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 X123049.01+122330.4 chandra ccd7 737.709 184.96 273.327 35.5255 0.0581618 0.00755953 8.7748 1 1.5 0.376286 339.542 0.298355 A F 1.94e+20 3.03707e-13 1 dbscxf
Report srcpi bgdpi arf rmf 2 X123048.96+122330.9 chandra ccd7 739.29 185.884 342.466 37.7086 0.072874 0.00802408 10.9944 1 1.5 1.5 0 0.295459 T F 1.94e+20 5.41962e-13 1 dbscx
Report srcpi bgdpi arf rmf 3 X123048.64+122332.6 chandra ccd7 748.799 189.445 893.012 40.4577 0.190026 0.00860909 28.669 1 0.517705 0.517705 0 0.307342 F F 1.93e+20 1.41379e-12 1 dsx
Report srcpi bgdpi arf 4 X123048.26+122335.2 chandra ccd7 760.17 194.739 98.4358 25.5004 0.0209464 0.00542629 3.16015 0.999058 0.765957 0.765957 0 0.351294 F F 1.93e+20 1.55881e-13 1 dsx
Report srcpi bgdpi arf rmf 9 X123049.43+122328.4 chandra ccd7 725.393 180.771 4800.69 79.2979 1.02155 0.016874 154.12 1 0.574383 0.410318 334.469 0.331444 F F 1.94e+20 7.59386e-12 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