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 | 1 | X111642.87+571440.5 | chandra | ccd6 | 629.302 | 180.951 | 56.7841 | 8.87147 | 0.0111338 | 0.00173945 | 12.1288 | 1 | 9.44678 | 5.87178 | 0.29356 | 12.4361 | F | F | 7.14e+19 | 0 | 1 | ds | |||||
| Report | 1 | X111714.06+570819.1 | chandra | ccd2 | 245.118 | 770.235 | 31.8726 | 5.83097 | 0.00625311 | 0.00114398 | 52.761 | 1 | 2.5976 | 1.351 | 4.28396 | 8.77983 | A | F | 7.12e+19 | 0 | 1 | d | |||||
| Report | 1 | X111547.49+570310.1 | chandra | ccd3 | 654.181 | 366.255 | 24.4626 | 4.94597 | 0.00479936 | 0.000970357 | 40.4459 | 1 | 1.33913 | 0.801764 | 238.334 | 5.27747 | F | F | 7.23e+19 | 0 | 1 | ds | |||||
| Report | 3 | X111651.99+570609.8 | chandra | ccd2 | 609.75 | 506.5 | 7.88302 | 2.82843 | 0.00154658 | 0.000554912 | 13.0493 | 1 | 0.723471 | 0.492 | 71.0142 | 5.12571 | F | F | 7.15e+19 | 0 | 1 | d | |||||
| Report | 2 | X111713.89+570426.8 | chandra | ccd2 | 246.5 | 298 | 7.52073 | 2.82844 | 0.0014755 | 0.000554913 | 12.4496 | 1 | 2.01738 | 0.492 | 3.99466 | 6.81521 | A | F | 7.13e+19 | 0 | 1 | d | |||||
| Report | 2 | X111554.62+570017.0 | chandra | ccd1 | 766.071 | 1057.64 | 6.87749 | 2.64575 | 0.00134848 | 0.000518757 | 11.39 | 1 | 0.859881 | 0.492 | 159.624 | 4.7839 | A | F | 7.23e+19 | 0 | 1 | d | |||||
| Report | 2 | X111611.25+570251.0 | chandra | ccd3 | 259.7 | 326.3 | 4.96061 | 2.23607 | 0.000973226 | 0.000438696 | 8.20175 | 0.999998 | 0.492 | 0.492 | 45 | 2.03721 | F | F | 7.2e+19 | 0 | 1 | d | |||||
| Report | 6 | X111622.20+570234.3 | chandra | ccd3 | 78.1001 | 292.3 | 4.95301 | 2.23607 | 0.000971735 | 0.000438696 | 8.18919 | 0.999998 | 0.492 | 0.492 | 13.2825 | 0.522547 | F | F | 7.19e+19 | 0 | 1 | d | |||||
| Report | 5 | X111620.53+570522.7 | chandra | ccd3 | 105.7 | 634.5 | 4.94268 | 2.23607 | 0.000969709 | 0.000438696 | 8.17211 | 0.999998 | 0.616111 | 0.492 | 123.286 | 3.01442 | F | F | 7.18e+19 | 0 | 1 | d | |||||
| Report | 4 | X111605.27+570416.3 | chandra | ccd3 | 358.7 | 499.7 | 4.91878 | 2.23607 | 0.000965019 | 0.000438696 | 8.13259 | 0.999998 | 0.656894 | 0.492 | 62.2961 | 3.34691 | F | F | 7.2e+19 | 0 | 1 | d | |||||
| Report | 1 | X111538.42+565834.0 | chandra | ccd1 | 1035.7 | 848.9 | 4.82952 | 2.23607 | 0.00094693 | 0.00043843 | 7.99827 | 0.999998 | 1.09581 | 0.492 | 66.1551 | 7.54868 | A | F | 7.25e+19 | 0 | 1 | d | |||||
| Report | 3 | X111607.63+570236.2 | chandra | ccd3 | 319.75 | 296.25 | 3.96217 | 2 | 0.000777342 | 0.000392382 | 6.55096 | 0.99996 | 0.492 | 0.492 | 45 | 2.49524 | F | F | 7.21e+19 | 0 | 1 | d | |||||
| Report | 7 | X111609.42+570206.7 | chandra | ccd3 | 290.25 | 236.25 | 3.94 | 2 | 0.000772991 | 0.000392382 | 6.5143 | 0.99996 | 0.492 | 0.492 | 18.4349 | 2.27476 | F | F | 7.21e+19 | 0 | 1 | d | |||||
| Report | 1 | X111711.56+570134.4 | chandra | ccd0 | 501.167 | 945.5 | 2.72895 | 1.73206 | 0.000535396 | 0.000339814 | 4.53298 | 0.999461 | 1.10456 | 0.492 | 53.4954 | 6.26718 | A | F | 7.15e+19 | 0 | 1 | d | |||||
| Report | 2 | X111650.61+570127.4 | chandra | ccd0 | 848.7 | 930.5 | 4.88864 | 2.23607 | 0.000959107 | 0.000438697 | 8.12037 | 0.999998 | 0.492 | 0.492 | 39.345 | 3.50101 | F | F | 7.17e+19 | 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