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 1 X191333.64+171723.9 chandra ccd6 1078 974.833 5.97914 2.44949 0.00411401 0.0016854 22.3507 1 0.556816 0.492 80.6617 2.20682 F F 6.36e+21 0 1 d
Report 4 X191335.31+171428.4 chandra ccd6 1029.5 618.25 3.99122 2 0.0027462 0.00137612 14.9196 1 0.492 0.492 25.4531 5.10474 F F 6.4e+21 0 1 d
Report 2 X191352.08+171228.1 chandra ccd6 541.167 373.833 2.99991 1.73205 0.00206412 0.00119176 11.214 0.999999 0.678773 0.492 65.9936 8.73862 F F 6.58e+21 0 1 d
Report 1 X191254.38+171742.1 chandra ccd3 380.833 1094.17 2.97862 1.73205 0.00204947 0.00119176 11.3107 0.999999 0.492 0.492 45 8.63096 F F 6.11e+21 0 1 d
Report 1 X191321.13+170539.0 chandra ccd2 315.5 355.167 2.7163 1.73207 0.00186898 0.00119177 10.7051 0.999958 1.84053 1.16746 40.2688 13.9144 A F 6.48e+21 0 1 d
Report 3 X191403.10+171655.0 chandra ccd6 220.5 916.5 0.999992 1 0.000688055 0.00068806 3.73808 0.997558 0.492 0.492 90 8.32251 F F 6.62e+21 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