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 1 X074416.36+375645.2 chandra ccd7 99.5843 720.031 37.1719 6.99871 0.00107945 0.000203238 3.95457 0.999905 1.10483 1.10483 0 4.03728 F F 5.08e+20 7.31867e-15 1 dsx
Report srcpi bgdpi arf rmf 2 X074414.90+375645.7 chandra ccd7 134.671 720.956 139.539 13.1066 0.00405211 0.000380607 14.845 1 0.899234 0.899234 0 4.068 F T 5.08e+20 1.7827e-14 1 dsxf
Report srcpi bgdpi arf rmf 3 X074414.95+375656.6 chandra ccd7 133.65 743.165 518.267 23.5009 0.0150501 0.000682449 55.1363 1 1.27562 0.62965 323.033 4.24821 A T 5.08e+20 1.17682e-13 1 dsx
Report srcpi bgdpi arf 4 X074418.84+375723.1 chandra ccd7 40.0973 796.985 64.6983 9.10058 0.0018788 0.000264275 6.88299 1 1.20157 1.20157 0 4.68399 F T 5.07e+20 1.63589e-14 1 dsx
Report srcpi bgdpi arf rmf 5 X074417.47+375317.2 chandra ccd7 73.0145 297.107 1911.81 47.5119 0.0555178 0.00137972 203.39 1 0.409215 0.409215 0 0.578688 F T 5.11e+20 3.63588e-13 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