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 X123049.17+122329.0 chandra ccd7 241.9 632.379 898.847 47.564 0.169996 0.00899561 26.9651 1 1.5 0.563204 -0 0.744054 A F 1.94e+20 9.57828e-13 1 dscbxf
Report srcpi bgdpi arf rmf 2 X123049.03+122330.2 chandra ccd7 245.887 634.656 441.399 36.9923 0.0834801 0.00699621 13.2418 1 1.5 0.37414 341.433 0.760032 A F 1.94e+20 5.48126e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.5 chandra ccd7 257.842 639.367 1327.04 48.9363 0.250979 0.00925517 39.8107 1 0.483749 0.483749 0 0.787935 F F 1.93e+20 1.6481e-12 1 dsx
Report srcpi bgdpi arf rmf 4 X123048.24+122335.1 chandra ccd7 269.395 644.719 109.358 29.4639 0.0206825 0.0055724 3.2807 0.99939 0.687559 0.687559 0 0.835947 F F 1.93e+20 1.35848e-13 1 dsx
Report srcpi bgdpi arf rmf 9 X123049.39+122328.4 chandra ccd7 235.244 631.015 5975.45 86.1054 1.13011 0.0162848 179.261 1 0.911984 0.414884 338.779 0.714953 A F 1.94e+20 7.41909e-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