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 X123048.98+122330.5 chandra ccd7 472.882 283.561 266.579 44.6492 0.0518434 0.00868322 7.21669 1 1.5 0.330025 340.673 0.769151 A F 1.94e+20 3.10776e-13 1 dpscxf
Report srcpi bgdpi arf rmf 2 X123048.70+122333.2 chandra ccd7 481.445 288.973 1148.49 57.2316 0.223354 0.0111302 31.0913 1 2.34408 2.34408 0 0.736651 T F 1.94e+20 1.56887e-12 1 dcsx
Report 3 X123048.62+122332.6 chandra ccd7 483.666 287.819 1111.78 45.1228 0.216215 0.00877532 30.0976 1 0.655428 0.480507 341.175 0.723096 T F 1.93e+20 0 1 dsc
Report srcpi bgdpi arf 4 X123048.23+122335.3 chandra ccd7 495.198 293.221 89.3148 28.073 0.0173696 0.00545955 2.41789 0.991534 0.650351 0.650351 0 0.708437 F F 1.93e+20 1.21947e-13 1 dsx
Report srcpi bgdpi arf rmf 8 X123049.37+122328.6 chandra ccd7 461.24 279.665 7645.58 99.524 1.48689 0.0193551 206.977 1 0.891179 0.635255 330.725 0.79942 T F 1.94e+20 1.04488e-11 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