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 | 1 | X141309.95-652020.8 | chandra | ccd7 | 179.814 | 610.662 | 5348.03 | 82.0899 | 0.292097 | 0.00448357 | 392.751 | 1 | 0.552875 | 0.552875 | 0 | 1.88126 | F | F | 5.58e+21 | 6.97174e-12 | 1 | dscxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X141310.08-652029.5 | chandra | ccd7 | 178.262 | 592.945 | 114.923 | 14.7435 | 0.00627686 | 0.000805263 | 8.43977 | 1 | 0.487229 | 0.487229 | 0 | 2.02237 | F | F | 5.58e+21 | 6.31524e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X141311.25-652018.3 | chandra | ccd7 | 163.364 | 615.755 | 78.8123 | 14.1637 | 0.00430455 | 0.000773588 | 5.78786 | 1 | 0.419845 | 0.419845 | 0 | 1.89457 | F | F | 5.58e+21 | 4.3031e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 4 | X141310.25-652017.7 | chandra | ccd7 | 175.591 | 616.454 | 258.65 | 17.1466 | 0.0141269 | 0.000936506 | 18.9948 | 1 | 0.492 | 0.492 | 4.29893 | 1.84484 | F | F | 5.58e+21 | 1.41629e-13 | 1 | dpx | ||||
| Report | srcpi bgdpi arf rmf | 5 | X141309.44-652019.0 | chandra | ccd7 | 186.396 | 614.396 | 939.619 | 33.2459 | 0.0513199 | 0.00181582 | 69.0042 | 1 | 1.5 | 1.5 | 0 | 1.79916 | T | F | 5.58e+21 | 5.15041e-13 | 1 | dpscx | ||||
| Report | srcpi bgdpi arf rmf | 6 | X141312.22-652013.6 | chandra | ccd7 | 150.982 | 625.285 | 453.633 | 22.2393 | 0.0247764 | 0.00121466 | 33.3141 | 1 | 0.489403 | 0.397348 | 352.645 | 1.87159 | F | T | 5.59e+21 | 3.82311e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 7 | X141310.03-652044.4 | chandra | ccd7 | 178.831 | 562.677 | 2808.92 | 54.1133 | 0.153417 | 0.00295555 | 206.283 | 1 | 0.565706 | 0.403279 | 158.155 | 2.25678 | F | F | 5.56e+21 | 1.54756e-12 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X141305.55-652031.2 | chandra | ccd7 | 235.852 | 589.496 | 27.1522 | 7.67509 | 0.00148299 | 0.000419196 | 1.99402 | 0.974715 | 0.357255 | 0.357255 | 0 | 1.94636 | F | F | 5.58e+21 | 1.52385e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 10 | X141312.17-652007.1 | chandra | ccd7 | 151.596 | 638.648 | 53.2654 | 7.30615 | 0.00290924 | 0.000399045 | 3.91173 | 0.999909 | 0.470328 | 0.407846 | 0 | 1.7731 | F | F | 5.59e+21 | 5.14966e-14 | 1 | dspx | ||||
| Report | srcpi bgdpi arf | 11 | X141310.13-652001.9 | chandra | ccd7 | 177.523 | 649.109 | 63.6917 | 8.95752 | 0.0034787 | 0.00048924 | 4.67742 | 0.999996 | 0.38287 | 0.38287 | 0 | 1.59883 | F | F | 5.6e+21 | 3.48448e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 13 | X141308.63-652023.8 | chandra | ccd7 | 196.649 | 604.593 | 62.6181 | 15.1708 | 0.00342006 | 0.000828595 | 4.59858 | 0.999995 | 1.1712 | 1.1712 | 0 | 1.88781 | T | F | 5.58e+21 | 3.44901e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 14 | X141308.03-652005.5 | chandra | ccd7 | 204.334 | 641.927 | 50.0399 | 10.6687 | 0.00273307 | 0.0005827 | 3.67485 | 0.9998 | 1.5 | 1.5 | 0 | 1.54867 | T | F | 5.59e+21 | 2.75645e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 15 | X141312.53-652052.5 | chandra | ccd7 | 147.095 | 546.234 | 107.455 | 10.5747 | 0.00586894 | 0.000577566 | 7.89133 | 1 | 0.567411 | 0.567411 | 0 | 2.47129 | F | F | 5.56e+21 | 5.89946e-14 | 1 | dsx |
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