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 | 3 | X143254.80+352852.7 | chandra | ccd2 | 1006.04 | 953.563 | 24.1756 | 4.94027 | 0.00547218 | 0.00111824 | 45.9567 | 1 | 0.404618 | 0.404618 | 0 | 0.982395 | F | F | 1.11e+20 | 0 | 1 | ds | |||||
| Report | 1 | X143239.97+352154.4 | chandra | ccd0 | 324.881 | 107.411 | 24.1742 | 5.57989 | 0.00547186 | 0.00126301 | 12.9579 | 1 | 3.2876 | 1.92438 | 353.119 | 8.56571 | F | F | 1.11e+20 | 0 | 1 | ds | |||||
| Report | 2 | X143238.69+353051.1 | chandra | ccd1 | 354.852 | 146.28 | 13.8833 | 3.81352 | 0.00314472 | 0.000863803 | 17.0939 | 1 | 0.76341 | 0.293066 | 358.38 | 3.67028 | F | F | 1.12e+20 | 0 | 1 | ds | |||||
| Report | 2 | X143239.23+352846.7 | chandra | ccd0 | 342.571 | 945.597 | 11.5857 | 3.40378 | 0.00262244 | 0.000770451 | 6.21017 | 0.999999 | 0.946544 | 0.946544 | 0 | 3.56834 | F | F | 1.12e+20 | 0 | 1 | ds | |||||
| Report | 3 | X143213.09+352642.3 | chandra | ccd0 | 991.5 | 693.056 | 7.91827 | 3.00002 | 0.00179231 | 0.000679059 | 4.24436 | 0.999725 | 2.02801 | 1.67014 | 162.57 | 9.27597 | F | F | 1.13e+20 | 0 | 1 | d | |||||
| Report | 4 | X143236.51+352540.0 | chandra | ccd0 | 409.944 | 565.611 | 8.77393 | 3.00001 | 0.00198599 | 0.000679055 | 4.70301 | 0.999928 | 0.714749 | 0.492 | 166.517 | 5.74963 | F | F | 1.12e+20 | 0 | 1 | d | |||||
| Report | 1 | X143306.85+352224.7 | chandra | ccd2 | 706.125 | 164.5 | 7.67299 | 2.82843 | 0.00173679 | 0.00064022 | 14.586 | 1 | 1.30814 | 0.838753 | 101.957 | 7.74 | A | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | 5 | X143308.06+353152.3 | chandra | ccd3 | 663.5 | 275.071 | 6.92971 | 2.64575 | 0.00156855 | 0.000598869 | 12.072 | 1 | 0.492 | 0.492 | 60.8797 | 3.19418 | F | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | 1 | X143256.43+353539.0 | chandra | ccd3 | 952.072 | 735.929 | 6.89791 | 2.64575 | 0.00156135 | 0.00059887 | 12.0166 | 1 | 0.658607 | 0.492 | 167.829 | 5.82211 | F | F | 1.11e+20 | 0 | 1 | d | |||||
| Report | 2 | X143328.47+352904.0 | chandra | ccd2 | 169.786 | 976.643 | 6.54791 | 2.64576 | 0.00148213 | 0.000598871 | 12.4473 | 1 | 1.03589 | 0.670611 | 29.4305 | 6.65419 | A | F | 1.09e+20 | 0 | 1 | d | |||||
| Report | 1 | X143246.64+353205.6 | chandra | ccd1 | 157 | 297.25 | 3.96862 | 2 | 0.000898934 | 0.000453021 | 4.8864 | 0.999397 | 0.492 | 0.492 | 104.872 | 2.95812 | F | F | 1.11e+20 | 0 | 1 | d | |||||
| Report | 4 | X143314.14+353124.5 | chandra | ccd3 | 512.75 | 218.75 | 3.93823 | 2 | 0.000891423 | 0.000452703 | 6.86065 | 0.999975 | 0.720987 | 0.492 | 79.2761 | 4.01614 | F | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | 5 | X143245.83+352203.8 | chandra | ccd0 | 178.5 | 126 | 3.86971 | 2 | 0.000875914 | 0.000452703 | 2.07424 | 0.974007 | 0.492 | 0.492 | 90 | 8.03669 | F | F | 1.11e+20 | 0 | 1 | d | |||||
| Report | 3 | X143319.88+353052.7 | chandra | ccd3 | 370.167 | 154.167 | 2.92642 | 1.73205 | 0.000662399 | 0.000392052 | 5.09801 | 0.999622 | 0.615 | 0.492 | 45 | 4.97354 | F | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | 2 | X143253.43+353715.3 | chandra | ccd3 | 1026.5 | 931.5 | 2.87087 | 1.73206 | 0.000649824 | 0.000392054 | 5.00124 | 0.999622 | 0.492 | 0.492 | 180 | 7.44334 | F | F | 1.11e+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