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 | X112326.32+090117.0 | chandra | ccd7 | 1014.17 | 1114.39 | 392.332 | 19.9127 | 0.0394811 | 0.00200385 | 279.429 | 1 | 2.13132 | 1.28389 | 321.953 | 5.95871 | 342.235 | 26.4699 | -0.856417 | 0.0724438 | F | F | 3.5e+20 | 2.33886e-13 | 1 | dsxf |
Report | srcpi bgdpi arf | 4 | X112328.09+085557.1 | chandra | ccd7 | 960.925 | 464.168 | 47.6371 | 7.19731 | 0.0047938 | 0.000724278 | 33.9284 | 1 | 0.430587 | 0.306331 | 326.681 | 1.18083 | 24.6975 | 21.9395 | -0.0591378 | 0.170295 | F | F | 3.58e+20 | 3.61605e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X112322.63+084807.1 | chandra | ccd6 | 616.867 | 397.357 | 44.7862 | 7.98212 | 0.0045069 | 0.000803253 | 24.9822 | 1 | 3.40455 | 1.87279 | 155.985 | 7.80463 | 34.3479 | 10.6711 | -0.525928 | 0.20078 | A | F | 3.64e+20 | 5.41317e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X112342.00+085949.2 | chandra | ccd7 | 541.993 | 935.915 | 36.6346 | 6.5956 | 0.0036866 | 0.000663726 | 26.0921 | 1 | 1.48963 | 0.495528 | 110.302 | 4.8896 | 18.831 | 17.493 | -0.0368349 | 0.19737 | A | F | 3.56e+20 | 3.0915e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X112325.62+090037.5 | chandra | ccd7 | 1035.33 | 1034.06 | 39.0546 | 6.24937 | 0.00393013 | 0.000628884 | 27.8157 | 1 | 2.07699 | 1.12046 | 334.436 | 5.37717 | 6.45188 | 32.2186 | 0.666315 | 0.232458 | F | F | 3.5e+20 | 3.58927e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 14 | X112337.27+085350.9 | chandra | ccd7 | 684.414 | 207.743 | 33.9877 | 5.8299 | 0.00342023 | 0.000586672 | 24.2069 | 1 | 0.648129 | 0.354706 | 52.9777 | 2.0439 | 20.9072 | 10.8608 | -0.316242 | 0.22267 | F | F | 3.62e+20 | 2.64692e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 8 | X112332.32+085542.8 | chandra | ccd7 | 833.602 | 435.087 | 24.6823 | 4.96813 | 0.00248382 | 0.00049995 | 17.5794 | 1 | 0.472995 | 0.284963 | 73.3396 | 0.194094 | 21.8979 | 2.89794 | -0.766256 | 0.309877 | F | F | 3.59e+20 | 1.86551e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 9 | X112343.55+085630.2 | chandra | ccd7 | 495.187 | 531.534 | 11.2939 | 3.36064 | 0.00113652 | 0.000338187 | 8.04381 | 1 | 1.0078 | 0.287589 | 87.9534 | 2.88708 | 9.85495 | 0.758252 | -0.857112 | 0.553978 | A | F | 3.61e+20 | 8.80743e-15 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X112330.84+085505.8 | chandra | ccd7 | 877.6 | 359.3 | 9.40715 | 4.27872 | 0.000946656 | 0.000430574 | 12.2176 | 1 | 0.492 | 0.492 | 26.5651 | 0.604794 | 5.83061 | 3.83061 | -0.207013 | 0.456272 | F | F | 3.59e+20 | 7.17547e-15 | 1 | dx |
Report | srcpi bgdpi arf | 13 | X112336.92+085922.7 | chandra | ccd7 | 694.4 | 881.5 | 9.60709 | 4.27872 | 0.000966776 | 0.000430574 | 15.3266 | 1 | 0.742655 | 0.492 | 82.7871 | 3.99828 | 6.94387 | 1.71935 | -0.603069 | 0.561061 | A | F | 3.55e+20 | 7.49046e-15 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X112337.55+085435.8 | chandra | ccd7 | 675.389 | 298.389 | 8.57653 | 4.1225 | 0.00086307 | 0.000414853 | 13.1796 | 1 | 0.492 | 0.492 | 148.073 | 1.54698 | 2.91531 | 5.91531 | 0.339727 | 0.497804 | F | F | 3.61e+20 | 6.59675e-15 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X112318.09+084657.7 | chandra | ccd6 | 753.75 | 256.333 | 12.6744 | 4.84057 | 0.00127545 | 0.000487114 | 11.0084 | 1 | 2.61699 | 1.01247 | 124.171 | 9.28161 | 8.67756 | 3.99686 | -0.369303 | 0.409854 | A | F | 3.65e+20 | 1.58158e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X112305.81+084905.1 | chandra | ccd6 | 1124.28 | 515.787 | 18.2788 | 4.66345 | 0.00183942 | 0.00046929 | 9.81409 | 1 | 3.72417 | 3.72417 | 0 | 9.24161 | 11.8832 | 8.00445 | -0.195035 | 0.322312 | F | F | 3.58e+20 | 2.33396e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 4 | X112319.85+084720.6 | chandra | ccd6 | 700.763 | 302.921 | 14.5585 | 5.4441 | 0.00146504 | 0.000547848 | 6.90793 | 1 | 2.99112 | 2.06992 | 61.3231 | 8.76545 | 5.66145 | 9.14037 | 0.235033 | 0.379767 | F | F | 3.65e+20 | 1.85035e-14 | 1 | dx |
Report | srcpi bgdpi arf | 10 | X112339.78+085700.4 | chandra | ccd7 | 608.3 | 592.3 | 4.66123 | 3.39792 | 0.000469066 | 0.000341937 | 8.0084 | 0.999998 | 0.492 | 0.492 | 45 | 2.31788 | 3.83061 | -0.0846933 | -1 | 1.19471 | F | F | 3.6e+20 | 3.5691e-15 | 1 | dx |
Report | srcpi bgdpi arf | 7 | X112330.70+085540.2 | chandra | ccd7 | 881.7 | 429.3 | 4.66123 | 3.39792 | 0.000469066 | 0.000341937 | 8.0084 | 0.999998 | 0.492 | 0.492 | 120.473 | 0.478264 | 3.91531 | 0.830613 | -0.649967 | 0.86687 | F | F | 3.59e+20 | 3.53183e-15 | 1 | dx |
Report | srcpi bgdpi arf | 12 | X112325.20+085848.1 | chandra | ccd7 | 1047.3 | 811.3 | 4.68964 | 3.39792 | 0.000471925 | 0.000341937 | 8.41791 | 0.999999 | 0.67235 | 0.492 | 156.801 | 3.74349 | -0.124145 | 3.87585 | 1 | 1.18077 | F | F | 3.53e+20 | 3.85549e-15 | 1 | dx |
Report | srcpi bgdpi arf | 11 | X112343.89+085259.7 | chandra | ccd7 | 484.3 | 103.1 | 5.77754 | 3.59808 | 0.000581403 | 0.00036208 | 12.2496 | 1 | 0.562179 | 0.492 | 125.28 | 3.77715 | 3 | 2.77754 | -0.0385036 | 0.631489 | F | F | 3.65e+20 | 5.36673e-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