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 | X110714.99-183901.6 | chandra | ccd3 | 1083.27 | 377.208 | 51.994 | 7.21069 | 0.029976 | 0.00415717 | 177.155 | 1 | 0.482086 | 0.482086 | 0 | 1.21542 | F | F | 3.88e+20 | 0 | 1 | ds | |||||
| Report | 1 | X110731.40-183821.8 | chandra | ccd3 | 609.045 | 458.127 | 27.4511 | 5.23938 | 0.0158263 | 0.00302065 | 93.5318 | 1 | 0.807189 | 0.807189 | 0 | 4.81967 | F | F | 3.84e+20 | 0 | 1 | ds | |||||
| Report | 1 | X110640.65-184357.5 | chandra | ccd0 | 785.214 | 491 | 12.9783 | 3.74168 | 0.00748223 | 0.00215714 | 44.1095 | 1 | 2.60031 | 1.68271 | 158.069 | 8.45883 | A | F | 3.92e+20 | 0 | 1 | d | |||||
| Report | 1 | X110651.79-183039.0 | chandra | ccd1 | 735.5 | 1150.2 | 9.58461 | 3.16229 | 0.00552569 | 0.00182311 | 31.5465 | 1 | 2.85905 | 0.931833 | 5.15338 | 10.6135 | A | F | 3.97e+20 | 0 | 1 | d | |||||
| Report | 3 | X110708.19-183626.7 | chandra | ccd1 | 261.167 | 443.5 | 5.98102 | 2.44949 | 0.00344816 | 0.00141217 | 19.6858 | 1 | 0.492 | 0.492 | 24.1832 | 3.76207 | F | F | 3.91e+20 | 0 | 1 | d | |||||
| Report | 1 | X110741.67-184412.8 | chandra | ccd2 | 53.3333 | 762 | 5.93346 | 2.44949 | 0.00342074 | 0.00141217 | 19.8497 | 1 | 1.24593 | 0.520301 | 110.466 | 8.0768 | A | F | 3.79e+20 | 0 | 1 | d | |||||
| Report | 3 | X110708.98-184257.7 | chandra | ccd2 | 997.3 | 914.9 | 4.98868 | 2.23607 | 0.00287606 | 0.00128913 | 16.689 | 1 | 0.613615 | 0.492 | 164.086 | 2.99763 | F | F | 3.88e+20 | 0 | 1 | d | |||||
| Report | 2 | X110709.05-184218.9 | chandra | ccd2 | 995.3 | 993.7 | 4.96117 | 2.23607 | 0.0028602 | 0.00128913 | 16.597 | 1 | 0.634959 | 0.492 | 88.5688 | 2.37611 | F | F | 3.88e+20 | 0 | 1 | d | |||||
| Report | 4 | X110710.92-184454.0 | chandra | ccd2 | 941.167 | 678.5 | 2.99039 | 1.73205 | 0.00172401 | 0.000998557 | 10.004 | 0.999998 | 0.492 | 0.492 | 61.845 | 4.83807 | F | F | 3.86e+20 | 0 | 1 | d | |||||
| Report | 5 | X110708.32-184515.2 | chandra | ccd2 | 1016.17 | 635.5 | 2.98048 | 1.73205 | 0.00171829 | 0.000998557 | 9.97083 | 0.999998 | 0.492 | 0.492 | 3.1007e-08 | 5.26667 | F | F | 3.86e+20 | 0 | 1 | d | |||||
| Report | 2 | X110719.11-183353.2 | chandra | ccd3 | 963.5 | 1003.5 | 2.94822 | 1.73205 | 0.0016997 | 0.000998558 | 10.0452 | 0.999998 | 0.492 | 0.492 | 45 | 6.38917 | F | F | 3.9e+20 | 0 | 1 | d | |||||
| Report | 2 | X110646.38-183402.0 | chandra | ccd1 | 891.5 | 737.5 | 2.8457 | 1.73205 | 0.00164059 | 0.000998559 | 9.36627 | 0.999878 | 1.34613 | 0.492 | 36.2372 | 8.62827 | A | F | 3.97e+20 | 0 | 1 | d | |||||
| Report | 2 | X110649.16-184253.9 | chandra | ccd0 | 539.5 | 620.5 | 0.976054 | 1 | 0.000562712 | 0.000576518 | 3.31732 | 0.996462 | 0.492 | 0.492 | 90 | 6.18136 | F | F | 3.92e+20 | 0 | 1 | d | |||||
| Report | 3 | X110702.14-184457.9 | chandra | ccd0 | 164.625 | 368.625 | 7.92088 | 2.82843 | 0.00456652 | 0.00163064 | 26.9207 | 1 | 0.537905 | 0.492 | 90 | 5.45813 | F | F | 3.88e+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