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 X113304.92+255355.2 chandra ccd7 641.544 494.411 380.471 20.1691 0.0104427 0.000553577 117.831 1 0.415525 0.415525 0 0.585991 F T 1.58e+20 0 1 ds
Report 2 X113302.75+255355.6 chandra ccd7 701.152 495.163 81.0401 9.76882 0.00222429 0.000268123 25.0979 1 0.400602 0.400602 0 0.429791 F F 1.58e+20 0 1 ds
Report 3 X113313.95+255230.0 chandra ccd7 393.893 321.182 178.23 13.5393 0.00489184 0.00037161 55.1974 1 0.694323 0.694323 0 3.0541 F F 1.58e+20 0 1 ds
Report 4 X113259.24+255430.1 chandra ccd7 797.441 565.283 9.94188 4.06141 0.000272873 0.000111473 3.07898 0.997427 0.344265 0.344265 0 0.886954 F F 1.58e+20 0 1 dbs
Report 5 X113313.03+255210.5 chandra ccd7 419.247 281.551 24.9681 6.01624 0.000685293 0.000165126 7.73257 1 0.790324 0.790324 0 3.1066 F F 1.58e+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