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 | 2 | X113850.78+034216.3 | chandra | ccd2 | 1081.13 | 702.833 | 26.5279 | 6.26783 | 0.00528838 | 0.0012495 | 38.6076 | 1 | 2.16133 | 1.00427 | 112.936 | 7.85729 | 0.881968 | 25.6852 | 0.933605 | 0.323979 | A | F | 1.85e+20 | 7.9855e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X113932.78+032834.6 | chandra | ccd1 | 413.486 | 366.2 | 26.877 | 5.1843 | 0.00535479 | 0.00103289 | 46.2981 | 1 | 4.1517 | 2.695 | 323.88 | 9.44884 | 18.0106 | 6.74646 | -0.454988 | 0.283354 | F | F | 1.85e+20 | 7.80574e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X113855.68+033050.2 | chandra | ccd3 | 552.024 | 258.214 | 20.6974 | 5.66369 | 0.00412349 | 0.00112836 | 37.6271 | 1 | 1.87227 | 0.955776 | 135.355 | 6.98604 | 8.91355 | 11.8271 | 0.140475 | 0.277054 | A | F | 1.86e+20 | 5.61661e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X113910.65+034542.0 | chandra | ccd2 | 476.5 | 1120.93 | 13.4526 | 4.84057 | 0.0026818 | 0.000964978 | 18.1824 | 1 | 1.84908 | 1.70779 | 19.132 | 9.21524 | 7 | 5.45259 | -0.124264 | 0.383705 | F | F | 1.84e+20 | 4.68237e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X113853.38+033100.2 | chandra | ccd3 | 621.917 | 278.583 | 12.7121 | 4.7081 | 0.00253259 | 0.000937982 | 23.6912 | 1 | 1.41106 | 0.799659 | 28.1772 | 7.20912 | 10.952 | 1.80806 | -0.716607 | 0.457164 | A | F | 1.86e+20 | 3.49207e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X113858.51+034148.4 | chandra | ccd2 | 845.864 | 646.045 | 11.5262 | 4.57071 | 0.00229778 | 0.000911181 | 16.7458 | 1 | 1.49941 | 0.645351 | 139.239 | 6.30519 | 7.89067 | 3.67201 | -0.364852 | 0.423995 | A | F | 1.85e+20 | 3.22402e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X113909.10+032952.3 | chandra | ccd1 | 1133.75 | 523.5 | 7.77386 | 3.95804 | 0.00154879 | 0.000788562 | 16.3473 | 1 | 1.10542 | 0.492 | 43.5268 | 6.6641 | 1.92462 | 5.88693 | 0.507237 | 0.57417 | A | F | 1.86e+20 | 2.04672e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X113913.41+032854.8 | chandra | ccd1 | 1002.38 | 406.625 | 7.83834 | 3.95804 | 0.00156164 | 0.000788562 | 19.4948 | 1 | 1.82285 | 0.497196 | 70.3915 | 7.58684 | 4 | 3.86143 | -0.0176263 | 0.508892 | A | F | 1.86e+20 | 2.12696e-14 | 1 | dx |
| Report | 5 | X113852.40+034415.6 | chandra | ccd2 | 1031.67 | 945.333 | 5.40742 | 2.44951 | 0.00107798 | 0.000488314 | 9.28319 | 0.999998 | 0.492 | 0.492 | 45 | 9.19366 | F | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | 6 | X113905.32+033606.6 | chandra | ccd3 | 258.7 | 901.3 | 4.96682 | 2.23607 | 0.000989526 | 0.000445486 | 8.65866 | 0.999999 | 0.492 | 0.492 | 172.534 | 1.73766 | F | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X113927.20+033423.3 | chandra | ccd1 | 583 | 1074.5 | 3.91531 | 3.17945 | 0.000780048 | 0.000633443 | 13.4537 | 1 | 0.492 | 0.492 | 2.35032e-08 | 4.31162 | 2 | 1.91531 | -0.0216313 | 0.82671 | F | F | 1.85e+20 | 9.91506e-15 | 1 | dx |
| Report | 5 | X113856.76+033736.6 | chandra | ccd3 | 519.25 | 1084.25 | 3.93513 | 2 | 0.000783986 | 0.000398455 | 6.86012 | 0.999976 | 0.492 | 0.492 | 45 | 3.99102 | F | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | 2 | X113930.07+033129.8 | chandra | ccd1 | 495.5 | 721.75 | 3.74955 | 2.00001 | 0.000747024 | 0.000398462 | 6.45894 | 0.999973 | 0.917428 | 0.492 | 21.2765 | 6.71123 | A | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X113910.34+034317.1 | chandra | ccd2 | 486 | 826.25 | 3.8821 | 3.17945 | 0.000773904 | 0.00063383 | 11.3058 | 1 | 1.41332 | 0.492 | 56.9677 | 6.80607 | 1.97052 | 1.94105 | -0.00753557 | 0.82733 | A | F | 1.84e+20 | 1.10578e-14 | 1 | dx |
| Report | 3 | X113851.57+033641.8 | chandra | ccd3 | 677.167 | 972.833 | 2.95432 | 1.73205 | 0.000588581 | 0.000345072 | 5.15027 | 0.999624 | 0.492 | 0.492 | 90 | 5.13041 | F | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | 4 | X113909.94+033605.2 | chandra | ccd3 | 118.167 | 898.5 | 2.91491 | 1.73205 | 0.000580729 | 0.000345072 | 5.08156 | 0.999624 | 0.602575 | 0.492 | 90 | 0.677593 | T | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | 6 | X113900.93+034148.4 | chandra | ccd2 | 772.167 | 646.167 | 2.87774 | 1.73206 | 0.000573683 | 0.000345289 | 4.94036 | 0.999578 | 0.492 | 0.492 | 45 | 6.00245 | F | F | 1.85e+20 | 0 | 1 | d | |||||
| Report | 1 | X113938.44+033505.3 | chandra | ccd0 | 605.833 | 181.833 | 2.8031 | 1.73206 | 0.000558813 | 0.000345294 | 5.03237 | 0.999698 | 0.629173 | 0.492 | 4.73116 | 6.71783 | F | F | 1.84e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X113934.66+033852.8 | chandra | ccd0 | 721 | 644.25 | 3.88926 | 3.17945 | 0.000775343 | 0.00063384 | 11.6871 | 1 | 1.12841 | 0.492 | 112.04 | 6.11119 | 0.963085 | 2.92617 | 0.504746 | 0.932036 | A | F | 1.84e+20 | 1.03994e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X113938.59+033644.3 | chandra | ccd0 | 601.239 | 382.935 | 22.6024 | 5.8734 | 0.0045059 | 0.00117089 | 35.8446 | 1 | 1.80553 | 0.847847 | 165.141 | 6.6118 | 14.8012 | 7.76143 | -0.31201 | 0.27388 | A | F | 1.84e+20 | 5.97727e-14 | 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