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 X074335.36-514031.5 xmm pn 308.028 319.792 319.363 63.4214 0.0276242 0.00548581 0 10.875 10.875 0 1.69722 U U 1.35e+21 d
Report 2 X074347.35-514320.4 xmm pn 282.405 282.798 285.379 39.9275 0.0162055 0.00226732 0 10.875 10.875 0 1.62377 U U 1.35e+21 d
Report 3 X074341.80-514037.1 xmm pn 294.264 318.94 336.302 60.39 0.0317778 0.00570636 0 10.875 10.875 0 1.51694 U U 1.35e+21 d
Report 4 X074318.33-514117.7 xmm pn 344.429 310.28 349.914 64.1867 0.030085 0.00551867 0 10.875 10.875 0 3.44319 U U 1.35e+21 d
Report 5 X074338.80-514019.5 xmm pn 300.672 322.88 486.387 65.5743 0.0438138 0.00590693 0 10.875 10.875 0 1.7795 U U 1.35e+21 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