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 | X141028.14+135950.2 | chandra | ccd7 | 481.876 | 908.168 | 68.9185 | 8.53167 | 0.0171042 | 0.00211739 | 69.8679 | 1 | 0.374598 | 0.374598 | 0 | 0.291706 | F | F | 1.43e+20 | 1.2702e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X141014.82+135350.6 | chandra | ccd7 | 876.179 | 177.16 | 69.1616 | 8.31635 | 0.0171645 | 0.00206395 | 70.1144 | 1 | 1.94526 | 1.94526 | 0 | 7.09823 | F | F | 1.44e+20 | 1.44964e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X141100.09+134654.1 | chandra | ccd3 | 308.405 | 429.381 | 26.7018 | 6.48094 | 0.00662683 | 0.00160843 | 50.8811 | 1 | 6.71821 | 4.49845 | 52.2263 | 15.2849 | F | F | 1.45e+20 | 9.96947e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X141043.89+140802.8 | chandra | ccd6 | 756.964 | 1208.96 | 23.8294 | 5.29156 | 0.00591395 | 0.00131325 | 45.0567 | 1 | 3.47957 | 2.88382 | 29.479 | 8.76667 | F | F | 1.41e+20 | 8.23579e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X141029.82+135806.8 | chandra | ccd7 | 432.159 | 697.997 | 14.0348 | 3.7463 | 0.00348316 | 0.000929759 | 14.2281 | 1 | 0.482357 | 0.482357 | 0 | 2.03195 | F | F | 1.43e+20 | 2.6005e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X141024.25+135418.4 | chandra | ccd7 | 596.643 | 233.214 | 14.699 | 3.87299 | 0.00364798 | 0.000961193 | 14.9015 | 1 | 0.492 | 0.492 | 54.9916 | 5.90123 | F | F | 1.44e+20 | 3.35029e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X141046.99+140011.8 | chandra | ccd6 | 664.928 | 251.643 | 6.83164 | 2.64576 | 0.00169547 | 0.00065662 | 12.9173 | 1 | 1.0039 | 0.492 | 16.7988 | 4.49488 | A | F | 1.42e+20 | 1.95875e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X141026.07+135719.6 | chandra | ccd7 | 542.7 | 601.5 | 4.86236 | 2.23607 | 0.00120673 | 0.000554945 | 4.92934 | 0.999484 | 0.492 | 0.492 | 53.3496 | 2.85165 | F | F | 1.43e+20 | 9.17315e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X141059.11+135650.3 | chandra | ccd2 | 1126.25 | 952.25 | 3.78698 | 2.00001 | 0.000940572 | 0.000496741 | 7.00653 | 0.999986 | 0.492 | 0.492 | 7.01812 | 8.12585 | F | F | 1.43e+20 | 1.3261e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X141046.22+135951.8 | chandra | ccd6 | 687.5 | 211 | 1.95655 | 1.41422 | 0.000485574 | 0.000350978 | 3.69945 | 0.997038 | 0.492 | 0.492 | 90 | 4.31659 | F | F | 1.42e+20 | 5.61841e-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