Source List

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 X015841.40-432503.8 chandra ccd7 683.41 323.635 226.106 15.2907 0.0449108 0.00303714 162.981 1 0.669131 0.449272 198.018 0.289304 F F 1.44e+20 3.24054e-13 1 dsxf
Report srcpi bgdpi arf 2 X015834.18-432744.9 chandra ccd6 218.077 858.321 50.8536 7.13117 0.0101009 0.00141645 86.4963 1 0.992196 0.445442 27.8284 2.71845 A F 1.44e+20 1.08831e-13 1 dsx
Report srcpi bgdpi arf 1 X015818.99-431554.4 chandra ccd3 226.845 407.113 24.3024 6.25338 0.00482712 0.00124209 6.31662 1 5.45757 2.66943 346.02 10.258 F F 1.45e+20 6.94457e-14 1 dsx
Report srcpi bgdpi arf 1 X015751.85-432352.6 chandra ccd2 242.5 291.587 18.3701 4.7959 0.00364879 0.000952595 33.5423 1 4.51401 2.28753 21.7066 9.09359 A F 1.46e+20 5.24482e-14 1 dx
Report 7 X015827.67-432521.8 chandra ccd7 987.305 286.979 16.0982 4.01226 0.00319755 0.000796945 11.6038 1 0.523292 0.523292 0 2.4667 F F 1.44e+20 0 1 ds
Report 3 X015835.70-432417.1 chandra ccd7 809.57 418.652 13.952 3.73524 0.00277125 0.000741921 10.0568 1 0.510814 0.510814 0 1.46908 F F 1.44e+20 0 1 ds
Report srcpi bgdpi arf 4 X015849.36-432413.6 chandra ccd7 506.997 425.622 13.3453 3.65312 0.00265074 0.00072561 9.61951 1 0.322512 0.322512 0 1.85174 F F 1.43e+20 1.98625e-14 1 dsx
Report srcpi bgdpi arf 6 X015908.63-432057.9 chandra ccd7 79.0557 822.611 8.39596 3.00001 0.00166767 0.000595884 6.05195 0.999994 1.15077 0.59726 157.57 6.63233 A F 1.42e+20 1.35867e-14 1 dx
Report srcpi bgdpi arf 5 X015847.78-432201.7 chandra ccd7 541.375 693.375 7.79183 2.82843 0.00154767 0.000561803 5.61648 0.999966 0.492 0.492 63.8734 3.52929 F F 1.43e+20 1.18514e-14 1 dx
Report srcpi bgdpi arf 2 X015843.15-432518.2 chandra ccd7 644.167 294 5.8104 2.44949 0.0011541 0.000486536 4.18823 0.999139 0.492 0.492 111.355 0.346543 F F 1.44e+20 8.60601e-15 1 dx
Report srcpi bgdpi arf 1 X015809.66-432946.7 chandra ccd6 759.75 609.75 3.6315 2.00001 0.000721314 0.000397257 6.17678 0.999548 0.933236 0.519055 12.5574 7.24261 A F 1.45e+20 9.18694e-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