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 | X161801.67-510414.2 | chandra | ccd3 | 436.041 | 193.271 | 161.089 | 22.1285 | 0.0313526 | 0.00430685 | 7.2555 | 1 | 4.2624 | 4.2624 | 0 | 8.01619 | F | F | 2.05e+22 | 0 | 1 | ds | |||||
Report | 2 | X161747.50-510347.7 | chandra | ccd3 | 707.362 | 247.793 | 105.865 | 23.6788 | 0.0206043 | 0.00460855 | 4.76819 | 0.999998 | 6.02496 | 2.99269 | 346.391 | 6.75496 | T | F | 2.06e+22 | 0 | 1 | ds | |||||
Report | 3 | X161807.16-510324.8 | chandra | ccd3 | 330.673 | 293.491 | 122.497 | 15.9526 | 0.0238413 | 0.00310481 | 5.5173 | 1 | 5.64679 | 4.08393 | 84.3628 | 9.19659 | T | F | 2.04e+22 | 0 | 1 | ds | |||||
Report | 6 | X161804.21-510403.9 | chandra | ccd3 | 386.77 | 213.554 | 79.5522 | 12.2478 | 0.015483 | 0.00238376 | 3.58305 | 0.999767 | 1.3179 | 1.22717 | 5.94052 | 8.45473 | F | F | 2.04e+22 | 0 | 1 | d | |||||
Report | 7 | X161759.29-510351.2 | chandra | ccd3 | 481.587 | 240.261 | 141.531 | 21.5186 | 0.0275459 | 0.00418813 | 6.3746 | 1 | 5.63368 | 5.63368 | 0 | 7.98117 | T | F | 2.05e+22 | 0 | 1 | ds | |||||
Report | 11 | X161742.32-510331.0 | chandra | ccd3 | 806.701 | 281.841 | 120.175 | 23.4292 | 0.0233895 | 0.00456 | 5.41272 | 1 | 4.9423 | 4.9423 | 0 | 6.47837 | T | F | 2.06e+22 | 0 | 1 | ds | |||||
Report | 13 | X161745.02-510320.6 | chandra | ccd3 | 754.951 | 302.853 | 127.492 | 35.8087 | 0.0248136 | 0.00696939 | 5.74228 | 1 | 5.82965 | 5.82965 | 0 | 6.79873 | F | F | 2.06e+22 | 0 | 1 | ds | |||||
Report | 15 | X161748.39-510300.6 | chandra | ccd3 | 690.186 | 343.378 | 55.7709 | 26.1906 | 0.0108546 | 0.00509743 | 2.51194 | 0.993144 | 3.36608 | 3.36608 | 0 | 7.44407 | F | F | 2.06e+22 | 0 | 1 | ds | |||||
Report | 16 | X161736.24-510224.6 | chandra | ccd3 | 922.457 | 416.273 | 1778.57 | 44.9559 | 0.346158 | 0.00874965 | 80.1073 | 1 | 1.9644 | 1.5069 | 51.7912 | 7.06065 | F | T | 2.07e+22 | 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