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 X111816.96+074558.2 chandra ccd7 179.46 818.053 488.187 25.0025 0.0334776 0.00171455 79.683 1 0.4692 0.4692 0 0.296745 F F 3.57e+20 3.11756e-13 1 dsxf
Report srcpi bgdpi arf 4 X111812.05+074031.0 chandra ccd7 327.988 152.992 31.3919 5.96064 0.00215271 0.000408752 5.12386 0.999997 1.35013 1.35013 0 5.83836 F F 3.66e+20 1.71111e-14 1 dsx
Report srcpi bgdpi arf 5 X111815.10+074158.8 chandra ccd7 235.748 331.432 13.0175 3.60798 0.000892677 0.000247418 2.12475 0.979073 1.22608 0.51646 297.034 4.28079 F F 3.63e+20 6.8796e-15 1 dsx
Report srcpi bgdpi arf 6 X111816.16+074315.5 chandra ccd7 203.602 487.308 80.6781 9.4734 0.00553253 0.000649641 13.1685 1 0.71165 0.428471 312.137 2.99635 A F 3.6e+20 4.21004e-14 1 dsx

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 - 7.99 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), T = 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