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 | 3 | X142717.62+375016.8 | chandra | ccd2 | 819.6 | 494.456 | 17.4988 | 4.18316 | 0.00350696 | 0.000838353 | 33.4173 | 1 | 1.41157 | 0.589117 | 22.1415 | 4.37805 | 14.9293 | 3.78797 | -0.595244 | 0.340231 | F | F | 1.1e+20 | 4.53063e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X142643.22+374643.0 | chandra | ccd3 | 804.967 | 712.1 | 14.8298 | 4.96863 | 0.00297203 | 0.00099576 | 35.9447 | 1 | 1.19345 | 0.799538 | 133.719 | 6.3139 | 7.94326 | 7.88652 | -0.0035843 | 0.323639 | F | F | 1.07e+20 | 4.06544e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X142733.23+375054.7 | chandra | ccd2 | 443.67 | 571.712 | 12.5271 | 3.53936 | 0.00251057 | 0.000709328 | 23.9229 | 1 | 0.94503 | 0.94503 | 0 | 6.15011 | 7.91529 | 4.83058 | -0.242016 | 0.382755 | F | F | 1.1e+20 | 3.3943e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X142652.83+380251.5 | chandra | ccd6 | 816.447 | 864.29 | 17.083 | 5.55522 | 0.0034237 | 0.00111335 | 10.0022 | 1 | 3.8333 | 2.58946 | 88.0563 | 17.4771 | 13.7417 | 3.45569 | -0.598114 | 0.378252 | F | F | 1.12e+20 | 5.69208e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X142757.67+374741.9 | chandra | ccd0 | 444.652 | 1114.61 | 11.6118 | 3.40761 | 0.00232718 | 0.000682936 | 23.8974 | 1 | 2.69339 | 2.69339 | 0 | 8.62595 | 3.74599 | 6.15329 | 0.24318 | 0.464095 | F | F | 1.1e+20 | 3.42705e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X142656.12+373821.2 | chandra | ccd1 | 1073.9 | 531.8 | 10.6148 | 4.42783 | 0.00212733 | 0.000887393 | 17.1018 | 1 | 2.63793 | 1.09112 | 108.117 | 8.4431 | 3.92996 | 6.71982 | 0.261965 | 0.433318 | A | F | 1.05e+20 | 3.34439e-14 | 1 | dx |
| Report | 5 | X142714.49+374542.0 | chandra | ccd3 | 51.5 | 587.5 | 7.95916 | 2.82843 | 0.00159509 | 0.000566844 | 15.1998 | 1 | 0.492 | 0.492 | 58.2825 | 0.249056 | F | F | 1.07e+20 | 0 | 1 | d | |||||
| Report | 3 | X142700.19+374623.6 | chandra | ccd3 | 396 | 672.125 | 7.95157 | 2.82843 | 0.00159357 | 0.000566844 | 15.1853 | 1 | 0.492 | 0.492 | 173.187 | 2.94716 | F | F | 1.07e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X142717.89+375051.2 | chandra | ccd2 | 812.5 | 563.875 | 7.94489 | 3.95804 | 0.00159224 | 0.000793236 | 33.8419 | 1 | 0.756461 | 0.492 | 125.152 | 4.95379 | 7 | 0.944885 | -0.76214 | 0.633022 | A | F | 1.1e+20 | 2.40519e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X142751.44+374503.3 | chandra | ccd0 | 593.625 | 791.625 | 8.82178 | 4.1225 | 0.00176801 | 0.000826208 | 20.8965 | 1 | 1.57349 | 0.828013 | 85.6942 | 7.27158 | 4.95544 | 3.86633 | -0.123457 | 0.475401 | A | F | 1.09e+20 | 2.49819e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X142737.20+374448.2 | chandra | ccd0 | 937 | 760.375 | 7.86841 | 3.95804 | 0.00157694 | 0.000793248 | 21.6909 | 1 | 0.632848 | 0.492 | 75.302 | 4.54571 | 6 | 1.86841 | -0.525086 | 0.574182 | F | F | 1.07e+20 | 1.98859e-14 | 1 | dx |
| Report | 4 | X142656.62+374728.5 | chandra | ccd3 | 482.071 | 804.214 | 6.93463 | 2.64575 | 0.00138977 | 0.000530234 | 13.2432 | 1 | 0.492 | 0.492 | 43.6987 | 3.93231 | F | F | 1.07e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X142709.75+374211.3 | chandra | ccd1 | 744.9 | 999.3 | 4.91531 | 3.39792 | 0.000985091 | 0.000680986 | 16.8899 | 1 | 0.492 | 0.492 | 31.7175 | 3.88246 | 4 | 0.915307 | -0.627569 | 0.828535 | F | F | 1.06e+20 | 1.1985e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X142722.52+374259.5 | chandra | ccd1 | 436.7 | 1097.3 | 4.66123 | 3.39792 | 0.00093417 | 0.000680986 | 8.0084 | 0.999998 | 0.492 | 0.492 | 23.8632 | 3.30313 | 3.91531 | 0.74592 | -0.679947 | 0.894905 | F | F | 1.06e+20 | 1.14652e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X142724.78+374634.5 | chandra | ccd2 | 646.5 | 42.2998 | 6.93425 | 3.78388 | 0.0013897 | 0.000758332 | 27.0434 | 1 | 0.633842 | 0.492 | 14.0893 | 2.05061 | 5 | 1.93425 | -0.442116 | 0.603656 | F | F | 1.09e+20 | 3.20284e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X142706.13+374618.4 | chandra | ccd3 | 252.833 | 661.5 | 2.91531 | 2.93649 | 0.000584255 | 0.000588501 | 10.0175 | 0.999998 | 0.492 | 0.492 | 180 | 1.77665 | 2 | 0.915307 | -0.372068 | 1.09797 | F | F | 1.07e+20 | 7.00281e-15 | 1 | dx |
| Report | 4 | X142726.89+374806.9 | chandra | ccd2 | 595.833 | 230.167 | 2.95817 | 1.73205 | 0.000592851 | 0.000347123 | 5.64919 | 0.999811 | 0.543766 | 0.492 | 124.722 | 3.21671 | F | F | 1.09e+20 | 0 | 1 | d | |||||
| Report | 2 | X142702.84+374048.9 | chandra | ccd1 | 911.5 | 831.833 | 2.94324 | 1.73205 | 0.000589863 | 0.000347126 | 5.75037 | 0.999841 | 0.492 | 0.492 | 151.845 | 5.64882 | F | F | 1.06e+20 | 0 | 1 | d | |||||
| Report | 4 | X142735.54+374134.4 | chandra | ccd0 | 976.5 | 366.5 | 0.996435 | 1 | 0.0001997 | 0.000200414 | 2.05069 | 0.97615 | 0.492 | 0.492 | 90 | 5.96968 | F | F | 1.06e+20 | 0 | 1 | d | |||||
| Report | 5 | X142722.95+374455.6 | chandra | ccd0 | 1280.5 | 775.167 | 2.98721 | 1.73205 | 0.000598681 | 0.000347128 | 6.14776 | 0.999893 | 0.492 | 0.492 | 90 | 1.8794 | F | F | 1.07e+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