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 | 7 | X142855.52+352817.6 | chandra | ccd2 | 904.039 | 507.851 | 36.0236 | 8.03943 | 0.00797185 | 0.00177909 | 6.73498 | 1 | 1.05317 | 1.05317 | 0 | 7.64659 | F | F | 1.2e+20 | 0 | 1 | ds | |||||
Report | 2 | X142856.18+353042.2 | chandra | ccd2 | 886.792 | 801.333 | 23.1479 | 4.89899 | 0.0051225 | 0.00108412 | 4.32775 | 0.999946 | 1.14563 | 0.821499 | 90.4249 | 7.38419 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 4 | X142959.58+353026.9 | chandra | ccd1 | 755.908 | 619.423 | 19.6122 | 4.42857 | 0.00434312 | 0.000980705 | 32.5137 | 1 | 1.1628 | 0.617768 | 19.6499 | 5.59441 | F | F | 1.18e+20 | 0 | 1 | ds | |||||
Report | 3 | X142901.75+353322.2 | chandra | ccd2 | 748.125 | 1126.19 | 15.0436 | 4.00001 | 0.00332905 | 0.000885179 | 2.81255 | 0.995506 | 1.55948 | 1.12003 | 164.383 | 7.1173 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 2 | X142957.07+353054.4 | chandra | ccd1 | 818.192 | 675.189 | 18.6277 | 4.31598 | 0.00412511 | 0.000955775 | 30.8816 | 1 | 1.21511 | 1.21511 | 0 | 5.1552 | F | F | 1.18e+20 | 0 | 1 | ds | |||||
Report | 6 | X142927.69+352643.3 | chandra | ccd3 | 905.386 | 973.535 | 12.4456 | 3.52783 | 0.00275416 | 0.000780694 | 20.0072 | 1 | 0.706872 | 0.706872 | 0 | 3.2896 | F | F | 1.19e+20 | 0 | 1 | ds | |||||
Report | 5 | X142847.85+352813.4 | chandra | ccd2 | 1094.07 | 499.072 | 11.7087 | 3.7417 | 0.00259105 | 0.000828015 | 2.18905 | 0.983012 | 2.495 | 1.62289 | 155.681 | 9.18595 | A | F | 1.2e+20 | 0 | 1 | d | |||||
Report | 3 | X142950.89+352410.9 | chandra | ccd3 | 328.25 | 663.5 | 11.2513 | 3.46412 | 0.00248984 | 0.000766588 | 18.0873 | 1 | 1.50662 | 0.78423 | 22.7431 | 6.84783 | A | F | 1.18e+20 | 0 | 1 | d | |||||
Report | 5 | X142940.09+352000.1 | chandra | ccd3 | 596.682 | 153.591 | 8.95706 | 3.31667 | 0.00198214 | 0.000733958 | 14.3991 | 1 | 2.14839 | 1.93879 | 172.306 | 10.0052 | F | F | 1.18e+20 | 0 | 1 | d | |||||
Report | 1 | X142935.05+352901.2 | chandra | ccd3 | 722.167 | 1253.28 | 8.91334 | 3 | 0.00197247 | 0.000663882 | 14.3289 | 1 | 0.492 | 0.492 | 7.62756 | 1.03214 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 2 | X142928.87+352336.9 | chandra | ccd3 | 875.5 | 594.125 | 7.51571 | 2.82844 | 0.00166318 | 0.000625916 | 12.0821 | 1 | 1.01002 | 0.782086 | 114.295 | 6.30109 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 3 | X142959.34+353421.9 | chandra | ccd1 | 761.786 | 1096.5 | 6.79514 | 2.64576 | 0.00150476 | 0.000585892 | 11.2652 | 1 | 1.02273 | 0.492 | 70.16 | 7.10911 | A | F | 1.18e+20 | 0 | 1 | d | |||||
Report | 1 | X142957.85+353022.4 | chandra | ccd1 | 798.25 | 609.75 | 3.93396 | 2 | 0.000871159 | 0.000442892 | 6.52184 | 0.999961 | 0.600805 | 0.492 | 140.944 | 5.2369 | F | F | 1.18e+20 | 0 | 1 | d | |||||
Report | 1 | X142914.27+353435.8 | chandra | ccd0 | 1064.5 | 464.5 | 3.88909 | 2 | 0.000860633 | 0.000442589 | 6.33953 | 0.999954 | 0.492 | 0.492 | 90 | 5.96783 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 2 | X142929.65+353525.9 | chandra | ccd0 | 683 | 566.25 | 3.93577 | 2 | 0.000870961 | 0.000442588 | 6.41561 | 0.999954 | 0.507001 | 0.492 | 143.909 | 5.57819 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 3 | X142925.65+353333.2 | chandra | ccd0 | 782.3 | 337.1 | 4.88608 | 2.23607 | 0.00108126 | 0.000494829 | 7.96469 | 0.999997 | 0.759973 | 0.492 | 62.1902 | 3.91081 | A | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 4 | X142924.93+353351.7 | chandra | ccd0 | 800.1 | 374.7 | 4.88343 | 2.23607 | 0.00108067 | 0.000494829 | 7.96037 | 0.999997 | 0.511506 | 0.492 | 137.199 | 4.25059 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 5 | X142909.97+353616.2 | chandra | ccd0 | 1171.39 | 669.143 | 28.7788 | 5.36459 | 0.00636861 | 0.00118716 | 46.9117 | 1 | 2.83807 | 2.83807 | 0 | 7.84407 | F | F | 1.19e+20 | 0 | 1 | ds | |||||
Report | 6 | X142925.25+353639.6 | chandra | ccd0 | 792.125 | 716 | 7.3949 | 2.82844 | 0.00163645 | 0.000625917 | 12.0543 | 1 | 1.42618 | 0.559151 | 100.73 | 6.9284 | A | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 7 | X142955.57+353707.2 | chandra | ccd0 | 41.0905 | 772.88 | 13.7658 | 3.71023 | 0.0030463 | 0.000821056 | 22.4393 | 1 | 2.06626 | 2.06626 | 0 | 8.66629 | F | F | 1.18e+20 | 0 | 1 | ds | |||||
Report | 8 | X142947.61+353427.2 | chandra | ccd0 | 238.231 | 447.561 | 41.9002 | 6.47304 | 0.00927231 | 0.00143245 | 68.3006 | 1 | 1.82964 | 0.863219 | 53.3275 | 5.54574 | F | F | 1.19e+20 | 0 | 1 | ds | |||||
Report | 5 | X142937.22+353011.7 | chandra | ccd1 | 1310.17 | 587.5 | 2.97382 | 1.73205 | 0.000658541 | 0.000383556 | 4.9301 | 0.999453 | 0.492 | 0.492 | 180 | 1.06338 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 4 | X142931.66+352703.2 | chandra | ccd3 | 806.167 | 1013.5 | 2.9417 | 1.73205 | 0.00065098 | 0.000383293 | 4.729 | 0.999313 | 0.492 | 0.492 | 90 | 2.82729 | F | F | 1.19e+20 | 0 | 1 | d | |||||
Report | 7 | X142948.46+352621.8 | chandra | ccd3 | 388.833 | 929.5 | 2.93989 | 1.73205 | 0.00065058 | 0.000383293 | 4.7261 | 0.999313 | 0.492 | 0.492 | 3.85109e-08 | 4.82447 | F | F | 1.18e+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