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 | X131800.25+325752.3 | chandra | ccd0 | 704.299 | 884.743 | 104.441 | 10.6769 | 0.0397314 | 0.00406172 | 47.7802 | 1 | 2.22337 | 1.26522 | 2.01395 | 6.64782 | F | F | 1.23e+20 | 0 | 1 | ds | |||||
| Report | 2 | X131838.46+330557.1 | chandra | ccd3 | 897.773 | 992.091 | 21.3055 | 4.69043 | 0.00810499 | 0.00178432 | 31.1529 | 1 | 1.53613 | 0.951953 | 79.402 | 7.09823 | A | F | 1.28e+20 | 0 | 1 | d | |||||
| Report | 5 | X131811.87+330037.3 | chandra | ccd1 | 559.768 | 200.763 | 17.7653 | 4.21489 | 0.00675829 | 0.00160343 | 44.6503 | 1 | 0.844697 | 0.844697 | 0 | 4.42216 | F | F | 1.25e+20 | 0 | 1 | ds | |||||
| Report | 6 | X131844.73+325901.0 | chandra | ccd3 | 737.692 | 147.011 | 11.4021 | 3.51248 | 0.00433759 | 0.00133622 | 16.6722 | 1 | 0.948972 | 0.204682 | 88.481 | 2.77636 | A | F | 1.29e+20 | 0 | 1 | ds | |||||
| Report | 3 | X131835.28+325906.7 | chandra | ccd3 | 979.284 | 158.38 | 10.2992 | 3.20924 | 0.00391804 | 0.00122086 | 15.0595 | 1 | 0.30911 | 0.30911 | 0 | 0.804212 | F | F | 1.28e+20 | 0 | 1 | ds | |||||
| Report | 1 | X131906.78+325552.7 | chandra | ccd2 | 10.7727 | 810.227 | 10.3538 | 3.31664 | 0.00393876 | 0.00126171 | 26.6473 | 1 | 1.90615 | 0.838736 | 98.6468 | 8.0377 | A | F | 1.32e+20 | 0 | 1 | d | |||||
| Report | 5 | X131845.71+330612.1 | chandra | ccd3 | 712.6 | 1022.7 | 9.56742 | 3.16229 | 0.00363962 | 0.00120299 | 13.9895 | 1 | 1.64567 | 0.655946 | 37.5001 | 7.78964 | A | F | 1.29e+20 | 0 | 1 | d | |||||
| Report | 1 | X131809.88+330110.0 | chandra | ccd1 | 610 | 266.875 | 7.92628 | 2.82843 | 0.0030153 | 0.00107599 | 19.9215 | 1 | 0.605258 | 0.492 | 139.642 | 5.01699 | F | F | 1.24e+20 | 0 | 1 | d | |||||
| Report | 3 | X131814.63+330318.4 | chandra | ccd1 | 488.625 | 527.625 | 7.91867 | 2.82843 | 0.00301241 | 0.00107599 | 19.9023 | 1 | 0.665224 | 0.492 | 45 | 5.56556 | F | F | 1.25e+20 | 0 | 1 | d | |||||
| Report | 4 | X131821.58+325703.0 | chandra | ccd0 | 158.738 | 784.152 | 14.1079 | 3.75605 | 0.00536695 | 0.00142888 | 6.45416 | 0.999999 | 0.506385 | 0.506385 | 0 | 2.85171 | F | F | 1.26e+20 | 0 | 1 | ds | |||||
| Report | 4 | X131757.75+330602.5 | chandra | ccd1 | 919.5 | 861.75 | 3.87384 | 2 | 0.00147368 | 0.000760837 | 9.73628 | 0.999999 | 1.002 | 0.496974 | 100.542 | 9.9745 | A | F | 1.23e+20 | 0 | 1 | d | |||||
| Report | 3 | X131837.56+325045.2 | chandra | ccd2 | 758.25 | 184.75 | 3.71975 | 2.00001 | 0.00141506 | 0.00076084 | 9.57345 | 0.999981 | 0.492 | 0.492 | 45 | 8.34951 | F | F | 1.29e+20 | 0 | 1 | d | |||||
| Report | 2 | X131811.42+330120.4 | chandra | ccd1 | 570.833 | 287.833 | 2.96049 | 1.73205 | 0.00112623 | 0.000658904 | 7.44074 | 0.999977 | 0.492 | 0.492 | 0 | 4.81032 | F | F | 1.25e+20 | 0 | 1 | d | |||||
| Report | 2 | X131831.13+325459.0 | chandra | ccd2 | 923 | 700.5 | 1.95874 | 1.41421 | 0.000745139 | 0.000537993 | 5.04116 | 0.999488 | 0.492 | 0.492 | 63.4349 | 4.02278 | F | F | 1.28e+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