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 | 1 | X100119.94-710214.5 | chandra | ccd7 | 867.611 | 923.944 | 8.49081 | 4.1225 | 0.00265412 | 0.00128864 | 11.899 | 1 | 0.928872 | 0.797902 | 174.429 | 6.56984 | 6.85452 | 0.781776 | -0.795247 | 0.669257 | F | F | 8.15e+20 | 2.26179e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X100158.72-710322.9 | chandra | ccd7 | 483.5 | 785.3 | 14.8306 | 4.96863 | 0.00463587 | 0.00155313 | 36.0346 | 1 | 0.492 | 0.492 | 90 | 4.76503 | 6.91531 | 7.91531 | 0.0674281 | 0.337906 | F | F | 8.04e+20 | 3.83079e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X100120.40-710242.0 | chandra | ccd7 | 862.929 | 867.929 | 6.65666 | 3.78388 | 0.00208079 | 0.00118279 | 11.3603 | 1 | 1.33467 | 0.492 | 19.5922 | 6.14303 | 5.96879 | 0.750295 | -0.776668 | 0.72145 | A | F | 8.13e+20 | 1.74456e-14 | 1 | dx |
| Report | 5 | X100141.67-710440.4 | chandra | ccd7 | 652.1 | 627.7 | 4.92148 | 2.23607 | 0.00153839 | 0.000698968 | 6.44731 | 0.999967 | 0.492 | 0.492 | 71.0625 | 3.64644 | F | F | 8.04e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X100126.71-711154.7 | chandra | ccd6 | 795.25 | 786.75 | 3.91531 | 3.17945 | 0.00122391 | 0.000993882 | 13.4537 | 1 | 0.492 | 0.492 | 45 | 4.4358 | 2 | 1.91531 | -0.0216313 | 0.82671 | F | F | 7.91e+20 | 1.40882e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X100114.22-710643.1 | chandra | ccd7 | 922.75 | 377.75 | 3.91531 | 3.17945 | 0.00122388 | 0.000993857 | 13.4537 | 1 | 0.492 | 0.492 | 45 | 3.6388 | 2.91531 | 1 | -0.489184 | 0.920111 | F | F | 8.04e+20 | 1.01593e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 7 | X100222.29-710813.8 | chandra | ccd7 | 251.25 | 193.75 | 3.83061 | 3.17945 | 0.0011974 | 0.000993857 | 9.30741 | 0.999999 | 0.492 | 0.492 | 45 | 2.15652 | -0.169387 | 4 | 1 | 1.14412 | F | F | 7.9e+20 | 9.3499e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X100233.88-711241.2 | chandra | ccd6 | 135.5 | 692.167 | 2.92422 | 2.93649 | 0.000914097 | 0.000917934 | 10.6224 | 0.999999 | 0.550073 | 0.492 | 161.565 | 5.49363 | 1.92422 | 1 | -0.316056 | 1.07594 | F | F | 7.82e+20 | 1.08267e-14 | 1 | dx |
| Report | 3 | X100226.43-711446.2 | chandra | ccd6 | 209.167 | 438.167 | 2.96831 | 1.73205 | 0.000927882 | 0.000541432 | 6.11821 | 0.999894 | 0.704961 | 0.492 | 168.019 | 7.07919 | F | F | 7.81e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X100148.18-711409.1 | chandra | ccd6 | 584.167 | 513.833 | 2.90326 | 2.93649 | 0.000907545 | 0.000917934 | 9.33411 | 0.999997 | 0.861 | 0.492 | 45 | 6.04183 | 3 | -0.0967441 | -1 | 1.41421 | A | F | 7.83e+20 | 1.07826e-14 | 1 | dx |
| Report | 5 | X100149.03-711310.4 | chandra | ccd6 | 575.833 | 633.167 | 2.97164 | 1.73205 | 0.000928921 | 0.000541432 | 6.12506 | 0.999894 | 0.492 | 0.492 | 90 | 5.06143 | F | F | 7.85e+20 | 0 | 1 | d | |||||
| Report | 6 | X100202.22-710922.8 | chandra | ccd7 | 449.167 | 53.8333 | 2.92272 | 1.73205 | 0.000913607 | 0.000541418 | 3.82887 | 0.996972 | 0.563657 | 0.492 | 45 | 1.34876 | F | F | 7.91e+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