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 | X235034.19-255315.7 | chandra | ccd2 | 1090.83 | 758.167 | 5.89613 | 2.44949 | 0.00125131 | 0.000519847 | 10.9939 | 1 | 0.562382 | 0.492 | 70.0972 | 5.79766 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 1 | X235028.48-255439.2 | chandra | ccd3 | 216.5 | 773.5 | 4.90786 | 2.23607 | 0.00104158 | 0.000474553 | 9.29644 | 0.999999 | 0.492 | 0.492 | 28.155 | 4.76555 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 2 | X235008.93-255916.0 | chandra | ccd3 | 751.9 | 210.5 | 4.89782 | 2.23607 | 0.00103945 | 0.000474553 | 9.27743 | 0.999999 | 0.675996 | 0.492 | 38.5625 | 6.28504 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 3 | X235041.65-255705.5 | chandra | ccd2 | 886.25 | 291.25 | 3.95778 | 2 | 0.000839945 | 0.000424453 | 7.37964 | 0.999987 | 0.492 | 0.492 | 45 | 2.21415 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 2 | X235013.59-260320.9 | chandra | ccd1 | 827 | 765 | 3.95376 | 2 | 0.000839091 | 0.000424453 | 7.73198 | 0.999992 | 0.492 | 0.492 | 103.283 | 6.78558 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 1 | X235101.07-260327.7 | chandra | ccd0 | 543.5 | 543 | 3.90047 | 2 | 0.000827781 | 0.000424453 | 4.50986 | 0.998948 | 0.841606 | 0.492 | 127.982 | 7.0137 | A | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 2 | X235033.10-255154.4 | chandra | ccd2 | 1120.75 | 923.5 | 3.85039 | 2 | 0.000817155 | 0.000424453 | 7.17941 | 0.999987 | 0.595276 | 0.492 | 39.6902 | 7.17233 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 4 | X235023.29-255857.5 | chandra | ccd3 | 358.5 | 248.5 | 2.98212 | 1.73205 | 0.000632885 | 0.000367587 | 5.64872 | 0.999799 | 0.492 | 0.492 | 90 | 3.0553 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 3 | X235024.77-255608.7 | chandra | ccd3 | 318 | 591.5 | 1.97396 | 1.41421 | 0.000418927 | 0.000300133 | 3.73907 | 0.997068 | 0.492 | 0.492 | 180 | 3.96473 | F | F | 1.73e+20 | 0 | 1 | d | |||||
| Report | 1 | X235008.26-260653.1 | chandra | ccd1 | 972.5 | 333.5 | 0.982605 | 1 | 0.000208535 | 0.000212226 | 1.92159 | 0.971228 | 0.492 | 0.492 | 90 | 10.1514 | F | F | 1.72e+20 | 0 | 1 | d | |||||
| Report | 3 | X235107.80-255852.9 | chandra | ccd0 | 359.292 | 1102.37 | 31.2992 | 5.66103 | 0.00664255 | 0.00120143 | 36.1892 | 1 | 2.35222 | 2.35222 | 0 | 6.92282 | F | F | 1.73e+20 | 0 | 1 | ds |
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