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 X133038.13+250938.5 chandra ccd7 168.232 775.413 58.0313 8.11683 0.00160247 0.000224137 8.70982 1 0.395405 0.395405 0 0.238024 F F 1.03e+20 9.99684e-15 1 dsx
Report srcpi bgdpi arf rmf 2 X133037.69+250911.0 chandra ccd7 180.434 719.541 4041.31 64.8009 0.111596 0.0017894 606.554 1 0.407815 0.407815 0 0.59534 F F 1.03e+20 6.90809e-13 1 dsxf
Report srcpi bgdpi arf 4 X133031.80+250603.0 chandra ccd7 342.994 337.526 23.74 5.62643 0.000655553 0.000155368 3.5631 0.999626 1.19355 1.19355 0 3.98632 F F 1.05e+20 4.24024e-15 1 dsx
Report srcpi bgdpi arf 7 X133035.38+250849.0 chandra ccd7 244.141 674.817 51.2755 7.4316 0.00141592 0.000205215 7.69586 1 0.500386 0.343268 115.267 1.21377 F F 1.04e+20 1.32929e-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