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 | 8 | X134715.40+172726.0 | chandra | ccd3 | 966.568 | 74.3571 | 642.425 | 25.7696 | 0.128449 | 0.00515248 | 142.975 | 1 | 0.855705 | 0.382456 | 31.959 | 0.486953 | 582.546 | 29.9621 | -0.902166 | 0.0566842 | A | F | 1.78e+20 | 1.32095e-12 | 1 | dsxf |
| Report | srcpi bgdpi arf | 4 | X134736.40+173405.4 | chandra | ccd3 | 356.19 | 886.373 | 93.8003 | 10.608 | 0.0187548 | 0.002121 | 20.8758 | 1 | 3.12046 | 1.90939 | 120.07 | 8.62869 | 85.8446 | 19.8602 | -0.624233 | 0.127049 | F | F | 1.78e+20 | 2.77353e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X134706.04+172600.5 | chandra | ccd0 | 227.855 | 961.614 | 31.4328 | 5.6065 | 0.00628479 | 0.00112098 | 53.9726 | 1 | 0.553873 | 0.553873 | 0 | 2.55896 | 18.8306 | 13 | -0.183176 | 0.215415 | F | F | 1.78e+20 | 7.4577e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X134727.66+172545.0 | chandra | ccd2 | 644.127 | 903.193 | 17.7243 | 4.21002 | 0.00354387 | 0.000841769 | 30.6216 | 1 | 0.628622 | 0.628622 | 0 | 3.03677 | 12 | 5.74598 | -0.352419 | 0.320182 | F | F | 1.78e+20 | 4.37482e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X134722.61+172024.0 | chandra | ccd2 | 790.5 | 250.214 | 13.7817 | 4.84057 | 0.00275553 | 0.000967833 | 29.4938 | 1 | 1.57679 | 0.677689 | 125.062 | 6.7535 | 9.89083 | 3.89083 | -0.435361 | 0.385641 | A | F | 1.77e+20 | 3.76964e-14 | 1 | dx |
| Report | 5 | X134729.10+173017.4 | chandra | ccd3 | 567.875 | 422.25 | 7.90849 | 2.82843 | 0.00158124 | 0.000565521 | 1.76008 | 0.962097 | 0.645372 | 0.492 | 47.3818 | 4.56176 | F | F | 1.78e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X134644.29+172745.2 | chandra | ccd1 | 833 | 135.167 | 5.61886 | 3.59808 | 0.00112345 | 0.000719406 | 9.10142 | 1 | 1.48506 | 0.514216 | 151.334 | 7.60141 | 4.91205 | 0.794773 | -0.721465 | 0.787749 | A | F | 1.78e+20 | 1.53183e-14 | 1 | dx |
| Report | 2 | X134705.18+172712.0 | chandra | ccd1 | 225.5 | 67.5 | 3.93278 | 2 | 0.000786326 | 0.000399884 | 6.90392 | 0.999977 | 0.58344 | 0.492 | 2.35031e-08 | 2.58947 | F | F | 1.78e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X134745.20+171934.2 | chandra | ccd2 | 132.75 | 149.25 | 3.76933 | 3.17945 | 0.000753647 | 0.000635705 | 7.84818 | 0.999996 | 1.57114 | 0.611465 | 104.324 | 10.163 | 0.901142 | 2.86819 | 0.521856 | 0.968398 | A | F | 1.77e+20 | 1.25188e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X134706.68+172154.7 | chandra | ccd0 | 208.833 | 461.5 | 2.93351 | 2.93649 | 0.00058653 | 0.000587127 | 11.3761 | 0.999999 | 0.627179 | 0.492 | 123.69 | 5.52161 | 1 | 1.93351 | 0.318222 | 1.0732 | F | F | 1.78e+20 | 7.62498e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X134712.37+172235.5 | chandra | ccd0 | 43.8844 | 544.865 | 21.8387 | 4.67319 | 0.00436651 | 0.000934375 | 37.4988 | 1 | 1.10578 | 1.10578 | 0 | 4.45883 | 13.9153 | 6.66126 | -0.352539 | 0.29323 | F | F | 1.78e+20 | 6.12095e-14 | 1 | dsx |
| Report | 4 | X134709.20+172438.0 | chandra | ccd0 | 136.052 | 793.908 | 28.8427 | 5.37054 | 0.00576692 | 0.00107381 | 49.5252 | 1 | 0.493562 | 0.493562 | 0 | 2.84058 | F | F | 1.78e+20 | 0 | 1 | ds | |||||
| Report | 3 | X134707.76+173325.1 | chandra | ccd1 | 150.167 | 825.833 | 2.89718 | 1.73205 | 0.000579268 | 0.00034631 | 5.08595 | 0.999643 | 0.492 | 0.492 | 90 | 6.74351 | F | F | 1.78e+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