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 | X004111.84-210752.7 | chandra | ccd7 | 912.192 | 945.899 | 254.811 | 16.3483 | 0.032494 | 0.00208477 | 114.749 | 1 | 0.406346 | 0.406346 | 0 | 0.312139 | F | F | 1.49e+20 | 1.85716e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X004114.31-210737.1 | chandra | ccd7 | 841.776 | 977.625 | 44.6061 | 6.97115 | 0.00568825 | 0.000888974 | 20.0874 | 1 | 0.381418 | 0.381418 | 0 | 0.890541 | F | F | 1.5e+20 | 4.53055e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X004131.90-211217.2 | chandra | ccd7 | 341.983 | 408.191 | 25.2205 | 6.19352 | 0.00321617 | 0.00078981 | 11.3575 | 1 | 1.50716 | 1.50716 | 0 | 6.70852 | F | F | 1.5e+20 | 2.64308e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X004117.39-210856.3 | chandra | ccd7 | 754.248 | 816.706 | 17.8799 | 4.22846 | 0.00228008 | 0.000539222 | 8.05183 | 1 | 0.57639 | 0.57639 | 0 | 1.96672 | F | F | 1.5e+20 | 1.70857e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X004120.93-211031.2 | chandra | ccd7 | 653.874 | 623.863 | 12.9877 | 3.60385 | 0.00165621 | 0.000459568 | 5.84874 | 0.999996 | 0.720911 | 0.720911 | 0 | 3.65026 | F | F | 1.5e+20 | 1.27079e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X004112.45-211104.6 | chandra | ccd7 | 894.754 | 555.986 | 12.7061 | 3.56456 | 0.0016203 | 0.000454559 | 5.72192 | 0.999996 | 0.949407 | 0.229715 | 324.329 | 3.32167 | A | F | 1.49e+20 | 1.24869e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X004056.74-205827.7 | chandra | ccd6 | 664.591 | 1296.77 | 8.98127 | 3.31666 | 0.0011453 | 0.000422945 | 11.1849 | 1 | 3.05143 | 1.34831 | 124.686 | 9.86446 | A | F | 1.5e+20 | 1.5498e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X004115.54-211223.5 | chandra | ccd7 | 806.5 | 395 | 7.38113 | 2.82844 | 0.000941251 | 0.000360686 | 3.32394 | 0.998207 | 0.753625 | 0.492 | 37.9819 | 4.75223 | A | F | 1.49e+20 | 7.42478e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X004053.08-210822.8 | chandra | ccd6 | 768.071 | 87.2144 | 6.73865 | 2.64576 | 0.000859322 | 0.00033739 | 8.39205 | 1 | 0.679204 | 0.511046 | 0.79557 | 4.11945 | F | F | 1.49e+20 | 1.04369e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X004052.86-210714.9 | chandra | ccd6 | 774.5 | 225.3 | 4.82892 | 2.23607 | 0.000615789 | 0.000285147 | 6.01374 | 0.999942 | 0.565074 | 0.492 | 72.8566 | 4.16328 | F | F | 1.49e+20 | 7.1045e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X004054.48-210408.0 | chandra | ccd6 | 728.5 | 605.167 | 5.30785 | 2.44951 | 0.000676864 | 0.000312364 | 6.61019 | 0.999942 | 1.32101 | 0.803317 | 41.0464 | 5.2344 | A | F | 1.49e+20 | 7.94498e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X004051.02-210252.0 | chandra | ccd6 | 827 | 759.5 | 3.50957 | 2.00002 | 0.000447545 | 0.000255045 | 4.37067 | 0.999455 | 0.996084 | 0.492 | 4.21348 | 6.70465 | A | F | 1.49e+20 | 5.47756e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X004049.75-210644.2 | chandra | ccd6 | 862.833 | 287.5 | 5.92708 | 2.44949 | 0.000755829 | 0.000312362 | 7.38134 | 0.999995 | 0.492 | 0.492 | 180 | 4.96437 | F | F | 1.49e+20 | 9.62581e-15 | 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