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 2 X194938.38+263149.0 chandra ccd7 376.747 510.484 112.546 10.6541 0.0653627 0.00618752 114.647 1 0.409128 0.409128 0 0.597102 F F 1.02e+22 1.77024e-12 1 dsxf
Report srcpi bgdpi arf 1 X194910.17+262506.9 chandra ccd3 638.433 979.1 13.9639 3.873 0.00810952 0.00224924 37.1596 1 2.97829 1.58673 123.356 9.67393 A F 1.03e+22 1.38226e-13 1 dx
Report srcpi bgdpi arf 2 X194923.11+262504.0 chandra ccd3 285.136 972.773 10.5882 3.31663 0.0061491 0.00192613 28.1765 1 1.41153 0.815802 25.875 7.91568 A F 1.03e+22 1.01291e-13 1 dx
Report 1 X195008.42+263040.4 chandra ccd6 585.75 656.75 3.93921 2 0.00228769 0.0011615 9.7954 0.999999 1.34746 0.588133 165.827 6.24688 A F 1.02e+22 0 1 d
Report 2 X195017.61+262647.5 chandra ccd6 334.5 183.75 3.86473 2 0.00224444 0.0011615 9.6102 0.999999 0.492 0.492 90 9.64312 F F 1.02e+22 0 1 d

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