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 2 X132938.61+582505.8 chandra ccd7 229.977 715.726 541.576 23.3985 0.114311 0.00493876 222.661 1 1.26481 0.674184 337.912 4.23341 A F 1.75e+20 0 1 ds
Report 1 X132805.33+581235.7 chandra ccd2 948.394 31.7126 60.2606 10.7709 0.0127193 0.00227343 88.6633 1 3.12163 2.61073 148.553 15.6427 F F 1.53e+20 0 1 d
Report 1 X132940.13+582453.9 chandra ccd7 205.167 691.056 8.6143 3.00001 0.00181823 0.000633216 3.54165 0.998777 0.689948 0.492 34.9845 3.99876 F F 1.75e+20 0 1 d
Report 2 X132950.94+581747.4 chandra ccd6 288.375 824.25 7.90451 2.82843 0.00166842 0.000597 12.4085 1 0.529819 0.492 139.594 3.24924 F F 1.68e+20 0 1 d
Report 1 X132957.94+581537.0 chandra ccd6 176 559.25 3.87598 2 0.000818108 0.000422144 6.0845 0.999934 0.72294 0.492 76.4252 5.58394 F F 1.67e+20 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