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 X145453.53+032456.8 chandra ccd7 533.572 945.223 445.281 21.3903 0.0701871 0.00337163 229.627 1 0.443099 0.392731 91.5775 0.289307 F F 3.71e+20 4.84889e-13 1 dsxf
Report srcpi bgdpi arf 3 X145527.17+031448.3 chandra ccd3 522.197 613.986 71.7425 10.4406 0.0113083 0.00164568 94.321 1 7.28849 6.5338 51.9506 13.3893 F F 3.85e+20 1.62192e-13 1 dx
Report srcpi bgdpi arf 2 X145503.00+032429.8 chandra ccd7 245.338 890.37 28.567 5.34481 0.00450286 0.000842472 14.7317 1 0.8158 0.410178 334.137 2.47506 F F 3.74e+20 3.47002e-14 1 dsx
Report srcpi bgdpi arf 1 X145509.56+033704.4 chandra ccd5 1236.27 705.568 20.2761 6.63353 0.00319598 0.0010456 13.751 1 6.90498 3.60315 139.984 12.4946 A F 3.7e+20 3.40942e-14 1 dx
Report srcpi bgdpi arf 4 X145437.50+032425.7 chandra ccd7 1021.37 882.065 19.4648 4.41189 0.00306812 0.00069542 10.0378 1 0.742013 0.742013 0 4.0815 F F 3.67e+20 2.48748e-14 1 dsx
Report srcpi bgdpi arf 2 X145533.82+033742.9 chandra ccd5 498.056 784 18.4319 6.00023 0.0029053 0.000945776 12.5003 1 4.30123 3.33036 73.5858 16.0255 F F 3.8e+20 3.09304e-14 1 dx
Report srcpi bgdpi arf 1 X145528.93+032436.0 chandra ccd2 1075.13 985.945 14.304 4.16892 0.00225466 0.000657122 8.15589 1 2.61003 2.61003 0 8.85958 F F 3.84e+20 3.3861e-14 1 dsx
Report srcpi bgdpi arf 2 X145521.09+031426.4 chandra ccd3 707.088 569.382 11.4599 4.12321 0.00180634 0.000649914 15.0665 1 5.20699 4.21941 88.0673 12.8016 F F 3.83e+20 2.61647e-14 1 dx
Report srcpi bgdpi arf 3 X145452.69+032619.5 chandra ccd7 559.104 1113.24 10.3035 3.61683 0.00162408 0.0005701 5.31342 0.99999 0.957691 0.957691 0 1.10937 F F 3.7e+20 1.22425e-14 1 dsx
Report srcpi bgdpi arf 7 X145503.25+032236.8 chandra ccd7 237.125 660.25 7.66243 2.82843 0.00120778 0.000445827 3.95145 0.999459 0.597527 0.492 47.8123 3.57225 F F 3.75e+20 9.9864e-15 1 dx
Report srcpi bgdpi arf 1 X145518.41+031803.5 chandra ccd3 788.9 1010.7 5.76001 2.64578 0.000907913 0.000417036 7.57278 0.999997 0.532296 0.492 115.264 9.48989 F F 3.83e+20 1.29781e-14 1 dx
Report srcpi bgdpi arf 5 X145454.91+032544.2 chandra ccd7 491.167 1041 5.7348 2.4495 0.000903939 0.000386098 2.95739 0.994594 0.492 0.492 54.9276 0.606524 F F 3.71e+20 6.79059e-15 1 dx
Report srcpi bgdpi arf 2 X145508.51+032628.5 chandra ccd6 669.3 272.1 4.86833 2.23607 0.000767363 0.000352457 6.40285 0.999968 0.645067 0.492 10.4623 3.9368 F F 3.75e+20 8.46515e-15 1 dx
Report srcpi bgdpi arf 1 X145505.16+032749.1 chandra ccd6 771 436 3.94145 2 0.000621266 0.000315247 5.18382 0.999666 0.492 0.492 45 3.88563 F F 3.73e+20 7.08222e-15 1 dx
Report srcpi bgdpi arf 6 X145443.72+032417.7 chandra ccd7 831.5 865.25 3.80043 2.00001 0.000599036 0.000315248 1.95985 0.961876 0.600932 0.492 114.922 2.62233 F F 3.69e+20 4.55486e-15 1 dx
Report 5 X145506.39+033146.8 chandra ccd6 733.75 919 3.7799 2.00001 0.000595802 0.000315248 4.97135 0.999666 0.492 0.492 52.0181 7.28777 F F 3.72e+20 0 1 d
Report srcpi bgdpi arf 4 X145453.42+033132.8 chandra ccd6 1128.5 890.5 3.5242 2.00001 0.000555496 0.000315249 4.63504 0.999666 0.492 0.492 90 6.30997 F F 3.68e+20 8.59092e-15 1 dx
Report 3 X145514.17+032916.5 chandra ccd6 496.833 613.5 2.72819 1.73206 0.000430026 0.000273013 3.58812 0.997056 0.621484 0.492 104.305 6.54538 F F 3.76e+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