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 | X220451.29-181538.0 | chandra | ccd2 | 453.274 | 449.657 | 1208.28 | 35.907 | 0.237982 | 0.00707222 | 134.225 | 1 | 7.2771 | 6.2017 | 18.4477 | 12.1757 | F | F | 2.48e+20 | 0 | 1 | ds | |||||
Report | 8 | X220356.83-182258.6 | chandra | ccd7 | 670.874 | 360.865 | 148.35 | 12.4117 | 0.0292002 | 0.00244303 | 76.745 | 1 | 0.961938 | 0.961938 | 0 | 4.04021 | F | F | 2.54e+20 | 0 | 1 | ds | |||||
Report | 1 | X220410.52-180524.2 | chandra | ccd5 | 346.438 | 422.972 | 55.4084 | 11.5999 | 0.0109062 | 0.00228326 | 6.22802 | 1 | 9.72954 | 5.12466 | 24.9607 | 13.8284 | F | F | 2.56e+20 | 0 | 1 | ds | |||||
Report | 6 | X220403.34-182533.9 | chandra | ccd7 | 482.505 | 45.2408 | 16.7363 | 4.50053 | 0.00329426 | 0.000885853 | 8.65809 | 1 | 2.58892 | 0.84478 | 134.956 | 6.44445 | F | F | 2.52e+20 | 0 | 1 | ds | |||||
Report | 1 | X220355.84-182109.8 | chandra | ccd7 | 699.446 | 582.005 | 17.5078 | 4.18423 | 0.00344613 | 0.000823598 | 9.05721 | 1 | 0.391195 | 0.391195 | 0 | 2.5142 | F | F | 2.54e+20 | 0 | 1 | ds | |||||
Report | 2 | X220359.43-180656.7 | chandra | ccd5 | 667.278 | 234.5 | 17.4165 | 5.1963 | 0.00342814 | 0.0010228 | 1.95765 | 0.971471 | 4.60374 | 2.88105 | 41.7136 | 12.2058 | A | F | 2.57e+20 | 0 | 1 | d | |||||
Report | 2 | X220403.98-181917.9 | chandra | ccd7 | 463.949 | 809.388 | 13.8749 | 3.7249 | 0.00273104 | 0.000733184 | 7.17782 | 1 | 0.368451 | 0.368451 | 0 | 0.476838 | F | F | 2.54e+20 | 0 | 1 | ds | |||||
Report | 7 | X220354.13-182520.0 | chandra | ccd7 | 748.785 | 73.4337 | 12.2899 | 5.04892 | 0.00241906 | 0.000993796 | 6.35786 | 1 | 1.5 | 1.02225 | 327.814 | 6.4824 | F | F | 2.53e+20 | 0 | 1 | ds | |||||
Report | 4 | X220352.97-181350.5 | chandra | ccd6 | 815.845 | 418.762 | 25.3051 | 5.03042 | 0.00498089 | 0.000990155 | 46.7877 | 1 | 1.64745 | 1.64745 | 0 | 5.7104 | F | F | 2.57e+20 | 0 | 1 | ds | |||||
Report | 2 | X220404.01-181234.3 | chandra | ccd6 | 495.577 | 573.346 | 12.3298 | 3.60556 | 0.00242691 | 0.000709694 | 22.797 | 1 | 1.58043 | 1.0444 | 40.0207 | 6.57856 | A | F | 2.56e+20 | 0 | 1 | d | |||||
Report | 3 | X220405.61-181826.4 | chandra | ccd7 | 416.772 | 914.02 | 11.2452 | 3.35339 | 0.00221344 | 0.000660061 | 5.81741 | 0.999991 | 0.50677 | 0.50677 | 0 | 1.08412 | F | F | 2.54e+20 | 0 | 1 | ds | |||||
Report | 1 | X220434.01-182424.9 | chandra | ccd3 | 941.7 | 425.6 | 8.79213 | 3.1623 | 0.00173058 | 0.000622446 | 17.8312 | 1 | 2.15436 | 1.85102 | 115.023 | 9.23268 | F | F | 2.47e+20 | 0 | 1 | d | |||||
Report | 3 | X220358.27-181133.1 | chandra | ccd6 | 661.875 | 697.625 | 7.49429 | 2.82844 | 0.00147512 | 0.00055673 | 13.8565 | 1 | 1.73079 | 1.2832 | 131.74 | 7.63624 | F | F | 2.57e+20 | 0 | 1 | d | |||||
Report | 5 | X220415.00-181741.6 | chandra | ccd7 | 144.333 | 1004.67 | 5.91717 | 2.44949 | 0.0011647 | 0.000482141 | 3.0611 | 0.994819 | 0.536871 | 0.492 | 154.024 | 3.38577 | F | F | 2.53e+20 | 0 | 1 | d | |||||
Report | 1 | X220401.32-181535.0 | chandra | ccd6 | 573.5 | 206 | 1.95516 | 1.41422 | 0.00038484 | 0.000278365 | 3.61497 | 0.996645 | 0.492 | 0.492 | 90 | 3.55539 | F | F | 2.55e+20 | 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