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 X181800.45+742857.6 xmm pn 385.302 238.812 192.842 61.339 0.016682 0.00530619 3.22768 0.999319 4.85771 3.65933 359.952 7.61944 F F 8.29138 1.10536e-13 1 dsxf
Report srcpi bgdpi arf 3 X181800.66+742856.8 xmm mos2 385.111 238.636 56.8991 25.4361 0.00398639 0.00178207 2.34231 0.989081 3.78442 3.78442 0 7.65454 F F 8.29233 1.01948e-13 1 dsx
Report srcpi bgdpi arf 2 X181838.05+743346.8 xmm mos1 350.345 305.447 82.6878 15.426 0.00721786 0.00134654 0 10.875 10.875 0 3.79748 F F 8.25027 8.90108e-14 1 dx
Report srcpi bgdpi arf 1 X181951.29+743503.5 xmm mos2 283.144 324.069 83.7518 14.7206 0.00605759 0.00106471 3.44773 0.999616 10.875 10.875 0 2.16398 F F 8.16913 5.78265e-14 1 dpbx
Report srcpi bgdpi arf 1 X182015.63+742052.2 xmm mos1 260.273 127.088 70.0999 15.0317 0.00449127 0.000963077 0 10.875 10.875 0 12.7272 F F 8.14061 1.46615e-13 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