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 X182752.47-105149.4 xmm pn 192.726 222.297 33.4217 7.76775 0.0121024 0.00281279 0 10.875 10.875 0 9.44508 U U 1.49e+22 d
Report 2 X182731.69-105125.0 xmm pn 263.119 227.716 34.892 8.08016 0.00956553 0.00221515 0 10.875 10.875 0 5.73106 U U 1.46e+22 d
Report 3 X182738.66-104401.3 xmm pn 239.49 329.708 39.9089 8.55015 0.0111058 0.00237933 0 10.875 10.875 0 4.83776 U U 1.43e+22 d
Report 1 X182749.04-105322.3 xmm mos2 204.354 200.745 24.7957 6.26566 0.00643905 0.00162709 0 10.875 10.875 0 9.83313 U U 1.5e+22 d
Report 2 X182736.30-105341.5 xmm mos2 247.507 195.99 34.6964 7.91617 0.00460635 0.00105096 0 10.875 10.875 0 8.29459 U U 1.48e+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