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 X151150.03+075918.7 chandra ccd7 307.167 403.38 446.709 21.5209 0.0870778 0.0041951 110.178 1 0.617001 0.409556 105.35 2.10399 F T 2.38e+20 5.21311e-13 1 dsxf
Report srcpi bgdpi arf 2 X151143.06+075656.8 chandra ccd7 517.167 114.611 8.66853 3.00001 0.00168976 0.000584793 2.13803 0.982323 0.492 0.492 54.2175 1.48184 F F 2.39e+20 1.10248e-14 1 dx
Report srcpi bgdpi arf 1 X151133.80+075056.3 chandra ccd6 392.833 346.833 2.6813 1.73206 0.000522667 0.000337632 3.60912 0.997503 0.979688 0.802425 143.35 7.77283 F T 2.4e+20 5.69501e-15 1 dx
Report srcpi bgdpi arf 2 X151131.46+075343.9 chandra ccd6 463.5 687.5 1.93444 1.41422 0.00037708 0.000275674 2.60381 0.981366 0.492 0.492 90 5.40531 F F 2.39e+20 3.82115e-15 1 dx

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