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 2 X174856.30-313045.6 chandra ccd3 665.9 133.5 4.83061 3.39792 0.00248253 0.00174625 11.7372 1 0.492 0.492 150.482 3.05155 -0.0846933 4.91531 1 0.992474 F F 6.32e+21 3.4112e-14 1 dx
Report srcpi bgdpi arf 1 X174905.56-312419.3 chandra ccd3 424.3 918.5 4.8352 3.39792 0.00248489 0.00174625 11.9107 1 1.19911 1.16688 2.35064e-08 8.20622 2.8352 2 -0.172733 0.723977 F F 6.41e+21 3.79624e-14 1 dx
Report 1 X174850.91-313128.8 chandra ccd2 693 1078.75 3.97793 2 0.00204433 0.00102783 11.5416 1 0.507001 0.492 143.909 2.01842 F F 6.35e+21 0 1 d
Report 2 X174848.81-313435.2 chandra ccd2 747.5 699.75 3.96962 2 0.00204006 0.00102783 11.5175 1 0.492 0.492 28.9973 4.05264 F F 6.27e+21 0 1 d
Report 3 X174903.61-313018.8 chandra ccd3 475.833 187.833 2.98319 1.73205 0.00153311 0.000890131 8.45061 0.999991 0.492 0.492 45 4.6358 F F 6.26e+21 0 1 d
Report 1 X174759.88-312914.2 chandra ccd1 1128.5 161.5 0.947473 1.00001 0.000486923 0.00051392 2.71135 0.993124 0.492 0.492 90 9.10983 F F 6.93e+21 0 1 d
Report srcpi bgdpi arf 2 X174813.72-313001.1 chandra ccd1 768.667 66.5 5.93454 3.59808 0.00304986 0.00184911 23.1952 1 1.27293 0.492 174.594 6.07495 4.96727 0.96727 -0.67402 0.740845 A F 6.77e+21 7.73787e-14 1 dx

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