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 rmf 1 X113910.25-135040.5 chandra ccd7 138.005 752.227 145.416 12.1073 0.0163275 0.00135942 24.152 1 1.3593 1.3593 0 0.588064 T F 3.31e+20 1.02895e-13 1 dpsxf
Report srcpi bgdpi arf rmf 2 X113910.70-135043.7 chandra ccd7 124.778 745.698 3436.6 60.1076 0.385865 0.00674895 570.78 1 0.390108 0.390108 0 0.587807 F F 3.31e+20 2.26945e-12 1 dsx
Report srcpi bgdpi arf 3 X113910.94-134943.1 chandra ccd7 117.609 868.784 25.3835 5.0382 0.0028501 0.000565697 4.21591 0.999937 0.367691 0.367691 0 0.471971 F F 3.31e+20 1.68501e-14 1 dsx
Report srcpi bgdpi arf 4 X113907.26-135519.4 chandra ccd7 226.581 185.335 32.504 5.70123 0.00364959 0.000640141 5.39855 0.999999 1.72284 0.948532 313.601 5.25576 F F 3.32e+20 2.27211e-14 1 dsx
Report srcpi bgdpi arf 6 X113909.31-135050.6 chandra ccd7 165.988 731.542 52.0497 7.47087 0.00584421 0.000838839 8.64487 1 0.387849 0.387849 0 0.854991 F F 3.31e+20 3.45404e-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