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 X005915.17-281904.4 xmm pn 247.233 372.324 59.7532 12.4431 0.0603448 0.0125663 0 10.875 10.875 0 6.5174 F F 7.90081 0 1 dp
Report srcpi bgdpi 3 X005926.23-281714.5 xmm pn 213.613 398.038 68.7145 14.003 0.0693948 0.0141416 0 10.875 10.875 0 9.48487 F F 7.88372 0 1 d
Report srcpi bgdpi 1 X005905.97-282701.5 xmm mos1 275.178 263.127 107.2 15.5022 0.0279801 0.00404621 23.3024 1 10.875 10.875 0 3.06541 F F 7.85066 0 1 d
Report srcpi bgdpi 3 X005837.25-282716.6 xmm mos2 362.236 260.116 104.731 14.9296 0.0267808 0.00381766 22.3369 1 10.875 10.875 0 5.39567 F F 7.93042 0 1 d
Report srcpi bgdpi 2 X005836.85-282708.8 xmm mos1 363.459 261.642 11.4777 5.71326 0.0161246 0.00802633 2.49494 0.989724 6.91422 6.91422 0 5.37708 F F 7.93051 0 1 ds
Report srcpi bgdpi 2 X005906.10-282659.4 xmm mos2 274.78 263.811 21.8769 6.62275 0.0284855 0.00862336 4.66588 0.999977 10.2937 6.07206 90 3.08089 F F 7.85041 0 1 dbs

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