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 | 2 | X173353.12-300132.4 | chandra | ccd1 | 719.438 | 32.5625 | 14.1929 | 4.00003 | 0.00658959 | 0.00185716 | 30.596 | 1 | 2.82173 | 1.54434 | 9.72032 | 8.80648 | A | F | 7.05e+21 | 1.60588e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X173325.73-300111.5 | chandra | ccd3 | 412.5 | 128 | 9.80317 | 3.16228 | 0.00454493 | 0.00146609 | 20.2202 | 1 | 0.821987 | 0.533173 | 65.0304 | 8.02501 | A | F | 6.75e+21 | 6.86796e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X173410.95-294511.9 | chandra | ccd0 | 192.5 | 980 | 5.00492 | 2.44952 | 0.00232037 | 0.00113564 | 10.4051 | 1 | 2.49795 | 1.94407 | 132.487 | 11.1853 | F | F | 6.67e+21 | 3.82975e-14 | 1 | dx | ||||
| Report | 2 | X173334.61-295134.9 | chandra | ccd2 | 114.1 | 269.1 | 4.95176 | 2.23607 | 0.00229573 | 0.00103668 | 10.2543 | 1 | 0.492 | 0.492 | 25.0972 | 1.96776 | F | F | 6.51e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X173315.85-295908.5 | chandra | ccd3 | 673.5 | 377.9 | 4.83614 | 2.23607 | 0.00224213 | 0.00103669 | 9.9751 | 1 | 0.850052 | 0.492 | 160.097 | 7.18377 | A | F | 6.53e+21 | 3.33663e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X173308.46-295728.1 | chandra | ccd3 | 868.9 | 581.9 | 4.81899 | 2.23607 | 0.00223417 | 0.00103669 | 9.93973 | 1 | 1.14427 | 0.706308 | 108.127 | 7.23907 | A | F | 6.4e+21 | 3.45467e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X173320.70-295809.3 | chandra | ccd3 | 545.5 | 498.25 | 3.96856 | 2 | 0.0018399 | 0.000927238 | 8.18562 | 0.999995 | 0.492 | 0.492 | 90 | 5.76248 | F | F | 6.56e+21 | 2.84692e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X173331.57-294948.9 | chandra | ccd2 | 194.5 | 484.5 | 3.96778 | 2 | 0.00183954 | 0.000927238 | 8.21667 | 0.999995 | 0.492 | 0.492 | 2.35031e-08 | 3.84144 | F | F | 6.42e+21 | 2.59288e-14 | 1 | dx | ||||
| Report | 6 | X173310.52-300010.8 | chandra | ccd3 | 814.25 | 251.25 | 3.68196 | 2.00001 | 0.00170703 | 0.000927241 | 7.59448 | 0.999895 | 0.999745 | 0.492 | 64.6847 | 8.71821 | A | F | 6.5e+21 | 0 | 1 | d | |||||
| Report | 4 | X173339.06-295345.6 | chandra | ccd3 | 60.5 | 1034.5 | 2.94974 | 1.73205 | 0.00136755 | 0.000803013 | 6.08417 | 0.999895 | 0.492 | 0.492 | 90 | 0.622363 | F | F | 6.62e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X173359.55-294948.6 | chandra | ccd0 | 494.5 | 417.833 | 2.90215 | 1.73205 | 0.00134549 | 0.000803012 | 6.03348 | 0.999901 | 0.492 | 0.492 | 90 | 6.22975 | F | F | 6.69e+21 | 1.97254e-14 | 1 | dx | ||||
| Report | 1 | X173343.83-295707.8 | chandra | ccd1 | 964.5 | 570.5 | 1.99384 | 1.41421 | 0.000925714 | 0.0006566 | 4.29816 | 0.998586 | 0.492 | 0.492 | 90 | 3.95936 | F | F | 6.76e+21 | 0 | 1 | d | |||||
| Report | 5 | X173320.58-300044.2 | chandra | ccd3 | 548.5 | 183.5 | 0.881862 | 1.00001 | 0.000408848 | 0.000463622 | 1.81894 | 0.976345 | 0.492 | 0.492 | 90 | 8.00156 | F | F | 6.66e+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