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 X123048.92+122330.3 chandra ccd7 104.112 745.821 151.275 39.1199 0.0348803 0.00902009 4.9698 0.999999 1.1 1.1 0 0.765753 T F 1.94e+20 2.14628e-13 1 dsxf
Report srcpi bgdpi arf rmf 2 X123048.62+122332.3 chandra ccd7 112.969 749.842 921.922 41.0816 0.212572 0.00947239 30.2877 1 0.515293 0.515293 0 0.730406 F F 1.93e+20 1.52176e-12 1 dsx
Report srcpi bgdpi arf 3 X123048.23+122335.1 chandra ccd7 124.566 755.617 66.4074 24.9678 0.0153119 0.00575695 2.18167 0.984141 0.663047 0.663047 0 0.712648 F F 1.93e+20 1.09496e-13 1 dsx
Report srcpi bgdpi arf rmf 6 X123049.65+122318.9 chandra ccd7 82.5033 722.681 102.522 21.4781 0.023639 0.00495231 3.36813 0.999563 1.5 1.5 0 0.92611 T F 1.94e+20 1.69348e-13 1 dsx
Report srcpi bgdpi arf rmf 7 X123049.38+122328.2 chandra ccd7 90.5651 741.622 8235.14 99.0309 1.89882 0.0228341 270.547 1 0.533813 0.533813 0 0.769673 F F 1.94e+20 1.35774e-11 1 dsx

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