X042749.72-594023.1 | chandra | ccd6 | 86.8333 | 440.167 | 2.91714 | 1.73205 | 0.000911914 | 0.000541451 | 5.88906 | 0.999876 | 0.921538 | 0.625576 | 176.203 | 6.10625 | F | F | 1.41e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X042713.62-594132.7 | chandra | ccd6 | 642.5 | 299 | 4.83061 | 3.39792 | 0.00151008 | 0.00106221 | 11.7372 | 1 | 0.492 | 0.492 | 90 | 4.05491 | -0.0846933 | 4.91531 | 1 | 0.992474 | F | F | 1.4e+20 | 1.69739e-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