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 | 1 | X033336.37-360825.4 | chandra | ccd7 | 672.653 | 226.575 | 1208.02 | 41.2932 | 0.0903966 | 0.00308999 | 136.24 | 1 | 0.460272 | 0.460272 | 0 | 0.128209 | F | F | 1.34e+20 | 0 | 1 | dsc | |||||
Report | 16 | X033334.62-360936.4 | chandra | ccd7 | 715.829 | 82.1244 | 617.953 | 25.5 | 0.0462415 | 0.00190817 | 69.6923 | 1 | 0.447645 | 0.447645 | 0 | 1.2386 | F | F | 1.36e+20 | 0 | 1 | ds | |||||
Report | 13 | X033336.02-360819.4 | chandra | ccd7 | 681.372 | 238.628 | 47.9732 | 13.9366 | 0.00358984 | 0.00104288 | 5.41039 | 1 | 1.0778 | 1.0778 | 0 | 0.0887357 | T | F | 1.34e+20 | 0 | 1 | ds | |||||
Report | 11 | X033344.28-360717.8 | chandra | ccd7 | 477.93 | 363.873 | 87.0094 | 9.51155 | 0.00651093 | 0.000711751 | 9.81286 | 1 | 0.443299 | 0.443299 | 0 | 2.03702 | F | F | 1.34e+20 | 0 | 1 | ds | |||||
Report | 12 | X033336.17-360829.7 | chandra | ccd7 | 677.566 | 217.757 | 353.948 | 22.4323 | 0.026486 | 0.00167862 | 39.918 | 1 | 3 | 3 | 0 | 0.160516 | T | F | 1.34e+20 | 0 | 1 | dsc | |||||
Report | 2 | X033312.83-361153.6 | chandra | ccd6 | 477.751 | 519.995 | 117.973 | 11.3587 | 0.00882792 | 0.000849969 | 35.4954 | 1 | 2.33945 | 1.55325 | 359.983 | 5.825 | F | F | 1.37e+20 | 0 | 1 | ds | |||||
Report | 9 | X033340.28-360726.6 | chandra | ccd7 | 576.404 | 345.884 | 49.7504 | 7.42079 | 0.00372283 | 0.000555299 | 5.61082 | 1 | 0.391963 | 0.391963 | 0 | 1.31343 | F | F | 1.34e+20 | 0 | 1 | ds | |||||
Report | 8 | X033341.84-360731.4 | chandra | ccd7 | 537.961 | 336.188 | 50.6675 | 7.24419 | 0.00379146 | 0.000542083 | 5.71425 | 1 | 0.408971 | 0.408971 | 0 | 1.49972 | F | F | 1.34e+20 | 0 | 1 | ds | |||||
Report | 5 | X033331.59-360808.6 | chandra | ccd7 | 790.35 | 260.672 | 44.8547 | 7.58094 | 0.00335648 | 0.000567283 | 5.05868 | 0.999999 | 0.396279 | 0.396279 | 0 | 0.878577 | F | F | 1.36e+20 | 0 | 1 | ds | |||||
Report | 1 | X033249.92-360359.2 | chandra | ccd2 | 223.31 | 372.367 | 28.9984 | 6.30324 | 0.00216995 | 0.000471672 | 8.85168 | 1 | 5.0101 | 2.3381 | 332.49 | 10.2595 | F | F | 1.39e+20 | 0 | 1 | ds | |||||
Report | 10 | X033337.31-360723.1 | chandra | ccd7 | 649.571 | 353.104 | 22.2211 | 5.26061 | 0.00166281 | 0.000393652 | 2.50608 | 0.991404 | 0.35725 | 0.35725 | 0 | 1.05262 | F | F | 1.34e+20 | 0 | 1 | ds | |||||
Report | 2 | X033332.34-360902.6 | chandra | ccd7 | 771.945 | 150.889 | 16.9961 | 4.36828 | 0.00127182 | 0.000326879 | 1.91681 | 0.968494 | 0.307787 | 0.307787 | 0 | 0.953135 | F | F | 1.36e+20 | 0 | 1 | ds | |||||
Report | 3 | X033330.34-360821.4 | chandra | ccd7 | 821.045 | 234.626 | 16.3537 | 5.05183 | 0.00122375 | 0.00037803 | 1.84436 | 0.960225 | 0.457433 | 0.457433 | 0 | 1.09701 | F | F | 1.36e+20 | 0 | 1 | ds | |||||
Report | 1 | X033312.20-361136.0 | chandra | ccd6 | 493 | 555.214 | 12.7308 | 3.74168 | 0.000952648 | 0.00027999 | 3.83042 | 0.999509 | 0.777707 | 0.593105 | 25.1174 | 5.73939 | F | F | 1.37e+20 | 0 | 1 | d | |||||
Report | 5 | X033323.21-361202.0 | chandra | ccd6 | 222.056 | 502.722 | 8.61869 | 3.00001 | 0.000644937 | 0.000224491 | 2.59317 | 0.990314 | 0.742105 | 0.492 | 175.143 | 4.43785 | A | F | 1.36e+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