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 rmf | 3 | X110926.43-650224.9 | chandra | ccd2 | 197.226 | 282.62 | 895.381 | 30.2325 | 0.175151 | 0.00591398 | 1362.42 | 1 | 1.14637 | 0.843698 | 4.11468 | 5.77729 | F | T | 5.21e+21 | 2.51556e-12 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X110947.76-645245.4 | chandra | ccd1 | 1021.83 | 486.956 | 31.8989 | 5.64791 | 0.00623997 | 0.00110483 | 50.6981 | 1 | 0.940948 | 0.53721 | 89.9746 | 4.16524 | F | F | 5.72e+21 | 8.55774e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X110924.82-651223.6 | chandra | ccd7 | 994.5 | 490.643 | 14.0635 | 4.58269 | 0.00275105 | 0.000896451 | 13.8542 | 1 | 5.79068 | 2.99231 | 146.093 | 15.6267 | A | F | 4.82e+21 | 3.76834e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X110948.48-645924.8 | chandra | ccd3 | 953.813 | 704.322 | 12.9403 | 3.59726 | 0.00253296 | 0.000704136 | 20.3729 | 1 | 0.441227 | 0.441227 | 0 | 2.64305 | F | F | 5.43e+21 | 3.41581e-14 | 1 | dsx | ||||
| Report | 1 | X110908.06-645810.7 | chandra | ccd2 | 434.667 | 798.833 | 9.93292 | 3.16228 | 0.00194305 | 0.000618595 | 15.114 | 1 | 0.492 | 0.492 | 149.679 | 3.79854 | F | F | 5.36e+21 | 0 | 1 | d | |||||
| Report | 1 | X111017.30-645747.5 | chandra | ccd3 | 581.375 | 900.875 | 7.89041 | 2.82843 | 0.00154446 | 0.000553635 | 12.4225 | 1 | 0.492 | 0.492 | 113.645 | 3.87344 | F | F | 5.57e+21 | 0 | 1 | d | |||||
| Report | 2 | X111022.50-645410.8 | chandra | ccd1 | 572.167 | 312.333 | 5.96167 | 2.44949 | 0.0011662 | 0.000479161 | 9.47511 | 1 | 0.492 | 0.492 | 57.1139 | 5.08599 | F | F | 5.75e+21 | 0 | 1 | d | |||||
| Report | 9 | X111034.56-650255.0 | chandra | ccd3 | 360.833 | 275.333 | 5.85463 | 2.44949 | 0.00114598 | 0.000479462 | 9.21739 | 1 | 0.492 | 0.492 | 26.5651 | 8.22823 | F | T | 5.4e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X111004.07-650153.1 | chandra | ccd3 | 752.833 | 402.167 | 5.82979 | 2.44949 | 0.00114112 | 0.000479462 | 9.17829 | 1 | 0.817842 | 0.492 | 25.5362 | 5.54216 | A | F | 5.36e+21 | 1.58599e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X111019.05-645448.3 | chandra | ccd1 | 616.9 | 236.1 | 4.9435 | 2.23607 | 0.000967032 | 0.000437413 | 7.85689 | 0.999996 | 0.492 | 0.492 | 79.0993 | 4.4573 | F | T | 5.71e+21 | 1.27584e-14 | 1 | dx | ||||
| Report | 6 | X111008.80-645857.9 | chandra | ccd3 | 691.3 | 758.1 | 4.90959 | 2.23607 | 0.000960999 | 0.000437687 | 7.72955 | 0.999996 | 0.638414 | 0.492 | 173.215 | 3.54669 | F | F | 5.5e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X111049.24-645705.5 | chandra | ccd3 | 168.9 | 984.9 | 4.83462 | 2.23607 | 0.000946324 | 0.000437687 | 7.61152 | 0.999996 | 0.492 | 0.492 | 180 | 7.14701 | F | T | 5.69e+21 | 1.32975e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X110854.26-650004.5 | chandra | ccd2 | 611.9 | 567.1 | 4.83376 | 2.23607 | 0.000945564 | 0.000437413 | 7.35509 | 0.999994 | 0.645883 | 0.492 | 174.345 | 5.95846 | F | F | 5.24e+21 | 1.36599e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X111045.16-645807.4 | chandra | ccd3 | 222.1 | 859.3 | 4.51444 | 2.23608 | 0.000883652 | 0.000437689 | 7.10743 | 0.999936 | 1.08772 | 0.671414 | 146.375 | 6.82569 | A | F | 5.63e+21 | 1.23554e-14 | 1 | dx |
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