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 X041833.86+573223.1 chandra ccd7 142.094 785.817 227.847 16.3748 0.00326223 0.000234448 49.3077 1 0.303008 0.303008 0 0.290898 F F 4.22e+21 1.60978e-14 1 dsxf
Report srcpi bgdpi arf 3 X041826.50+573053.7 chandra ccd7 262.649 603.994 11.7414 6.36091 0.000168109 9.10733e-05 2.54092 0.993019 0.4561 0.4561 0 2.00449 F F 4.21e+21 1.83088e-15 1 dsx
Report srcpi bgdpi arf 4 X041828.52+573113.6 chandra ccd7 229.614 644.488 10.9198 5.9289 0.000156345 8.48876e-05 2.36312 0.988448 0.40154 0.40154 0 1.59013 F F 4.21e+21 1.45626e-15 1 dsx
Report srcpi bgdpi arf 5 X041838.16+573241.4 chandra ccd7 71.83 822.878 13.9899 4.57398 0.000200303 6.54887e-05 3.02751 0.99764 0.486859 0.486859 0 0.635861 F F 4.22e+21 3.25232e-15 1 dsx
Report srcpi bgdpi arf 6 X041822.87+572842.6 chandra ccd7 322.294 337.624 13.0834 6.18035 0.000187324 8.84881e-05 2.83134 0.995889 0.660484 0.660484 0 4.20538 F F 4.19e+21 1.80081e-15 1 dsx
Report srcpi bgdpi arf 7 X041824.40+572731.9 chandra ccd7 297.336 193.947 27.4013 6.76336 0.000392322 9.68354e-05 5.92983 1 0.827505 0.827505 0 5.28533 F F 4.18e+21 5.52157e-15 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