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 | X024619.81-301602.9 | chandra | ccd7 | 118.495 | 353.98 | 144.293 | 12.4263 | 0.0251245 | 0.00216368 | 24.0598 | 1 | 0.389972 | 0.389972 | 0 | 1.00119 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 2 | X024619.64-301626.0 | chandra | ccd7 | 122.526 | 306.474 | 59.1045 | 8.8319 | 0.0102913 | 0.00153781 | 9.85524 | 1 | 1.2824 | 0.922804 | 133.865 | 0.613756 | T | T | 2.03e+20 | 0 | 1 | db | |||||
| Report | 3 | X024618.97-301629.0 | chandra | ccd7 | 140.679 | 300.856 | 1796.66 | 44.8265 | 0.312836 | 0.00780522 | 299.58 | 1 | 0.396173 | 0.396173 | 0 | 0.566742 | F | T | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 4 | X024619.33-301638.6 | chandra | ccd7 | 131.2 | 281.341 | 18.4032 | 10.3562 | 0.00320439 | 0.00180324 | 3.0686 | 0.998107 | 0.372145 | 0.372145 | 0 | 0.400924 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 6 | X024618.28-301655.6 | chandra | ccd7 | 158.893 | 246.867 | 38.7144 | 6.44802 | 0.00674098 | 0.00112273 | 6.45534 | 1 | 0.346374 | 0.346374 | 0 | 0.261291 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 7 | X024617.57-301705.1 | chandra | ccd7 | 177.361 | 227.493 | 20.2933 | 4.76361 | 0.00353349 | 0.000829443 | 3.38376 | 0.999271 | 0.534102 | 0.258564 | 163.045 | 0.384381 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 8 | X024617.90-301603.9 | chandra | ccd7 | 168.433 | 351.433 | 12.7439 | 3.87302 | 0.00221898 | 0.000674371 | 2.12496 | 0.977767 | 0.68838 | 0.492 | 138.871 | 1.02881 | T | F | 2.02e+20 | 0 | 1 | db | |||||
| Report | 9 | X024617.38-301604.5 | chandra | ccd7 | 182.39 | 350.707 | 12.3772 | 3.51812 | 0.00215513 | 0.000612579 | 2.06381 | 0.977767 | 0.607781 | 0.607781 | 0 | 1.05871 | F | F | 2.02e+20 | 0 | 1 | ds | |||||
| Report | 11 | X024615.38-301427.7 | chandra | ccd7 | 235.138 | 547.395 | 15.6819 | 3.96004 | 0.00273055 | 0.000689526 | 2.61484 | 0.992994 | 0.545731 | 0.545731 | 0 | 2.72078 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 12 | X024617.06-301331.2 | chandra | ccd7 | 190.938 | 662.137 | 10.9639 | 3.31118 | 0.00190904 | 0.000576544 | 1.82815 | 0.956017 | 0.787219 | 0.787219 | 0 | 3.55741 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
| Report | 15 | X024621.76-301746.9 | chandra | ccd7 | 67.157 | 142.424 | 15.9768 | 4.76399 | 0.00278189 | 0.000829507 | 2.66401 | 0.992994 | 0.397091 | 0.397091 | 0 | 0.902922 | F | F | 2.03e+20 | 0 | 1 | ds |
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