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 4 X121037.06+102503.8 chandra ccd7 513.7 636.5 4.9845 2.23607 0.00420702 0.00188729 15.829 1 0.504455 0.492 15.2328 3.01205 F F 1.75e+20 0 1 d
Report 2 X121040.64+102723.0 chandra ccd7 406.3 919.5 4.94272 2.23607 0.00417175 0.00188729 15.6963 1 0.5904 0.492 180 5.48877 F F 1.76e+20 0 1 d
Report 1 X121016.25+102217.1 chandra ccd7 1137.83 297.833 2.98458 1.73205 0.00251905 0.00146189 9.47798 0.999996 0.492 0.492 45 3.80402 F F 1.72e+20 0 1 d
Report 1 X120950.53+103041.6 chandra ccd3 608.5 778.5 2 1.41421 0.00168804 0.00119363 12.5035 0.999997 2.47533 0.492 116.565 13.1182 A F 1.74e+20 0 1 d
Report srcpi bgdpi arf 1 X120936.52+102023.0 chandra ccd2 777.5 550.5 0.998347 1 0.000842625 0.000844021 5.87385 0.999591 0.492 0.492 90 13.7164 F F 1.6e+20 1.09043e-14 1 dx
Report srcpi bgdpi arf 3 X121036.47+102631.3 chandra ccd7 531.5 814.5 0.987264 1 0.000833271 0.000844021 3.1352 0.995397 0.492 0.492 90 4.33033 F F 1.76e+20 4.84387e-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