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 X025642.60-331521.2 chandra ccd7 707.104 546.868 30.7541 5.7253 0.0206668 0.00384742 36.4365 1 0.414979 0.414979 0 1.49347 F T 2.43e+20 1.12959e-13 1 dsx
Report srcpi bgdpi arf 4 X025647.86-331524.6 chandra ccd7 573.049 539.906 21.5753 4.73185 0.0144987 0.00317982 25.5617 1 0.46475 0.25516 23.0127 0.605144 F F 2.43e+20 7.78212e-14 1 dsx
Report 2 X025639.20-331503.1 chandra ccd7 793.778 583.518 21.4419 4.63157 0.0144091 0.00311244 25.4037 1 0.388047 0.388047 0 2.26767 F F 2.49e+20 0 1 ds
Report 3 X025652.29-331335.6 chandra ccd7 460.073 761.474 4.60469 2.14585 0.00309437 0.00144202 5.45549 0.999901 0.626294 0.626294 0 2.45153 F F 2.42e+20 0 1 ds
Report arf 1 X025641.18-332529.3 chandra ccd2 169.5 732.4 8.78298 3.1623 0.0036056 0.00129819 20.5135 1 2.24083 1.37138 59.9387 9.67685 A T 2.5e+20 4.1198e-14 1 dx
Report srcpi bgdpi arf 5 X025636.70-331700.9 chandra ccd7 856.875 343.625 7.48327 2.82844 0.003072 0.00116112 8.86594 1 0.492 0.492 176.942 2.8066 F F 2.49e+20 1.75446e-14 1 dx
Report arf 1 X025713.38-332100.8 chandra ccd6 532.625 651.75 7.37493 2.82844 0.00302762 0.00116115 14.0083 1 1.24086 1.12158 137.382 7.1587 F T 2.42e+20 2.95513e-14 1 dx
Report arf 3 X025714.04-331827.4 chandra ccd6 515.5 963.5 4.88988 2.23607 0.00200743 0.00091797 9.28805 1 0.492 0.492 90 5.77457 F F 2.42e+20 1.89272e-14 1 dx
Report arf 2 X025717.61-331709.5 chandra ccd6 424.25 1121.75 3.90105 2 0.00160149 0.000821057 7.40983 0.999989 0.800747 0.492 86.0464 6.07241 A F 2.41e+20 1.58829e-14 1 dx
Report 6 X025701.97-331741.0 chandra ccd6 822.833 1058.17 2.97423 1.73205 0.001221 0.000711056 5.64937 0.999803 0.492 0.492 90 3.19157 F F 2.42e+20 0 1 d
Report arf 4 X025646.16-332130.1 chandra ccd6 1225.83 592.5 2.95546 1.73205 0.0012133 0.000711056 5.61373 0.999803 0.492 0.492 118.155 5.58204 F F 2.49e+20 1.26036e-14 1 dx
Report arf 5 X025655.67-332107.6 chandra ccd6 983.5 638.167 2.9331 1.73205 0.00120412 0.000711057 5.57126 0.999803 0.492 0.492 151.845 5.34998 F F 2.44e+20 1.14025e-14 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