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 | X011200.39-011645.2 | chandra | ccd3 | 193.618 | 702.059 | 31.32 | 5.83098 | 0.00532962 | 0.000992239 | 51.224 | 1 | 2.13216 | 1.62173 | 118.195 | 8.07796 | F | F | 4.77e+20 | 6.90515e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X011230.14-011407.7 | chandra | ccd7 | 456.374 | 323.646 | 20.7052 | 4.5503 | 0.00352141 | 0.000773886 | 20.8108 | 1 | 0.316699 | 0.316699 | 0 | 1.31015 | F | F | 4.73e+20 | 2.46836e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X011255.25-012015.4 | chandra | ccd6 | 357.994 | 391.22 | 32.4636 | 6.78916 | 0.00552122 | 0.00115466 | 8.79353 | 1 | 4.16454 | 4.16454 | 0 | 9.97035 | F | F | 4.81e+20 | 6.41445e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X011236.27-011224.1 | chandra | ccd7 | 269.474 | 534.207 | 15.3129 | 3.91317 | 0.00260432 | 0.000665527 | 15.391 | 1 | 0.548332 | 0.548332 | 0 | 1.94183 | F | F | 4.71e+20 | 1.83896e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X011213.54-011304.3 | chandra | ccd7 | 962.44 | 452.591 | 26.8326 | 5.18002 | 0.00456352 | 0.000880986 | 26.9695 | 1 | 1.00919 | 1.00919 | 0 | 3.78659 | F | F | 4.71e+20 | 3.51646e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X011151.17-012129.6 | chandra | ccd2 | 1150.25 | 926.388 | 19.758 | 6.75566 | 0.00336032 | 0.00114896 | 3.88377 | 0.999775 | 10.2563 | 3.31732 | 52.5903 | 12.8125 | F | F | 4.91e+20 | 4.48609e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X011206.18-012508.9 | chandra | ccd2 | 692.218 | 480.244 | 24.409 | 6.24519 | 0.00415134 | 0.00106214 | 4.798 | 0.999992 | 5.30915 | 4.57682 | 85.2765 | 13.5127 | F | F | 4.87e+20 | 5.78659e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X011238.52-011520.2 | chandra | ccd6 | 867.278 | 990.833 | 8.91137 | 3 | 0.00151559 | 0.000510222 | 2.41385 | 0.987333 | 0.521956 | 0.492 | 91.3213 | 3.47835 | F | F | 4.76e+20 | 1.54313e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X011227.58-011221.9 | chandra | ccd7 | 533.722 | 538.167 | 8.80827 | 3 | 0.00149806 | 0.000510223 | 8.8532 | 1 | 0.492 | 0.492 | 5.00399 | 0.576745 | F | F | 4.7e+20 | 1.04677e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X011201.63-011743.8 | chandra | ccd3 | 155.864 | 582.864 | 8.58558 | 3.31667 | 0.00146098 | 0.000564387 | 14.0417 | 1 | 3.13948 | 2.29317 | 122.922 | 8.33768 | F | F | 4.78e+20 | 1.8883e-14 | 1 | dx | ||||
Report | 2 | X011239.87-011231.0 | chandra | ccd7 | 159.357 | 519.643 | 6.84014 | 2.64576 | 0.00116333 | 0.000449974 | 6.87503 | 0.99999 | 0.591572 | 0.492 | 15.3093 | 2.80694 | F | F | 4.71e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 7 | X011238.47-010956.1 | chandra | ccd7 | 202 | 834.5 | 5.81277 | 2.44949 | 0.000988601 | 0.000416595 | 5.84242 | 0.999922 | 0.492 | 0.492 | 52.0181 | 3.81115 | F | F | 4.67e+20 | 7.85961e-15 | 1 | dx | ||||
Report | 6 | X011224.19-010956.3 | chandra | ccd7 | 637.25 | 834.25 | 3.8732 | 2 | 0.000658731 | 0.000340149 | 3.89296 | 0.996493 | 0.493356 | 0.492 | 126.449 | 3.14115 | F | F | 4.66e+20 | 0 | 1 | d | |||||
Report | 5 | X011222.75-011116.8 | chandra | ccd7 | 681.167 | 670.5 | 2.85949 | 1.73206 | 0.000486326 | 0.000294578 | 2.87408 | 0.981626 | 0.492 | 0.492 | 2.4438e-08 | 2.17921 | F | F | 4.68e+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