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 16 X175024.93-290214.8 chandra ccd2 1051.59 710.144 6701.33 111.835 3.87096 0.0646005 124.379 1 6.84381 2.56741 81.4232 8.88883 A T 9.26e+21 1.46467e-10 1 dscxf
Report 1 X175024.95-290210.9 chandra ccd2 1050.58 717.535 4310.46 77.0601 2.31806 0.041441 80.0033 1 0.492 0.492 101.834 8.96266 F F 9.26e+21 0 1 dc
Report srcpi bgdpi arf 1 X175123.08-290102.8 chandra ccd0 500.971 1040.97 15.5723 4.12313 0.00722989 0.00191427 25.8693 1 2.04702 1.07135 84.9611 9.40745 A F 8.37e+21 1.29787e-13 1 dx
Report srcpi bgdpi arf 1 X175025.90-291211.4 chandra ccd3 853.63 513.511 12.2893 4.22832 0.00570571 0.00196313 5.19811 0.999977 2.2422 0.640059 100.879 7.5322 F F 8.83e+21 9.66416e-14 1 dsx
Report 2 X175059.00-290830.0 chandra ccd1 989.214 1142.5 6.91929 2.64575 0.0032171 0.00123013 12.5124 1 0.492 0.492 180 0.863123 F F 8.44e+21 0 1 d
Report 1 X175109.31-291114.9 chandra ccd1 714.833 807.167 2.94537 1.73205 0.00136944 0.000805312 5.32622 0.999714 0.639127 0.492 45 4.30823 F F 8.17e+21 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