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 X053529.18-691558.4 chandra ccd7 745.14 454.184 39.6101 10.9058 0.00153995 0.000423993 3.05957 0.99857 1.35131 1.35131 0 0.464036 T F 2.65e+21 1.28701e-14 1 dsx
Report srcpi bgdpi arf rmf 2 X053527.98-691610.9 chandra ccd7 758.036 428.689 27463.2 167.816 1.06771 0.0065243 2121.32 1 0.669487 0.669487 0 0.291989 T F 2.65e+21 4.48792e-12 1 dsxf
Report srcpi bgdpi arf rmf 3 X053526.49-691627.3 chandra ccd7 774.2 395.454 118.666 10.938 0.00461347 0.000425244 9.16602 1 2.16579 2.16579 0 0.288525 T F 2.65e+21 3.86293e-14 1 dsx
Report srcpi bgdpi arf 4 X053524.78-691626.9 chandra ccd7 792.551 396.254 32.0811 7.33085 0.00124724 0.000285007 2.47801 0.991881 0.35988 0.35988 0 0.24044 F F 2.64e+21 1.04586e-14 1 dsx
Report srcpi bgdpi arf 6 X053529.55-691554.2 chandra ccd7 741.103 462.699 31.246 8.26106 0.00121477 0.00032117 2.41351 0.990113 1.5 0.595316 62.87 0.537899 A F 2.65e+21 1.06418e-14 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