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 X123049.11+122329.9 chandra ccd7 456.904 278.216 610.069 43.9224 0.129868 0.00934997 18.6527 1 1.5 0.367451 340.708 0.756244 A F 1.94e+20 8.2929e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.63+122332.6 chandra ccd7 471.331 283.741 1128.63 44.5471 0.240256 0.00948292 34.5076 1 0.637484 0.433611 340.464 0.725529 F F 1.93e+20 1.69102e-12 1 dsx
Report srcpi bgdpi arf 3 X123048.24+122335.1 chandra ccd7 482.711 288.812 67.5805 26.2718 0.0143862 0.00559259 2.06626 0.980104 0.566817 0.566817 0 0.710472 F F 1.93e+20 1.01201e-13 1 dsx
Report srcpi bgdpi arf 5 X123047.47+122348.1 chandra ccd7 505.811 315.285 92.7915 26.8129 0.0197529 0.00570779 2.83708 0.997461 2.771 0.346375 145.879 0.860065 A F 1.93e+20 1.38859e-13 1 dsx
Report srcpi bgdpi arf rmf 6 X123049.38+122328.6 chandra ccd7 449.017 275.595 7224.85 95.6545 1.53799 0.0203624 220.898 1 0.809489 0.577896 329.701 0.799489 T F 1.94e+20 1.08245e-11 1 dscpx

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