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 X123049.02+122330.0 chandra ccd7 525.715 226.761 255.603 34.3749 0.0545673 0.0073385 8.7672 1 1.07949 1.07949 0 0.290954 T F 1.94e+20 3.56403e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.97+122330.6 chandra ccd7 527.294 227.849 300.633 38.2603 0.0641807 0.00816801 10.3117 1 1.1277 1.1277 0 0.30604 T F 1.94e+20 4.74654e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.64+122332.5 chandra ccd7 536.989 231.722 862.297 39.9086 0.184087 0.00851989 29.5769 1 0.497454 0.497454 0 0.337922 F F 1.93e+20 1.36115e-12 1 dsx
Report srcpi bgdpi arf 4 X123048.21+122335.2 chandra ccd7 549.89 237.326 74.2539 22.5713 0.0158521 0.00481863 2.54691 0.994224 0.631577 0.631577 0 0.410677 F F 1.93e+20 1.17211e-13 1 dsx
Report srcpi bgdpi arf rmf 7 X123049.40+122328.3 chandra ccd7 514.259 223.275 3512.22 67.1362 0.749806 0.0143326 120.469 1 0.826056 0.41525 338.015 0.285154 A F 1.94e+20 5.54723e-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