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 5 X174446.01-274732.7 chandra ccd7 104.299 373.566 213.936 14.7614 0.0437704 0.00302011 107.487 1 1.74474 1.1576 354.185 5.44707 F F 9.33e+21 2.38078e-13 1 dsxf
Report srcpi bgdpi arf 1 X174442.29-273412.7 chandra ccd6 167.947 951.796 44.4805 7.64215 0.00910053 0.00156355 11.9212 1 5.57544 5.57544 0 9.85412 F F 8.73e+21 1.4857e-13 1 dsx
Report srcpi bgdpi arf 1 X174439.69-274559.7 chandra ccd7 274.25 562.333 11.6968 3.46411 0.00239311 0.000708738 5.87677 0.999996 0.600271 0.492 15.3112 3.35964 F F 9.18e+21 3.05296e-14 1 dbx
Report 2 X174435.40-274453.1 chandra ccd7 389.944 697.611 8.84364 3 0.00180936 0.000613784 4.44326 0.99975 0.492 0.492 80.1266 1.90717 F F 9.08e+21 0 1 d
Report srcpi bgdpi arf 1 X174523.04-273607.8 chandra ccd2 433.5 870.1 7.46612 3.16233 0.00152753 0.000646996 11.2747 1 3.55256 2.38429 123.661 14.1154 F F 9.37e+21 2.8277e-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