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 X143023.74+420436.6 chandra ccd7 635.874 596.307 2259.23 48.5997 0.213837 0.00459998 416.31 1 0.408227 0.408227 0 0.297954 F T 1.15e+20 1.909e-12 1 dsxf
Report srcpi bgdpi arf 2 X143030.98+420308.0 chandra ccd7 471.98 416.266 29.9725 6.01745 0.00283691 0.000569555 5.52306 0.999999 0.715475 0.393468 204.493 2.24341 F F 1.16e+20 2.08337e-14 1 dsx
Report srcpi bgdpi arf 3 X143020.89+420530.3 chandra ccd7 700.397 705.543 21.2095 5.23434 0.00200748 0.000495431 3.90829 0.999803 0.38786 0.38786 0 0.86861 F F 1.15e+20 1.47026e-14 1 dsx
Report srcpi bgdpi arf 4 X143037.36+420246.4 chandra ccd7 327.615 372.505 44.6157 6.87642 0.00422289 0.000650855 8.22137 1 0.870462 0.430405 3.237 3.3959 F F 1.16e+20 4.12553e-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