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 X123049.18+122329.2 chandra ccd7 651.708 211.57 801.149 40.834 0.170203 0.00867515 25.7202 1 1.33018 1.33018 0 0.293261 T F 1.94e+20 1.14337e-12 1 dscbxf
Report srcpi bgdpi arf rmf 2 X123049.02+122330.4 chandra ccd7 656.71 213.929 259.619 33.3675 0.0551558 0.00708889 8.33485 1 1.5 0.31903 340.678 0.296771 A F 1.94e+20 4.101e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.5 chandra ccd7 668.135 218.363 868.035 39.7164 0.184413 0.00843771 27.8675 1 0.503325 0.503325 0 0.31853 F F 1.93e+20 1.37067e-12 1 dsx
Report srcpi bgdpi arf 4 X123048.25+122335.1 chandra ccd7 679.438 223.589 98.8783 23.6475 0.0210066 0.0050239 3.17441 0.999155 0.757114 0.757114 0 0.380063 T F 1.93e+20 1.56257e-13 1 dsx
Report srcpi bgdpi arf rmf 10 X123049.41+122328.3 chandra ccd7 645.089 209.806 3140.02 71.4246 0.667094 0.0151741 100.808 1 0.546888 0.546888 0 0.307767 F F 1.94e+20 4.96158e-12 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