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 | X125937.65+600834.7 | chandra | ccd3 | 626.422 | 988.293 | 48.6411 | 7.65944 | 0.00357832 | 0.000563472 | 21.2548 | 1 | 0.884319 | 0.884319 | 0 | 6.04509 | F | U | 1.31e+20 | 0 | 1 | ds | |||||
| Report | 1 | X125929.23+600845.7 | chandra | ccd3 | 754.479 | 1010.58 | 54.9943 | 7.41625 | 0.00404569 | 0.000545581 | 24.031 | 1 | 2.0586 | 1.01652 | 349.909 | 6.61832 | F | U | 1.3e+20 | 0 | 1 | ds | |||||
| Report | 8 | X130033.02+595944.9 | chandra | ccd2 | 573.579 | 596.436 | 23.7192 | 6.33932 | 0.00174492 | 0.000466357 | 7.46446 | 1 | 1.18547 | 0.292453 | 70.7363 | 5.89365 | A | U | 1.28e+20 | 0 | 1 | ds | |||||
| Report | 5 | X125922.59+600103.3 | chandra | ccd1 | 169.638 | 850.689 | 23.1531 | 4.81205 | 0.00170327 | 0.000354001 | 10.4096 | 1 | 1.218 | 0.499784 | 306.668 | 4.1717 | F | U | 1.25e+20 | 0 | 1 | ds | |||||
| Report | 1 | X125902.56+595831.5 | chandra | ccd1 | 474.554 | 542.244 | 15.7826 | 5.06696 | 0.00116106 | 0.000372754 | 7.09584 | 1 | 0.963504 | 0.963504 | 0 | 7.61878 | F | U | 1.23e+20 | 0 | 1 | ds | |||||
| Report | 5 | X130052.28+600122.4 | chandra | ccd2 | 280.319 | 794.535 | 21.1651 | 4.98917 | 0.00155703 | 0.000367032 | 6.66068 | 1 | 2.11767 | 1.00253 | 233.737 | 7.5576 | F | U | 1.31e+20 | 0 | 1 | ds | |||||
| Report | 5 | X125938.00+600523.7 | chandra | ccd3 | 621 | 600.001 | 8.94264 | 3.82383 | 0.000657871 | 0.000281302 | 3.90769 | 0.999635 | 0.299945 | 0.299945 | 0 | 3.15801 | F | U | 1.29e+20 | 0 | 1 | ds | |||||
| Report | 1 | X125950.65+600041.8 | chandra | ccd2 | 1218 | 711.5 | 7.9285 | 2.82843 | 0.000583263 | 0.000208075 | 2.49511 | 0.992097 | 0.492 | 0.492 | 76.7175 | 2.16131 | F | U | 1.26e+20 | 0 | 1 | d | |||||
| Report | 2 | X130010.75+600506.4 | chandra | ccd2 | 912.357 | 1249.5 | 6.92219 | 2.64575 | 0.000509234 | 0.000194636 | 2.17842 | 0.984438 | 0.492 | 0.492 | 38.9526 | 3.18416 | F | U | 1.31e+20 | 0 | 1 | d | |||||
| Report | 1 | X125942.67+595818.7 | chandra | ccd0 | 670.786 | 1202.79 | 6.87926 | 2.64575 | 0.000506191 | 0.00019468 | 8.64836 | 1 | 0.616748 | 0.492 | 84.9377 | 4.70268 | F | U | 1.24e+20 | 0 | 1 | d | |||||
| Report | 2 | X130006.53+595509.1 | chandra | ccd0 | 307.725 | 817.859 | 93.9729 | 9.69396 | 0.00691476 | 0.000713306 | 118.139 | 1 | 3.36945 | 2.31886 | 101.301 | 7.87171 | F | U | 1.23e+20 | 0 | 1 | ds | |||||
| Report | 2 | X125858.30+600011.3 | chandra | ccd1 | 539.929 | 745.928 | 6.69128 | 2.64576 | 0.000492247 | 0.000194636 | 3.00839 | 0.994969 | 0.588389 | 0.492 | 6.69625 | 7.30754 | F | U | 1.23e+20 | 0 | 1 | d | |||||
| Report | 3 | X125910.43+600502.5 | chandra | ccd3 | 1039.5 | 557.167 | 5.79483 | 2.44949 | 0.000426299 | 0.000180198 | 2.53218 | 0.992296 | 0.600188 | 0.492 | 154.903 | 5.72728 | F | U | 1.26e+20 | 0 | 1 | d | |||||
| Report | 1 | X130127.83+600524.3 | chandra | ccd6 | 754.5 | 387 | 3.5979 | 2.00001 | 0.000264681 | 0.000147132 | 4.34601 | 0.999285 | 0.631129 | 0.492 | 70.6701 | 12.1268 | F | U | 1.36e+20 | 0 | 1 | d | |||||
| Report | 2 | X130149.99+600833.5 | chandra | ccd6 | 420.5 | 773.833 | 2.94649 | 1.73205 | 0.00021676 | 0.000127419 | 3.55915 | 0.994652 | 0.492 | 0.492 | 90 | 15.6842 | F | U | 1.39e+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