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 1 X190532.79+065933.5 chandra ccd7 927.115 596.689 19.1189 4.69446 0.00889906 0.00218508 15.8254 1 0.303559 0.303559 0 0.761121 F F 1.55e+22 1.23662e-13 1 dsx
Report srcpi bgdpi arf 4 X190546.92+065737.7 chandra ccd7 499.405 361.283 18.5879 4.31137 0.00865191 0.00200677 15.3859 1 1.05961 0.439954 230.714 3.4483 F F 1.54e+22 1.23171e-13 1 dsx
Report 1 X190518.19+065536.0 chandra ccd6 309.5 263.5 3.97107 2 0.00184835 0.000930906 9.10719 0.999998 0.492 0.492 90 5.0831 F F 1.55e+22 0 1 d
Report srcpi bgdpi arf 1 X190544.39+070828.7 chandra ccd3 552.5 320 3.60489 2.00001 0.00167791 0.000930911 8.71732 0.999969 1.50005 0.956872 2.92801 9.9705 A F 1.54e+22 3.37439e-14 1 dx
Report srcpi bgdpi arf 2 X190540.32+070709.6 chandra ccd3 676.266 159.771 23.2062 4.81728 0.0108015 0.00224225 56.117 1 3.86617 1.36712 113.068 8.45956 A F 1.55e+22 2.02195e-13 1 dsx
Report 2 X190602.57+065631.1 chandra ccd7 25.1667 225.5 2.85424 1.73206 0.00132851 0.000806191 2.36256 0.983265 0.561105 0.492 64.9028 7.48108 F F 1.53e+22 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 - 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