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 X042957.74+033433.4 chandra ccd6 645.125 663.375 7.49337 2.82844 0.00226958 0.000856673 14.4229 1 1.25486 0.867659 66.5559 6.17628 F F 1.07e+21 2.4791e-14 1 dx
Report srcpi bgdpi arf 1 X042905.20+034051.6 chandra ccd3 482.786 1149.21 6.42009 2.64577 0.00194451 0.000801345 13.1026 1 1.81 1.3696 60.9304 9.94146 F F 1.1e+21 2.73025e-14 1 dx
Report 2 X042908.09+033522.8 chandra ccd3 394.833 480.833 5.59548 2.4495 0.00169475 0.0007419 11.4196 1 0.492 0.492 170.783 10.1875 F T 1.1e+21 0 1 d
Report 1 X042919.92+033037.7 chandra ccd2 611 762.25 3.82165 2 0.00115749 0.000605758 7.96276 0.999996 1.28986 0.882412 66.526 11.1015 F F 1.09e+21 0 1 d
Report srcpi bgdpi arf 2 X042915.87+032731.4 chandra ccd2 734.167 383.667 5.1215 2.44951 0.00155119 0.000741904 10.6711 1 1.52499 0.668437 43.4421 14.2677 A T 1.08e+21 2.2062e-14 1 dx
Report 1 X042947.19+034444.0 chandra ccd7 443.167 1009.5 2.89675 1.73205 0.000877364 0.000524602 3.73109 0.996587 0.492 0.492 161.565 4.94292 F F 1.08e+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