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 | 1 | X133959.24-642444.1 | chandra | ccd1 | 1094.92 | 461.049 | 25.9489 | 5.51685 | 0.00519548 | 0.00110458 | 12.2505 | 1 | 1.01004 | 0.374876 | 113.262 | 4.44209 | 10.9371 | 15.8114 | 0.182225 | 0.239083 | F | F | 1.03e+22 | 8.17902e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X134010.53-643436.6 | chandra | ccd2 | 198.236 | 539.807 | 19.2568 | 4.38826 | 0.00385559 | 0.000878615 | 33.1889 | 1 | 1.55403 | 0.79 | 17.1328 | 5.57472 | 19.7848 | -0.258257 | -1 | 0.399042 | F | F | 9.43e+21 | 6.25581e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X133949.45-643153.8 | chandra | ccd2 | 474.562 | 870.586 | 15.9594 | 3.99492 | 0.0031954 | 0.000799865 | 27.5059 | 1 | 0.750098 | 0.750098 | 0 | 3.58433 | 12.8305 | 3.91527 | -0.532388 | 0.354676 | F | F | 9.68e+21 | 4.84683e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X134038.46-643225.7 | chandra | ccd3 | 828.145 | 503.519 | 8.57451 | 3.50055 | 0.00171676 | 0.000700869 | 4.47015 | 0.999876 | 0.927303 | 0.250368 | 59.2043 | 4.60696 | 7.95426 | 0.95426 | -0.785765 | 0.594207 | F | F | 9.59e+21 | 2.78666e-14 | 1 | dsx |
Report | 3 | X134021.54-642655.9 | chandra | ccd1 | 800.9 | 192.6 | 9.9061 | 3.16228 | 0.0019834 | 0.000633151 | 4.67667 | 0.999929 | 0.582477 | 0.492 | 88.325 | 2.47144 | F | F | 1.01e+22 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 4 | X133948.41-643625.1 | chandra | ccd2 | 487 | 318.625 | 7.82836 | 3.95804 | 0.00156738 | 0.000792472 | 18.8959 | 1 | 1.1786 | 0.796354 | 30.7785 | 7.72217 | 5.94279 | 1.88558 | -0.518271 | 0.575509 | F | F | 9.3e+21 | 2.68634e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X134109.85-643315.0 | chandra | ccd3 | 416.7 | 401.7 | 4.47768 | 3.39792 | 0.000896507 | 0.000680319 | 6.19564 | 0.999982 | 0.558444 | 0.492 | 122.268 | 7.73634 | 3.62692 | 0.850766 | -0.619997 | 0.906425 | F | F | 9.46e+21 | 1.52972e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X134001.75-643115.9 | chandra | ccd2 | 312.9 | 947.3 | 4.74592 | 3.39792 | 0.00095022 | 0.000680325 | 9.41532 | 1 | 0.492 | 0.492 | 166.717 | 2.37948 | 5 | -0.169387 | -1 | 0.975663 | F | F | 9.73e+21 | 1.41298e-14 | 1 | dx |
Report | 5 | X134016.76-643143.4 | chandra | ccd3 | 1112 | 589.25 | 3.96015 | 2 | 0.000792889 | 0.000400434 | 2.06455 | 0.965711 | 0.492 | 0.492 | 142.018 | 2.79817 | F | F | 9.67e+21 | 0 | 1 | d | |||||
Report | 3 | X134010.78-643327.4 | chandra | ccd2 | 194.5 | 680 | 3.94962 | 2 | 0.000790786 | 0.000400437 | 6.80714 | 0.999973 | 0.492 | 0.492 | 26.5651 | 4.42187 | F | F | 9.53e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 5 | X133935.81-643206.0 | chandra | ccd2 | 652.833 | 844.833 | 2.66123 | 2.93649 | 0.000532826 | 0.000587939 | 4.57222 | 0.999581 | 0.492 | 0.492 | 163.155 | 4.74763 | 0.830613 | 1.91531 | 0.39502 | 1.17468 | F | F | 9.67e+21 | 8.25536e-15 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X133857.79-642437.6 | chandra | ccd0 | 879.618 | 715.559 | 14.9467 | 5.33013 | 0.00299266 | 0.00106721 | 8.55388 | 1 | 3.74096 | 2.32589 | 91.0221 | 8.90418 | 8.15772 | 7.99958 | -0.00978738 | 0.338695 | A | F | 1.02e+22 | 5.13591e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X133935.90-642537.6 | chandra | ccd0 | 377.93 | 595.883 | 86.2175 | 9.81098 | 0.0172626 | 0.00196437 | 27.213 | 1 | 1.18197 | 0.783515 | 128.166 | 4.97512 | 30.9439 | 62.4948 | 0.337665 | 0.121394 | F | F | 1.02e+22 | 2.74463e-13 | 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