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 X043334.05+242117.0 chandra ccd7 96.0866 303.724 420.453 20.9683 0.0302706 0.00150962 112.744 1 0.428203 0.428203 0 0.709075 F F 1.49e+21 0 1 ds
Report 3 X043334.71+242149.5 chandra ccd7 77.8524 369.845 14.2774 3.77854 0.00102791 0.000272037 3.82846 0.999731 0.410981 0.410981 0 1.25179 F F 1.49e+21 0 1 ds
Report 4 X043334.52+242347.9 chandra ccd7 82.9738 610.416 19.3035 4.39357 0.00138976 0.000316317 5.17621 0.999996 0.538244 0.538244 0 3.22281 F F 1.49e+21 0 1 ds
Report 5 X043333.74+242424.8 chandra ccd7 104.675 685.496 12.3332 3.51187 0.000887933 0.000252838 3.30713 0.998807 0.595307 0.595307 0 3.83959 F F 1.49e+21 0 1 ds
Report 6 X043334.55+242105.7 chandra ccd7 82.1084 280.813 862.901 30.2196 0.0621248 0.00217567 231.386 1 0.413256 0.413256 0 0.522608 F F 1.5e+21 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