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 arf rmf 1 X053850.54-440508.0 xmm pn 315.822 314.227 12528.2 124.747 1.12322 0.0111843 227.459 1 5.79126 5.79126 0 1.70508 F F 1.08914 2.38789e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X053850.61-440508.4 xmm mos2 315.657 314.145 6238.79 88.9628 0.399526 0.00569709 211.565 1 5.43996 5.08952 12.8398 1.69609 F F 1.08902 3.92508e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X053850.63-440508.8 xmm mos1 315.612 314.053 6178.7 89.1171 0.395801 0.00570874 204.244 1 5.30078 5.30078 0 1.69209 F F 1.089 3.57546e-12 1 dsxf
Report srcpi bgdpi arf 4 X053935.21-435354.8 xmm mos2 204.894 468.725 61.0099 9.58235 0.00390694 0.000613634 2.06893 0.979716 10.875 10.875 0 14.086 F F 0.927036 1.60951e-13 1 dpx
Report srcpi bgdpi arf 3 X053750.52-440931.8 xmm mos2 464.279 253.078 52.3555 9.45279 0.00335274 0.000605337 1.77544 0.959861 10.875 10.875 0 12.4652 F F 1.27773 6.87485e-14 1 dx

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