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 X123049.16+122328.7 chandra ccd7 118.886 741.666 501.232 49.2403 0.106576 0.0104699 15.8886 1 1.5 1.5 0 0.75399 T F 1.94e+20 8.19057e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.63+122332.2 chandra ccd7 134.699 748.801 1130.87 43.858 0.240456 0.00932551 35.8476 1 0.519059 0.519059 0 0.745881 F F 1.93e+20 1.64202e-12 1 dsx
Report srcpi bgdpi arf 3 X123048.24+122334.9 chandra ccd7 146.372 754.255 78.6367 26.2438 0.0167204 0.00558018 2.49272 0.992978 0.595122 0.595122 0 0.746137 F F 1.93e+20 1.14141e-13 1 dsx
Report srcpi bgdpi arf rmf 6 X123048.90+122342.7 chandra ccd7 126.53 770.135 123.672 23.1507 0.0262963 0.00492251 3.9203 0.999938 1.5 1.5 0 0.568197 T F 1.93e+20 1.78833e-13 1 dsx
Report srcpi bgdpi arf rmf 7 X123049.38+122328.2 chandra ccd7 112.447 740.663 8411.07 98.2272 1.78843 0.0208859 266.624 1 0.546619 0.434288 333.703 0.76625 F F 1.94e+20 1.21975e-11 1 dscx

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