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 arf 1 X112646.92+432525.3 chandra ccd3 633.542 627.042 18.2079 4.89908 0.0104024 0.00279891 54.1452 1 8.31293 3.81575 49.4789 12.2145 A F 2.45e+20 1.21118e-13 1 dx
Report srcpi bgdpi arf 3 X112607.34+433406.2 chandra ccd7 692.034 675.839 13.5538 4.5921 0.00774354 0.00262355 4.93811 0.999986 0.438081 0.438081 0 2.53556 F F 2.38e+20 4.18117e-14 1 dsx
Report srcpi bgdpi arf 2 X112557.98+433242.1 chandra ccd7 898.278 504.5 8.08937 3.00002 0.00462157 0.00171395 2.94723 0.995199 0.735125 0.492 55.2282 4.68794 F F 2.39e+20 2.49296e-14 1 dx
Report arf 2 X112636.57+433912.2 chandra ccd6 689.5 501.5 0.979411 1 0.000559551 0.000571315 2.66204 0.991625 0.492 0.492 90 4.8939 F F 2.32e+20 5.16208e-15 1 dx
Report arf 1 X112635.59+434302.5 chandra ccd6 711.5 969.5 0.932995 1 0.000533033 0.000571316 2.53588 0.991625 0.492 0.492 90 7.77115 F F 2.3e+20 5.17738e-15 1 dx

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