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 1 X180027.65-221956.7 xmm pn 399.662 393.624 40.5446 11.2201 0.00843342 0.00233382 3.9567 0.999911 7.83915 4.06074 56.2881 10.096 A F 0.477759 0 1 ds
Report srcpi bgdpi 2 X180053.91-222354.2 xmm pn 315.897 339.145 46.4761 8.78733 0.0141669 0.00267856 4.53554 0.99999 10.875 10.875 0 3.21136 F F 0.356959 0 1 dp
Report srcpi bgdpi 3 X180101.74-222355.1 xmm pn 290.936 338.876 35.0345 10.8753 0.0072873 0.00226211 3.41897 0.99953 7.46788 7.46788 0 3.01982 F F 0.330916 0 1 ds
Report srcpi bgdpi 4 X180100.26-222728.0 xmm pn 295.656 289.93 30.0382 11.2838 0.00624804 0.00234706 2.93139 0.9979 4.44894 4.44894 0 0.654105 F T 0.30634 0 1 ds
Report srcpi bgdpi 5 X180109.58-222739.4 xmm pn 265.977 287.295 66.426 15.5269 0.0138168 0.00322966 6.48243 1 3.71866 3.71866 0 2.47649 F F 0.27385 0 1 ds
Report srcpi bgdpi 1 X180109.66-222738.1 xmm mos2 265.713 287.599 36.1933 9.26357 0.00547045 0.00140015 5.97115 1 4.86515 4.86515 0 2.49147 F F 0.273743 0 1 ds
Report srcpi bgdpi 1 X180109.63-222738.3 xmm mos1 265.813 287.55 31.9539 8.78894 0.00482904 0.00132823 4.74805 0.999994 3.70258 3.70258 0 2.49067 F F 0.273674 0 1 ds
Report srcpi bgdpi 6 X180030.63-223205.7 xmm pn 390.026 226.047 36.5531 11.0017 0.00760318 0.00228839 3.56717 0.999658 7.28108 7.28108 0 8.42688 F F 0.367206 0 1 ds
Report srcpi bgdpi 7 X180122.06-224148.6 xmm pn 226.31 92.4587 34.5074 7.8905 0.00690161 0.00157813 3.36753 0.999357 10.875 10.875 0 15.8225 F T 0.115012 0 1 dp
Report srcpi bgdpi 3 X180053.71-222357.2 xmm mos2 316.551 338.394 40.84 8.04362 0.00617279 0.00121576 6.73776 1 10.0716 10.0716 0 3.2331 F F 0.357425 0 1 ds
Report srcpi bgdpi 2 X180053.43-222020.3 xmm mos2 317.44 388.231 19.4268 6.04917 0.00467169 0.00145468 3.20502 0.998833 10.875 10.875 0 6.65431 F F 0.388029 0 1 db
Report srcpi bgdpi 4 X180027.80-221957.8 xmm mos2 399.18 393.394 21.314 5.9394 0.00322105 0.000897584 3.51637 0.999562 10.875 10.875 0 10.037 F T 0.476878 0 1 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