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 X090912.40+000221.9 chandra ccd7 914.792 897.979 19.8347 4.45362 0.0148416 0.00333249 16.8185 1 0.759306 0.759306 0 3.28294 F F 2.72e+20 0 1 ds
Report 2 X090924.01+000211.0 chandra ccd7 560.947 875.867 13.1248 3.98829 0.00982085 0.00298431 11.1289 1 0.318811 0.318811 0 0.55979 F F 2.71e+20 0 1 ds
Report 5 X090934.93+000210.0 chandra ccd7 227.5 873.333 5.95618 2.44949 0.00445668 0.00183282 5.05043 0.999898 0.492 0.492 25.8163 2.39673 F F 2.69e+20 0 1 d
Report 3 X090919.61+000259.3 chandra ccd7 694.7 973.5 4.97119 2.23607 0.00371967 0.00167313 4.21522 0.999401 0.492 0.492 119.518 1.52415 F F 2.71e+20 0 1 d
Report 4 X090931.74+000135.5 chandra ccd7 324.833 803.167 2.98687 1.73205 0.00223491 0.001296 2.53266 0.986105 0.492 0.492 16.845 1.85638 F F 2.69e+20 0 1 d
Report 1 X091008.55-000435.8 chandra ccd3 206.5 940.5 1.93699 1.41422 0.00144935 0.00105818 6.9334 0.999925 2.36275 0.492 51.3402 12.9463 A F 2.63e+20 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