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 X111816.96+074558.3 chandra ccd7 186.153 797.994 465.831 24.6247 0.0319466 0.00168876 75.4977 1 0.441349 0.392875 53.5739 0.291076 F F 3.57e+20 2.79433e-13 1 dsxf
Report srcpi bgdpi arf 8 X111816.16+074315.6 chandra ccd7 210.305 467.229 86.7415 9.77235 0.00594871 0.000670185 14.0583 1 0.802118 0.344114 312.148 2.99723 A F 3.6e+20 4.5258e-14 1 dsx
Report srcpi bgdpi arf 5 X111812.00+074032.6 chandra ccd7 335.997 135.965 36.1256 6.01046 0.00247749 0.000412196 5.85491 1 1.5 0.859315 90 5.84503 F F 3.66e+20 1.96874e-14 1 dsx
Report srcpi bgdpi arf 1 X111848.51+073909.4 chandra ccd3 706.4 343.6 7.56303 3.16233 0.00051867 0.000216872 7.65517 0.999999 1.99964 1.04458 158.468 10.6203 A F 3.75e+20 7.11231e-15 1 dx
Report srcpi bgdpi arf 2 X111837.69+073913.3 chandra ccd3 1033.25 351.417 9.51539 3.46418 0.000652563 0.000237572 9.63132 1 2.38192 1.22916 12.7121 8.75866 A F 3.73e+20 9.03045e-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