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 | X134844.72-302944.2 | chandra | ccd2 | 324.941 | 807.604 | 173.864 | 13.4545 | 0.120418 | 0.0093186 | 64.9756 | 1 | 2.02051 | 1.0662 | 64.8476 | 5.89315 | F | F | 4.56e+20 | 1.50627e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X134857.92-302204.6 | chandra | ccd3 | 314.643 | 763.857 | 13.0033 | 3.74167 | 0.00900581 | 0.0025914 | 38.3971 | 1 | 2.23816 | 1.2073 | 84.1088 | 8.40224 | A | F | 4.61e+20 | 1.20153e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X134814.81-303303.8 | chandra | ccd2 | 1110.06 | 401.611 | 8.80396 | 3 | 0.00609742 | 0.00207773 | 3.29017 | 0.997013 | 1.40856 | 0.796847 | 70.1795 | 7.2909 | A | F | 4.55e+20 | 7.37199e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X134859.51-302206.3 | chandra | ccd3 | 272.7 | 760.3 | 8.78629 | 3.1623 | 0.00608518 | 0.00219014 | 25.9447 | 1 | 2.58679 | 1.82183 | 97.1528 | 8.69447 | F | F | 4.61e+20 | 8.22696e-14 | 1 | dx | ||||
| Report | 5 | X134831.77-302123.4 | chandra | ccd3 | 1002.36 | 848.071 | 6.96926 | 2.64575 | 0.00482675 | 0.00183239 | 20.5793 | 1 | 0.547008 | 0.492 | 69.9495 | 4.95774 | F | F | 4.63e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X134903.78-302410.7 | chandra | ccd3 | 160.786 | 507.357 | 6.47113 | 2.64577 | 0.00448176 | 0.0018324 | 19.1084 | 1 | 2.43826 | 1.58191 | 131.197 | 8.87657 | A | F | 4.59e+20 | 6.09079e-14 | 1 | dx | ||||
| Report | 3 | X134840.09-302454.0 | chandra | ccd3 | 783.7 | 419.9 | 4.96848 | 2.23607 | 0.00344106 | 0.00154865 | 14.6713 | 1 | 0.528476 | 0.492 | 113.745 | 3.7472 | F | F | 4.6e+20 | 0 | 1 | d | |||||
| Report | 6 | X134848.27-302126.9 | chandra | ccd3 | 568.25 | 840.75 | 3.99713 | 2 | 0.00276832 | 0.00138515 | 11.803 | 1 | 0.492 | 0.492 | 45 | 7.02883 | F | F | 4.62e+20 | 0 | 1 | d | |||||
| Report | 1 | X134816.67-301931.4 | chandra | ccd1 | 383.75 | 764.75 | 3.93436 | 2 | 0.00272485 | 0.00138516 | 13.0819 | 1 | 0.495859 | 0.492 | 15.1282 | 6.65756 | F | F | 4.64e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X134740.03-302745.2 | chandra | ccd0 | 1050.25 | 778.25 | 3.64975 | 2.00001 | 0.00252774 | 0.00138516 | 12.4523 | 0.999998 | 3.15441 | 0.494757 | 108.113 | 9.52753 | A | F | 4.59e+20 | 3.73397e-14 | 1 | dx | ||||
| Report | 2 | X134808.82-302648.9 | chandra | ccd0 | 293.833 | 893.5 | 2.98387 | 1.73205 | 0.00206656 | 0.00119958 | 10.1804 | 0.999998 | 0.492 | 0.492 | 2.41265e-08 | 3.26329 | F | F | 4.59e+20 | 0 | 1 | d | |||||
| Report | 3 | X134808.25-303015.0 | chandra | ccd0 | 308.5 | 474.5 | 0.990226 | 1 | 0.000685808 | 0.000692578 | 3.37847 | 0.996515 | 0.492 | 0.492 | 90 | 5.35939 | F | F | 4.57e+20 | 0 | 1 | d | |||||
| Report | 5 | X134755.28-302726.3 | chandra | ccd0 | 649.5 | 817.167 | 2.98924 | 1.73205 | 0.00207028 | 0.00119958 | 10.1988 | 0.999998 | 0.492 | 0.492 | 151.845 | 6.24515 | F | F | 4.59e+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