Source List

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 X204933.19-322857.0 chandra ccd5 954.5 369.405 39.4421 9.16553 0.00441589 0.00102616 23.5125 1 1.94254 1.51465 26.0436 12.7332 F F 5.45e+20 4.7409e-14 1 dx
Report srcpi bgdpi arf 8 X204940.83-323818.5 chandra ccd6 623.776 257.668 28.376 5.32691 0.00317695 0.000596396 33.5546 1 0.987631 0.987631 0 3.31905 F F 5.47e+20 3.42081e-14 1 dsx
Report srcpi bgdpi arf 7 X205002.97-323513.3 chandra ccd6 54.5 633.433 18.1445 4.69047 0.00203144 0.00052514 21.4558 1 1.237 0.991805 132.65 8.08325 F F 5.63e+20 3.03431e-14 1 dx
Report srcpi bgdpi arf 3 X204935.01-324012.0 chandra ccd7 667.966 1077 12.0303 3.46847 0.0013469 0.000388326 4.7073 0.999946 0.474179 0.474179 0 1.69775 F F 5.43e+20 1.02861e-14 1 dsx
Report srcpi bgdpi arf 1 X204935.32-330419.3 chandra ccd9 398.227 193.864 12.5313 4.47226 0.0014035 0.000500889 15.1322 1 2.88896 1.5274 73.3869 22.7236 A F 5.37e+20 2.40604e-14 1 dx
Report srcpi bgdpi arf 5 X204936.47-323637.4 chandra ccd6 735.755 463.183 11.7821 3.44469 0.00131911 0.000385665 13.9323 1 1.19034 1.19034 0 5.02136 F F 5.45e+20 1.46948e-14 1 dsx
Report srcpi bgdpi arf 1 X204953.45-324729.5 chandra ccd7 195.399 187.654 8.65741 4.66051 0.000969277 0.000521786 3.38753 0.998783 0.774041 0.774041 0 6.57845 F F 5.52e+20 8.69127e-15 1 dsx
Report srcpi bgdpi arf 2 X204956.37-324425.0 chandra ccd7 119.786 562.214 9.51701 3.16229 0.00106551 0.000354046 3.72388 0.999546 0.492 0.492 164.368 4.52483 F F 5.55e+20 9.47486e-15 1 dx
Report srcpi bgdpi arf 8 X204941.06-324305.4 chandra ccd7 512.278 724.167 8.75011 3 0.000979653 0.000335877 3.4238 0.998783 0.492 0.492 125.783 1.51197 F F 5.46e+20 7.34961e-15 1 dx
Report srcpi bgdpi arf 6 X204948.26-323520.6 chandra ccd6 432.214 618.786 6.32184 2.64577 0.000707787 0.000296217 7.47557 0.999999 1.07925 0.492 15.9585 6.53883 A F 5.53e+20 8.71111e-15 1 dx
Report srcpi bgdpi arf 4 X204929.51-324557.8 chandra ccd7 808.333 373.667 5.61167 2.4495 0.000628277 0.000274243 2.19577 0.983404 0.621544 0.492 67.0304 4.82651 F F 5.39e+20 4.94831e-15 1 dx
Report srcpi bgdpi arf 5 X204930.62-324506.9 chandra ccd7 780 477.167 5.54259 2.4495 0.000620542 0.000274243 2.16874 0.983404 0.760919 0.492 155.964 3.96422 A F 5.39e+20 4.82766e-15 1 dx
Report srcpi bgdpi arf 4 X204932.59-323325.4 chandra ccd6 835 853 5.12414 2.44951 0.000573693 0.000274245 6.05929 0.999899 1.2609 0.492 29.3049 8.31938 A F 5.44e+20 7.24429e-15 1 dx
Report srcpi bgdpi arf 3 X204929.61-323437.1 chandra ccd6 911.3 707.3 4.64312 2.23608 0.000519839 0.000250349 5.49048 0.999899 0.492 0.492 45 7.29884 F F 5.41e+20 6.25879e-15 1 dx
Report srcpi bgdpi arf 6 X204949.49-324327.8 chandra ccd7 296.1 678.5 4.51095 2.23608 0.000505041 0.000250349 1.76507 0.965073 0.528708 0.492 60.4819 2.80301 F F 5.51e+20 3.86661e-15 1 dx
Report srcpi bgdpi arf 1 X204952.17-323738.1 chandra ccd6 332 339.25 3.88348 2 0.000434791 0.000223918 4.59221 0.999136 0.492 0.492 26.5651 4.79362 F F 5.55e+20 5.01718e-15 1 dx
Report 2 X204951.05-323730.1 chandra ccd6 360.75 355.5 3.88271 2 0.000434704 0.000223918 4.5913 0.999136 0.492 0.492 180 4.78039 F F 5.54e+20 0 1 d
Report srcpi bgdpi arf 9 X204947.65-323844.1 chandra ccd6 448.167 205.167 2.91526 1.73205 0.00032639 0.000193919 3.4473 0.993806 0.492 0.492 45 3.35447 F F 5.51e+20 3.50468e-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