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 X043334.06+242117.0 chandra ccd7 99.5866 309.708 926.307 31.4704 0.0658266 0.00223639 190.891 1 0.406582 0.406582 0 0.708668 F F 1.49e+21 0 1 ds
Report 2 X043334.72+242149.7 chandra ccd7 81.1484 376.266 21.376 5.41769 0.00151906 0.000385 4.40512 0.999946 0.390568 0.390568 0 1.25663 F F 1.49e+21 0 1 ds
Report 3 X043334.51+242348.1 chandra ccd7 86.9777 616.877 20.0993 4.48322 0.00142832 0.000318593 4.14202 0.999894 0.503486 0.503486 0 3.22633 F F 1.49e+21 0 1 ds
Report 5 X043333.70+242425.1 chandra ccd7 109.569 692.131 9.61881 4.01066 0.000683546 0.000285011 1.98222 0.974986 0.821038 0.821038 0 3.84307 F F 1.49e+21 0 1 ds
Report 6 X043334.56+242105.8 chandra ccd7 85.4986 286.902 624.753 25.7676 0.0443971 0.00183114 128.748 1 0.431845 0.386834 310.442 0.524145 F T 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