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 X020429.44-291748.5 chandra ccd7 554.228 889.67 150.594 12.5943 0.0515288 0.00430939 75.1949 1 0.399087 0.399087 0 0.583919 F F 1.39e+20 0 1 ds
Report 7 X020444.95-291926.0 chandra ccd7 141.849 691.489 25.3691 5.03677 0.00868058 0.00172344 12.6674 1 1.2095 0.50007 341.408 3.61647 F F 1.39e+20 0 1 ds
Report 2 X020432.68-291324.1 chandra ccd6 1061.97 558.216 10.9991 3.31649 0.00376357 0.0011348 26.1945 1 1.0615 0.387368 27.4265 3.98788 F F 1.37e+20 0 1 ds
Report 1 X020431.87-291030.0 chandra ccd6 1083.17 911.5 5.71647 2.4495 0.00195601 0.000838146 13.6139 1 1.45382 0.854778 129.96 6.87709 A F 1.36e+20 0 1 d
Report 1 X020503.65-292140.1 chandra ccd2 1259.75 446 3.80509 2.00001 0.00130199 0.000684344 9.30618 0.999972 0.788935 0.504101 110.157 8.26667 A F 1.39e+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