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 | 8 | X092617.94-532244.3 | chandra | ccd3 | 46.2761 | 188.63 | 62.9855 | 7.93881 | 0.0194683 | 0.00245382 | 146.966 | 1 | 0.413631 | 0.413631 | 0 | 0.26879 | F | F | 9.32e+21 | 0 | 1 | ds | |||||
| Report | 1 | X092646.22-532741.7 | chandra | ccd0 | 668.35 | 489.4 | 19.1927 | 4.47215 | 0.00593226 | 0.00138229 | 47.3726 | 1 | 1.51509 | 0.862127 | 35.4309 | 6.28742 | A | T | 9.34e+21 | 0 | 1 | d | |||||
| Report | 2 | X092545.32-532310.6 | chandra | ccd3 | 638.944 | 134.167 | 8.88058 | 3 | 0.0027449 | 0.00092727 | 20.7213 | 1 | 0.630146 | 0.492 | 125.783 | 5.13831 | F | F | 9.24e+21 | 0 | 1 | d | |||||
| Report | 1 | X092530.22-532639.2 | chandra | ccd1 | 1046.28 | 752.389 | 8.22353 | 3.00002 | 0.00254181 | 0.000927274 | 19.7977 | 1 | 2.18374 | 1.38745 | 121.157 | 8.31554 | A | T | 9.16e+21 | 0 | 1 | d | |||||
| Report | 7 | X092542.30-532211.1 | chandra | ccd3 | 694 | 255 | 5.90419 | 2.44949 | 0.00182493 | 0.000757113 | 13.7764 | 1 | 0.8712 | 0.492 | 159.407 | 5.60981 | A | F | 9.25e+21 | 0 | 1 | d | |||||
| Report | 1 | X092625.09-530432.1 | chandra | ccd6 | 992 | 899.167 | 5.21336 | 2.44951 | 0.0016114 | 0.000757119 | 12.0052 | 1 | 3.29298 | 0.492 | 136.693 | 18.289 | A | T | 9.36e+21 | 0 | 1 | d | |||||
| Report | 1 | X092610.01-532205.5 | chandra | ccd3 | 190 | 267 | 3.96451 | 2 | 0.00122539 | 0.00061818 | 9.25049 | 0.999999 | 0.492 | 0.492 | 67.5 | 1.6099 | F | T | 9.31e+21 | 0 | 1 | d | |||||
| Report | 4 | X092614.76-532001.9 | chandra | ccd3 | 103.75 | 518.25 | 3.95672 | 2 | 0.00122298 | 0.00061818 | 9.23231 | 0.999999 | 0.492 | 0.492 | 149.872 | 2.86963 | F | F | 9.34e+21 | 0 | 1 | d | |||||
| Report | 3 | X092614.23-532141.3 | chandra | ccd3 | 113.167 | 316.167 | 2.99201 | 1.73205 | 0.0009248 | 0.000535359 | 6.98134 | 0.999959 | 0.492 | 0.492 | 45 | 1.38129 | F | F | 9.32e+21 | 0 | 1 | d | |||||
| Report | 6 | X092611.61-531759.4 | chandra | ccd3 | 161.167 | 767.167 | 2.97704 | 1.73205 | 0.000920174 | 0.000535359 | 6.94641 | 0.999959 | 0.492 | 0.492 | 90 | 4.96369 | F | F | 9.36e+21 | 0 | 1 | d | |||||
| Report | 2 | X092627.85-532405.0 | chandra | ccd0 | 1001.5 | 930.167 | 2.97607 | 1.73205 | 0.000919872 | 0.000535359 | 7.34572 | 0.999973 | 0.492 | 0.492 | 90 | 1.76512 | F | F | 9.33e+21 | 0 | 1 | d | |||||
| Report | 3 | X092626.26-532605.4 | chandra | ccd0 | 1030.5 | 685.4 | 9.91407 | 3.16228 | 0.00306434 | 0.000977428 | 24.4706 | 1 | 0.540853 | 0.492 | 49.2654 | 3.42796 | F | F | 9.31e+21 | 0 | 1 | d | |||||
| Report | 5 | X092550.40-531945.2 | chandra | ccd3 | 547.167 | 551.833 | 2.96706 | 1.73205 | 0.000917086 | 0.000535359 | 6.9231 | 0.999959 | 0.492 | 0.492 | 16.845 | 5.33017 | F | F | 9.3e+21 | 0 | 1 | d | |||||
| Report | 1 | X092707.82-532228.3 | chandra | ccd2 | 194.5 | 69.5 | 0.885564 | 1.00001 | 0.000273719 | 0.000309091 | 2.19456 | 0.988098 | 0.492 | 0.492 | 90 | 7.1864 | F | T | 9.46e+21 | 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