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 X220418.35+044039.5 chandra ccd7 230.076 810.593 43.3102 7.16402 0.00118201 0.000195519 2.87907 0.997429 0.372735 0.372735 0 0.20313 F F 4.35e+20 0 1 ds
Report 2 X220417.27+044005.5 chandra ccd7 262.819 741.607 85.3855 13.7006 0.00233033 0.000373915 5.67606 1 1.5 0.842653 333.053 0.525159 T F 4.35e+20 0 1 ds
Report 4 X220417.65+044002.3 chandra ccd7 251.462 735.044 10347 106.478 0.282389 0.00290599 687.824 1 0.441808 0.38416 328.224 0.585563 F T 4.35e+20 0 1 ds
Report 6 X220416.21+043956.9 chandra ccd7 295.258 724.104 27.7398 5.75014 0.000757069 0.000156932 1.84402 0.967755 1.45003 1.45003 0 0.751465 T F 4.35e+20 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