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 1 X175425.18-261952.7 xmm mos2 314.113 315.242 5654.48 89.2446 0.687551 0.0108516 0 10.875 10.875 0 1.66619 U U 1.18e+22 d
Report 2 X175422.79-261931.2 xmm mos2 321.5 319.093 52.8059 13.4413 0.00681589 0.00173492 0 10.875 10.875 0 2.24469 U U 1.18e+22 d
Report 3 X175430.16-261952.8 xmm mos2 298.726 315.822 45.067 11.8509 0.00532826 0.00140113 0 10.875 10.875 0 1.26058 U U 1.17e+22 d
Report 4 X175424.48-261854.0 xmm mos2 316.281 328.207 42.2807 10.162 0.00586904 0.0014106 0 10.875 10.875 0 2.51633 U U 1.18e+22 d
Report 5 X175428.32-261846.5 xmm mos2 304.408 330.316 36.979 10.1121 0.00449436 0.00122901 0 10.875 10.875 0 2.35143 U U 1.18e+22 d
Report 6 X175422.75-261857.8 xmm mos2 321.629 327.104 34.4664 9.61815 0.00450586 0.0012574 0 10.875 10.875 0 2.67332 U U 1.18e+22 d
Report 7 X175421.58-262054.6 xmm mos2 325.212 300.851 40.0387 11.0272 0.00477979 0.00131642 0 10.875 10.875 0 1.94907 U U 1.18e+22 d

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 - 10.00 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), A = 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