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 10 X225030.34+105322.7 chandra ccd7 385.783 481.594 108.108 10.6617 0.0136175 0.00134297 17.9417 1 0.479863 0.479863 0 1.2647 F F 4.74e+20 9.63761e-14 1 dsxf
Report srcpi bgdpi arf rmf 1 X225046.68+103753.4 chandra ccd5 860.554 448.322 102.309 15.8437 0.0128871 0.00199572 66.8177 1 5.4867 5.11311 139.197 15.729 F F 4.81e+20 1.41295e-13 1 dx
Report srcpi bgdpi arf 3 X225019.43+105413.8 chandra ccd7 712.592 585.404 45.381 14.6347 0.00571629 0.00184342 7.53147 1 0.896184 0.896184 0 2.1531 F F 4.73e+20 4.31048e-14 1 dsx
Report srcpi bgdpi arf 1 X224946.66+104311.7 chandra ccd2 872.778 631.403 76.0121 10.909 0.00957485 0.00137416 99.1199 1 4.48375 3.97188 123.804 13.5702 F F 4.71e+20 1.3779e-13 1 dx
Report srcpi bgdpi arf 1 X225033.77+105324.3 chandra ccd7 283.196 484.743 21.545 4.64166 0.00271386 0.000584675 3.57562 0.999451 0.530813 0.530813 0 2.0494 F F 4.75e+20 2.08953e-14 1 dsx
Report srcpi bgdpi arf 5 X225013.26+105410.4 chandra ccd7 897.109 578.48 17.0133 4.91838 0.00214304 0.000619532 2.82354 0.996422 0.838302 0.838302 0 3.39644 F F 4.72e+20 1.72897e-14 1 dsx
Report srcpi bgdpi arf 8 X225026.40+105706.1 chandra ccd7 503.957 935.684 14.3974 3.79439 0.00181353 0.000477949 2.3894 0.987739 1.08557 0.496677 157.165 4.34112 F F 4.73e+20 1.43051e-14 1 dsx
Report srcpi bgdpi arf 2 X225004.69+104650.3 chandra ccd2 332.5 1075.67 5.58696 2.4495 0.00070376 0.000308551 7.2854 0.999997 0.966776 0.492 168.818 7.87835 A F 4.72e+20 9.58997e-15 1 dx
Report srcpi bgdpi arf 3 X225007.25+104430.5 chandra ccd2 256.039 791.346 10.6106 3.60559 0.00133657 0.000454177 13.8363 1 3.87729 1.66791 93.9766 9.43408 A F 4.72e+20 1.94031e-14 1 dx
Report 2 X225044.95+104937.4 chandra ccd6 435.833 945.167 2.9532 1.73205 0.000371996 0.000218176 3.4985 0.993883 0.492 0.492 90 5.64513 F F 4.78e+20 0 1 d
Report srcpi bgdpi arf 1 X225027.86+104658.7 chandra ccd6 947.5 622.5 2.90396 1.73205 0.000365793 0.000218176 3.44017 0.993883 0.492 0.492 45 5.80633 F F 4.75e+20 4.51686e-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