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 rmf 1 X123049.18+122329.1 chandra ccd7 671.712 212.125 633.37 38.3525 0.134776 0.00816109 22.9242 1 1.23067 1.23067 0 0.300864 T F 1.94e+20 9.16805e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123049.01+122329.7 chandra ccd7 676.708 213.393 289.527 33.8498 0.061609 0.00720296 10.4791 1 1.3548 1.3548 0 0.293993 T F 1.94e+20 4.58717e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.4 chandra ccd7 687.994 218.813 835.575 39.1344 0.177803 0.00832748 30.2428 1 0.492335 0.492335 0 0.314851 F F 1.93e+20 1.32101e-12 1 dscx
Report srcpi bgdpi arf rmf 4 X123048.40+122333.8 chandra ccd7 694.748 221.748 123.701 25.7968 0.0263226 0.00548936 4.47723 0.999994 1.5 1.5 0 0.367833 T F 1.93e+20 1.95564e-13 1 dscx
Report srcpi bgdpi arf rmf 8 X123049.41+122328.2 chandra ccd7 664.837 210.24 3346.3 65.0504 0.712064 0.0138422 121.116 1 0.690389 0.412654 335.24 0.315317 A F 1.94e+20 5.30147e-12 1 dscx

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