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 1 X123049.05+122329.9 chandra ccd7 408.885 298.478 447.128 37.5938 0.0951459 0.00799972 13.7247 1 1.49 1.49 0 0.755212 T F 1.94e+20 0 1 dsc
Report 2 X123048.94+122331.1 chandra ccd7 412.114 300.754 340.184 47.7683 0.072389 0.0101648 10.442 1 1.01923 1.01923 0 0.749964 T T 1.94e+20 0 1 dsc
Report 3 X123048.63+122332.5 chandra ccd7 421.311 303.773 1036.6 44.1962 0.220581 0.00940461 31.8186 1 0.504716 0.504716 0 0.734916 F F 1.93e+20 0 1 ds
Report 4 X123048.24+122335.1 chandra ccd7 432.811 309 98.1916 27.5307 0.0208945 0.00585835 3.01401 0.998525 0.637954 0.637954 0 0.730297 F F 1.93e+20 0 1 ds
Report 5 X123047.47+122344.8 chandra ccd7 455.906 328.712 111.538 20.9486 0.0237345 0.0044577 3.42368 0.99961 1.5 1.5 0 0.837779 T F 1.93e+20 0 1 ds
Report 6 X123049.38+122328.5 chandra ccd7 399.053 295.645 7018.04 95.3007 1.49339 0.0202794 215.42 1 0.706682 0.706682 0 0.791871 T F 1.94e+20 0 1 ds

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