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 | srcpi bgdpi arf | 2 | X142539.58+341858.6 | chandra | ccd2 | 616.907 | 974.657 | 29.0303 | 5.38834 | 0.00615743 | 0.00114289 | 69.3895 | 1 | 1.74057 | 0.848704 | 106.453 | 5.95365 | F | F | 1.14e+20 | 8.33219e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X142623.64+341550.0 | chandra | ccd1 | 975.127 | 462.081 | 13.2845 | 4.38517 | 0.00281768 | 0.000930109 | 5.4483 | 0.999995 | 0.51956 | 0.51956 | 0 | 3.73544 | F | F | 1.11e+20 | 3.16314e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X142549.25+341136.3 | chandra | ccd3 | 1174.03 | 741.461 | 13.0819 | 3.61689 | 0.00277473 | 0.000767159 | 30.6604 | 1 | 2.00763 | 1.00941 | 349.561 | 6.0271 | F | F | 1.1e+20 | 3.5034e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X142619.22+341408.7 | chandra | ccd3 | 418.422 | 1051.16 | 13.4808 | 3.67162 | 0.00285932 | 0.000778764 | 31.5954 | 1 | 0.788761 | 0.788761 | 0 | 3.65755 | F | F | 1.1e+20 | 3.23217e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X142621.95+340901.2 | chandra | ccd3 | 348.875 | 425.75 | 7.63834 | 2.82843 | 0.00162012 | 0.00059992 | 17.9022 | 1 | 1.18613 | 0.699076 | 57.9857 | 8.22991 | A | F | 1.09e+20 | 2.22718e-14 | 1 | dx | ||||
| Report | 2 | X142608.51+341258.7 | chandra | ccd3 | 687.928 | 908.357 | 6.93143 | 2.64575 | 0.00147018 | 0.000561173 | 16.2454 | 1 | 0.766172 | 0.492 | 7.71108 | 3.61312 | A | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X142541.41+342149.6 | chandra | ccd0 | 1275.17 | 488.667 | 5.60715 | 2.4495 | 0.00118929 | 0.000519547 | 12.5745 | 1 | 1.20061 | 0.806296 | 20.2709 | 7.3066 | F | F | 1.16e+20 | 1.59446e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X142610.85+341734.1 | chandra | ccd1 | 1297.1 | 673.1 | 4.96214 | 2.23607 | 0.00105249 | 0.000474278 | 2.0351 | 0.9596 | 0.492 | 0.492 | 45 | 1.44378 | F | F | 1.13e+20 | 1.16705e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142558.32+342331.4 | chandra | ccd0 | 849.5 | 695.3 | 4.81361 | 2.23607 | 0.00102098 | 0.000474278 | 10.7949 | 1 | 1.13932 | 0.492 | 125.294 | 7.1453 | A | F | 1.16e+20 | 1.31816e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X142540.34+341410.9 | chandra | ccd2 | 598 | 389.5 | 3.94593 | 2 | 0.000836945 | 0.000424207 | 9.43174 | 0.999999 | 0.589736 | 0.492 | 118.997 | 5.78648 | F | F | 1.12e+20 | 1.1596e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142556.83+342418.4 | chandra | ccd0 | 886.833 | 790.833 | 2.84116 | 1.73206 | 0.00060262 | 0.000367375 | 6.37152 | 0.999944 | 0.492 | 0.492 | 90 | 7.97767 | F | F | 1.16e+20 | 8.20894e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X142609.15+342343.4 | chandra | ccd0 | 577.379 | 720.206 | 10.5218 | 3.24373 | 0.00223171 | 0.000688007 | 23.596 | 1 | 1.16887 | 1.16887 | 0 | 7.20376 | F | F | 1.16e+20 | 2.7835e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X142630.68+341056.3 | chandra | ccd3 | 128.833 | 659.833 | 2.80749 | 1.73206 | 0.000595477 | 0.000367375 | 6.57999 | 0.999122 | 0.563657 | 0.492 | 26.5651 | 7.59958 | F | F | 1.09e+20 | 7.5462e-15 | 1 | dx |
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