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 9 X123417.49+615521.0 chandra ccd7 856.791 514.297 31.0622 5.57335 0.00505736 0.000907418 16.8172 1 0.962238 0.962238 0 3.37479 F F 1.16e+20 3.84465e-14 1 dsx
Report srcpi bgdpi arf 5 X123450.76+615418.8 chandra ccd7 378.989 388.515 30.6417 5.98987 0.00498889 0.000975233 16.5895 1 2.02449 2.02449 0 6.49589 F F 1.15e+20 3.99077e-14 1 dsx
Report srcpi bgdpi arf 1 X123450.73+621015.5 chandra ccd2 615.573 723.018 33.5593 8.27089 0.0054639 0.00134661 5.68489 1 8.12921 5.25257 58.6269 12.6504 F F 1.07e+20 7.86569e-14 1 dsx
Report srcpi bgdpi arf 2 X123411.77+615832.5 chandra ccd7 938.942 903.507 15.6889 4.30659 0.00255436 0.000701169 8.49403 1 0.405682 0.405682 0 0.302157 F T 1.15e+20 1.87166e-14 1 dsx
Report srcpi bgdpi arf 6 X123426.66+615431.9 chandra ccd7 725.024 414.568 15.0797 4.54219 0.00245518 0.00073953 8.16421 1 1.72174 0.434459 349.128 4.54946 F F 1.16e+20 1.89019e-14 1 dsx
Report srcpi bgdpi arf 8 X123455.70+615442.9 chandra ccd7 307.7 437.3 13.0123 3.87302 0.00211857 0.000630576 7.04493 1 1.80338 0.86552 140.435 6.69618 A F 1.14e+20 1.71028e-14 1 dx
Report srcpi bgdpi arf 4 X123433.91+615311.8 chandra ccd7 620.269 251.346 11.3748 3.60558 0.00185197 0.000587034 6.15838 0.999997 1.162 0.874923 30.7641 6.12001 F F 1.16e+20 1.48266e-14 1 dx
Report srcpi bgdpi arf 1 X123609.70+620508.1 chandra ccd3 273.346 765.654 10.1597 3.60561 0.00165412 0.000587039 13.7685 1 3.61414 2.25684 34.1219 15.572 A F 1.06e+20 2.59502e-14 1 dx
Report srcpi bgdpi arf 3 X123403.79+620004.2 chandra ccd7 1052.6 1089.4 9.71865 3.16228 0.00158232 0.00051486 5.26172 0.999986 0.496219 0.492 143.082 1.61787 F F 1.15e+20 1.48956e-14 1 dx
Report srcpi bgdpi arf 1 X123417.70+615823.4 chandra ccd7 853.5 884.5 7.71067 2.82843 0.00125539 0.000460505 4.17458 0.99977 0.492 0.492 90 1.01476 F F 1.16e+20 9.19471e-15 1 dx
Report srcpi bgdpi arf 6 X123342.33+615949.0 chandra ccd6 562.833 382.833 5.87915 2.44949 0.000957699 0.000399016 7.74007 0.999997 0.492 0.492 150.482 3.38936 F F 1.18e+20 1.05427e-14 1 dx
Report srcpi bgdpi arf 2 X123352.75+620146.4 chandra ccd6 413.5 621.167 5.82842 2.44949 0.000949435 0.000399017 7.67328 0.999997 0.730571 0.492 84.6902 3.72997 F T 1.16e+20 1.04825e-14 1 dx
Report srcpi bgdpi arf 3 X123357.44+620215.9 chandra ccd6 346.333 681.167 5.77565 2.4495 0.000940839 0.000399017 7.60381 0.999997 0.644939 0.492 119.321 3.93332 F F 1.15e+20 1.04708e-14 1 dx
Report srcpi bgdpi arf 4 X123309.38+620101.7 chandra ccd6 1033.9 531.9 4.48704 2.23608 0.000730928 0.000364252 5.90732 0.999969 1.05828 0.502543 138.607 7.43675 A F 1.21e+20 9.5984e-15 1 dx
Report srcpi bgdpi arf 5 X123343.99+620147.9 chandra ccd6 538.75 624.5 3.90458 2 0.000636047 0.000325796 5.1405 0.999669 0.521845 0.492 90 4.37143 F F 1.17e+20 7.1259e-15 1 dx
Report 1 X123321.56+620215.1 chandra ccd6 859.25 680.5 3.77497 2.00001 0.000614933 0.000325796 4.96986 0.999669 0.492 0.492 180 6.68817 F F 1.19e+20 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