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 3 X100443.47+480156.6 chandra ccd7 756.994 443.114 366.32 19.6789 0.0424584 0.00228089 113.215 1 0.390959 0.390959 0 0.129313 F F 8.86e+19 0 1 ds
Report 1 X100518.53+475903.5 chandra ccd7 40.95 91.45 36.7691 6.3246 0.00426171 0.000733052 11.3639 1 1.49215 0.947473 175.713 6.61813 A F 8.57e+19 0 1 d
Report 1 X100531.18+480746.3 chandra ccd3 445.656 220.625 25.35 5.65693 0.00293819 0.000655665 30.7287 1 3.61546 2.94456 167.067 9.82164 F F 8.89e+19 0 1 d
Report 2 X100530.01+480641.6 chandra ccd3 469 88.8999 14.2749 4.47225 0.00165453 0.000518355 17.3037 1 3.06387 1.71287 113.445 9.07023 A F 8.86e+19 0 1 d
Report 2 X100518.96+475905.8 chandra ccd7 32.1667 96.1667 11.811 3.60558 0.00136896 0.000417904 3.65032 0.999452 0.492 0.492 45 6.66506 F F 8.57e+19 0 1 d
Report 4 X100501.64+480047.9 chandra ccd7 386.443 303.679 12.1157 3.48076 0.00140427 0.000403439 3.74448 0.999452 0.530761 0.530761 0 3.31985 F F 8.75e+19 0 1 ds

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