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 | 2 | X131717.24+005956.9 | chandra | ccd7 | 642.536 | 401.958 | 18.6673 | 4.32057 | 0.00284057 | 0.000657452 | 18.9723 | 1 | 0.484879 | 0.484879 | 0 | 1.06878 | F | F | 2.09e+20 | 0 | 1 | ds | |||||
| Report | 1 | X131732.15+010219.9 | chandra | ccd7 | 187.5 | 692.131 | 18.2292 | 4.35891 | 0.00277388 | 0.000663283 | 18.527 | 1 | 1.04008 | 0.835772 | 148.081 | 5.43069 | F | F | 2.09e+20 | 0 | 1 | d | |||||
| Report | 1 | X131655.80+010903.8 | chandra | ccd3 | 70.6499 | 861.1 | 17.3995 | 4.47218 | 0.00264764 | 0.000680519 | 28.296 | 1 | 2.47795 | 1.79153 | 16.6549 | 10.2649 | F | F | 2.08e+20 | 0 | 1 | d | |||||
| Report | 3 | X131718.59+005609.6 | chandra | ccd6 | 228.465 | 922.114 | 17.5018 | 4.18352 | 0.00266322 | 0.000636598 | 26.867 | 1 | 0.794973 | 0.794973 | 0 | 3.84532 | F | F | 2.1e+20 | 0 | 1 | ds | |||||
| Report | 1 | X131638.03+010212.9 | chandra | ccd2 | 235.357 | 996.071 | 13.2295 | 4.00004 | 0.00201309 | 0.000608675 | 21.4578 | 1 | 0.790429 | 0.660849 | 35.5148 | 9.09385 | F | F | 2.1e+20 | 0 | 1 | d | |||||
| Report | 2 | X131708.44+005532.5 | chandra | ccd6 | 537.3 | 846.1 | 6.86286 | 2.64575 | 0.0010443 | 0.000402597 | 10.5352 | 1 | 0.492 | 0.492 | 121.717 | 4.36029 | F | F | 2.11e+20 | 0 | 1 | d | |||||
| Report | 10 | X131719.01+005800.9 | chandra | ccd7 | 588.167 | 165.833 | 5.83354 | 2.44949 | 0.000887674 | 0.000372733 | 5.92884 | 0.999932 | 0.492 | 0.492 | 123.401 | 2.28506 | F | F | 2.1e+20 | 0 | 1 | d | |||||
| Report | 6 | X131732.33+010234.6 | chandra | ccd7 | 182 | 722 | 5.74674 | 2.4495 | 0.000874465 | 0.000372733 | 5.84062 | 0.999932 | 0.518663 | 0.492 | 13.2825 | 5.59027 | F | F | 2.09e+20 | 0 | 1 | d | |||||
| Report | 3 | X131719.72+005903.0 | chandra | ccd7 | 566.3 | 291.9 | 4.81781 | 2.23607 | 0.000733113 | 0.000340257 | 4.89652 | 0.999498 | 0.492 | 0.492 | 97.6276 | 1.81025 | F | F | 2.1e+20 | 0 | 1 | d | |||||
| Report | 7 | X131731.84+010243.1 | chandra | ccd7 | 197.1 | 739.3 | 4.727 | 2.23608 | 0.000719294 | 0.000340257 | 4.80422 | 0.999498 | 0.501213 | 0.492 | 176.437 | 5.55834 | F | F | 2.09e+20 | 0 | 1 | d | |||||
| Report | 8 | X131713.62+010413.0 | chandra | ccd7 | 752.3 | 922.1 | 4.71952 | 2.23608 | 0.000718156 | 0.000340257 | 4.79662 | 0.999498 | 0.695327 | 0.492 | 146.125 | 4.47218 | F | F | 2.09e+20 | 0 | 1 | d | |||||
| Report | 1 | X131657.91+005553.6 | chandra | ccd6 | 858.25 | 889 | 3.93253 | 2 | 0.000598402 | 0.000304335 | 6.03682 | 0.999919 | 0.504692 | 0.492 | 37.9819 | 5.39988 | F | F | 2.11e+20 | 0 | 1 | d | |||||
| Report | 5 | X131722.24+010039.7 | chandra | ccd7 | 489.5 | 488.5 | 3.86926 | 2 | 0.000588775 | 0.000304335 | 3.93247 | 0.996806 | 0.492 | 0.492 | 45 | 2.47516 | F | F | 2.09e+20 | 0 | 1 | d | |||||
| Report | 4 | X131706.89+010012.3 | chandra | ccd7 | 957.5 | 432.833 | 2.90646 | 1.73205 | 0.000442268 | 0.000263562 | 2.95394 | 0.982905 | 0.492 | 0.492 | 90 | 1.60422 | F | F | 2.1e+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