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 8 X224030.20+032130.8 chandra ccd7 294.67 296.042 1223.47 35.3066 0.1554 0.0044845 457.308 1 0.740813 0.740813 0 0.132556 T F 5.06e+20 1.06903e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X223925.78+032039.4 chandra ccd3 1055.96 360.352 379.979 25.7499 0.0482633 0.00327065 432.794 1 3.5098 3.2922 173.652 16.0233 F F 5.03e+20 7.11877e-13 1 dx
Report srcpi bgdpi arf 2 X224022.87+032451.0 chandra ccd7 517.902 703.026 60.3794 7.77042 0.00766916 0.000986969 22.5686 1 1.2002 0.645209 340.061 3.87291 A F 5.01e+20 5.86067e-14 1 dsx
Report srcpi bgdpi arf 3 X224019.21+032614.1 chandra ccd7 629.165 871.931 42.3902 6.51078 0.00538424 0.000826973 15.8446 1 1.25227 1.25227 0 5.52331 F F 5e+20 4.25848e-14 1 dsx
Report srcpi bgdpi arf 6 X224024.23+032638.8 chandra ccd7 476.539 922.002 18.744 5.60796 0.00238079 0.000712302 7.00612 1 1.46119 0.543535 339.697 5.45005 F F 5e+20 1.87739e-14 1 dsx
Report srcpi bgdpi arf 1 X224021.45+032442.0 chandra ccd7 561.006 684.729 13.4271 3.6643 0.00170545 0.000465424 5.01877 0.99998 1.03781 0.408952 347.822 3.91474 F F 5.01e+20 1.303e-14 1 dsx
Report srcpi bgdpi arf 7 X224027.69+032459.7 chandra ccd7 370.5 720.214 6.46465 2.64576 0.000821113 0.000336054 2.41635 0.984796 0.773344 0.534413 132.449 3.63574 F F 5.02e+20 6.25196e-15 1 dx
Report srcpi bgdpi arf 3 X224038.25+031504.3 chandra ccd6 412.072 461.928 6.43348 2.64576 0.000817153 0.000336054 7.82755 0.999999 1.31583 0.492 45.6774 6.66461 A F 5.16e+20 8.91676e-15 1 dx
Report srcpi bgdpi arf 2 X224036.55+031518.9 chandra ccd6 463.928 491.643 6.20008 2.64577 0.000787508 0.000336055 7.54358 0.999993 1.343 0.709043 51.5432 6.30882 A F 5.15e+20 8.5743e-15 1 dx
Report 2 X223958.66+032041.9 chandra ccd3 55.2998 365.3 4.72602 2.23608 0.000600279 0.000284017 5.38292 0.999849 0.492 0.492 45 7.83225 F F 5.04e+20 0 1 d
Report 1 X224028.57+031850.3 chandra ccd6 706.75 921.25 3.90995 2 0.000496626 0.000254032 4.7572 0.999329 0.492 0.492 110.593 2.58623 F F 5.1e+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