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 X090900.41+105934.9 chandra ccd3 662.794 980.765 979.073 31.9144 0.207667 0.00676921 220.439 1 1.38428 0.706483 80.4123 4.96655 A F 3.17e+20 2.63587e-12 1 dsxf
Report srcpi bgdpi arf rmf 6 X090923.58+105303.1 chandra ccd1 895.484 578.324 125.54 11.5406 0.0266276 0.00244782 45.4005 1 1.77112 0.89313 315.178 6.38815 F F 3.36e+20 2.10638e-13 1 dsxf
Report srcpi bgdpi arf 3 X090934.40+110549.4 chandra ccd2 68.684 798.942 43.2385 6.92292 0.00917113 0.00146839 19.9692 1 2.96113 1.76789 19.211 7.25611 F F 3.12e+20 1.1785e-13 1 dsx
Report srcpi bgdpi arf 1 X090948.44+105635.1 chandra ccd0 604.7 89.9399 23.8047 5.00002 0.00504906 0.00106052 40.964 1 1.58877 1.29246 15.685 7.38188 F F 3.32e+20 6.56681e-14 1 dpx
Report srcpi bgdpi arf 2 X090937.61+110617.0 chandra ccd0 929.29 1272.5 17.7264 4.35892 0.00375983 0.000924541 30.5042 1 2.12852 1.18805 123.73 8.04491 A T 3.12e+20 5.023e-14 1 dx
Report 3 X090932.74+110011.6 chandra ccd0 1075.11 530.195 18.0701 4.25089 0.00383276 0.000901636 31.0957 1 0.503532 0.503532 0 3.07522 F F 3.19e+20 0 1 ds
Report srcpi bgdpi arf 4 X090915.29+105547.2 chandra ccd3 217.565 517.896 14.9114 3.86153 0.00316278 0.000819049 3.35731 0.998809 0.905293 0.426112 110.738 3.84328 F F 3.26e+20 3.72363e-14 1 dsx
Report srcpi bgdpi arf 3 X090935.52+105211.4 chandra ccd1 537.357 472.786 13.6064 3.74166 0.00288595 0.000793619 4.92063 0.999983 1.44078 0.616938 20.6725 8.08279 A F 3.42e+20 3.86183e-14 1 dx
Report srcpi bgdpi arf 3 X090859.71+105931.4 chandra ccd3 683.278 973.167 8.36964 3.00001 0.00177523 0.000636313 1.88443 0.970361 0.6616 0.492 144.958 5.13698 F F 3.17e+20 2.23002e-14 1 dx
Report srcpi bgdpi arf 4 X090949.79+110517.4 chandra ccd0 564.611 1151.5 8.28759 3.00002 0.00175783 0.000636313 14.2616 1 1.93669 1.66377 99.8994 9.26747 F F 3.14e+20 2.44819e-14 1 dx
Report srcpi bgdpi arf 5 X090931.84+105922.1 chandra ccd0 1102.07 429.661 11.3445 3.36816 0.00240622 0.000714402 19.522 1 0.587743 0.587743 0 2.7506 F F 3.2e+20 2.72525e-14 1 dsx
Report srcpi bgdpi arf 4 X090928.64+105253.2 chandra ccd1 743.375 557.625 7.81821 2.82843 0.00165827 0.00059992 2.82739 0.994503 1.17415 0.492 45 6.80379 A F 3.38e+20 2.12918e-14 1 dx
Report srcpi bgdpi arf 1 X090909.34+110148.6 chandra ccd2 817.875 309 7.80382 2.82843 0.00165522 0.00059992 3.60411 0.998842 0.944166 0.492 116.847 3.67261 A F 3.14e+20 1.96122e-14 1 dx
Report srcpi bgdpi arf 6 X090928.85+110131.0 chandra ccd0 1191.1 691.1 4.9274 2.23607 0.00104512 0.000474278 8.47924 0.999998 0.492 0.492 2.8553 2.92319 F F 3.17e+20 1.1876e-14 1 dx
Report srcpi bgdpi arf 2 X090922.06+110231.1 chandra ccd2 437.5 395.3 4.87259 2.23607 0.00103349 0.000474278 2.25035 0.978119 0.741042 0.492 27.504 3.13787 A T 3.15e+20 1.16422e-14 1 dx
Report srcpi bgdpi arf 7 X090941.20+110002.6 chandra ccd0 821.5 511.5 1.91608 1.41422 0.000406408 0.00029996 3.29727 0.995007 0.492 0.492 90 5.08798 F F 3.21e+20 4.83886e-15 1 dx
Report 8 X090937.10+110002.6 chandra ccd0 944.25 511.5 3.93085 2 0.000833746 0.000424207 6.76434 0.999972 0.715907 0.492 8.70899 4.0915 F F 3.2e+20 0 1 d
Report srcpi bgdpi arf 9 X090937.49+110112.5 chandra ccd0 932.5 653.5 1.95758 1.41422 0.000415209 0.00029996 3.36867 0.995007 0.521845 0.492 45 4.51477 F F 3.17e+20 4.97528e-15 1 dx
Report 10 X090935.47+105803.1 chandra ccd0 993.1 268.5 4.93054 2.23607 0.00104578 0.000474278 8.48464 0.999998 0.492 0.492 122.492 3.88188 F F 3.24e+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