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 | 8 | X142824.06+325052.2 | chandra | ccd2 | 396.379 | 679.172 | 78.9281 | 9.06853 | 0.0174665 | 0.00200683 | 61.352 | 1 | 0.760589 | 0.496736 | 130.763 | 3.59312 | F | F | 9.12e+19 | 0 | 1 | ds | |||||
| Report | 8 | X142911.23+324823.4 | chandra | ccd1 | 661.722 | 197.061 | 40.4176 | 6.35748 | 0.00894424 | 0.00140688 | 81.6625 | 1 | 1.21338 | 0.682656 | 356.854 | 6.83983 | A | F | 8.91e+19 | 0 | 1 | ds | |||||
| Report | 5 | X142850.47+324520.8 | chandra | ccd3 | 549.641 | 660.381 | 27.739 | 5.26678 | 0.00613853 | 0.00116552 | 20.4629 | 1 | 1.25815 | 1.25815 | 0 | 5.98027 | F | F | 8.99e+19 | 0 | 1 | ds | |||||
| Report | 4 | X142858.70+325158.3 | chandra | ccd1 | 983.308 | 633.549 | 21.8709 | 4.67663 | 0.00483994 | 0.00103492 | 44.1895 | 1 | 0.528347 | 0.528347 | 0 | 3.8106 | F | F | 8.95e+19 | 0 | 1 | ds | |||||
| Report | 1 | X142852.71+325026.9 | chandra | ccd1 | 1136.54 | 447.618 | 16.9497 | 4.117 | 0.0037509 | 0.000911076 | 34.2463 | 1 | 0.579885 | 0.579885 | 0 | 2.48439 | F | F | 8.98e+19 | 0 | 1 | ds | |||||
| Report | 3 | X142900.43+324513.0 | chandra | ccd3 | 293.767 | 644.167 | 14.4441 | 3.87299 | 0.00319639 | 0.00085707 | 10.6553 | 1 | 1.35739 | 0.837611 | 1.06392 | 7.05894 | A | F | 8.95e+19 | 0 | 1 | dp | |||||
| Report | 2 | X142836.28+324224.0 | chandra | ccd3 | 913.574 | 300.983 | 11.3261 | 3.87315 | 0.00250642 | 0.00085711 | 8.35521 | 1 | 2.81399 | 0.834646 | 357.323 | 8.63741 | F | F | 9.03e+19 | 0 | 1 | ds | |||||
| Report | 3 | X142857.94+325115.2 | chandra | ccd1 | 1002.62 | 545.842 | 14.0544 | 3.74892 | 0.00311018 | 0.00082962 | 28.3965 | 1 | 0.705037 | 0.421854 | 34.5021 | 3.53441 | F | F | 8.95e+19 | 0 | 1 | ds | |||||
| Report | 1 | X142849.70+325704.5 | chandra | ccd0 | 407.78 | 636.719 | 13.0155 | 3.6077 | 0.00288027 | 0.000798368 | 27.7726 | 1 | 1.90357 | 1.90357 | 0 | 6.33437 | F | F | 9.01e+19 | 0 | 1 | ds | |||||
| Report | 3 | X142808.35+325232.8 | chandra | ccd2 | 798.36 | 884.105 | 21.8313 | 4.6724 | 0.00483118 | 0.00103398 | 16.9698 | 1 | 1.1792 | 1.1792 | 0 | 7.06106 | F | F | 9.2e+19 | 0 | 1 | ds | |||||
| Report | 4 | X142851.82+324154.8 | chandra | ccd3 | 514.3 | 241.3 | 9.07226 | 3.1623 | 0.00200764 | 0.000699797 | 6.69256 | 0.999996 | 2.87894 | 1.45034 | 132.727 | 9.35631 | A | F | 8.98e+19 | 0 | 1 | d | |||||
| Report | 6 | X142816.43+325518.4 | chandra | ccd2 | 590.722 | 1219.94 | 8.87449 | 3 | 0.00196387 | 0.000663882 | 6.89828 | 0.999999 | 1.44582 | 0.516117 | 77.1662 | 6.74674 | A | F | 9.18e+19 | 0 | 1 | d | |||||
| Report | 2 | X142851.73+325040.9 | chandra | ccd1 | 1161.1 | 475.5 | 4.94182 | 2.23607 | 0.0010936 | 0.000494829 | 9.9848 | 1 | 0.492 | 0.492 | 90 | 2.2437 | F | F | 8.98e+19 | 0 | 1 | d | |||||
| Report | 1 | X142804.36+324805.7 | chandra | ccd2 | 900.9 | 340.7 | 4.85081 | 2.23607 | 0.00107346 | 0.000494829 | 3.77061 | 0.998385 | 0.688422 | 0.492 | 7.23515 | 8.25672 | F | F | 9.19e+19 | 0 | 1 | d | |||||
| Report | 5 | X142910.10+325510.8 | chandra | ccd1 | 691.1 | 1024.5 | 4.81681 | 2.23607 | 0.00106593 | 0.000494829 | 9.73222 | 1 | 0.492 | 0.492 | 143.35 | 7.37792 | F | F | 8.9e+19 | 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