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 | 1 | X120800.86-273112.4 | chandra | ccd3 | 940.351 | 762.677 | 16.6095 | 4.07548 | 0.008536 | 0.00209448 | 42.8168 | 1 | 0.886857 | 0.886857 | 0 | 4.43695 | F | F | 7.19e+20 | 1.00287e-13 | 1 | dsx | ||||
Report | 1 | X120731.21-272628.0 | chandra | ccd1 | 744 | 1016 | 3.91167 | 2 | 0.00201028 | 0.00102784 | 10.6336 | 1 | 0.492 | 0.492 | 45 | 9.62655 | F | F | 7.27e+20 | 0 | 1 | d | |||||
Report | 3 | X120752.52-273413.1 | chandra | ccd3 | 1165.5 | 394.833 | 2.97724 | 1.73205 | 0.00153005 | 0.000890131 | 7.67486 | 0.999981 | 0.492 | 0.492 | 90 | 0.900495 | F | F | 7.21e+20 | 0 | 1 | d | |||||
Report | 1 | X120805.07-273634.0 | chandra | ccd2 | 495.5 | 1076.5 | 1.98977 | 1.41421 | 0.00102258 | 0.000726789 | 5.03222 | 0.999433 | 0.492 | 0.492 | 90 | 3.48588 | F | F | 7.19e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X120814.21-273642.3 | chandra | ccd3 | 579.5 | 91.5 | 0.992915 | 1 | 0.000510276 | 0.000513917 | 2.55958 | 0.989752 | 0.492 | 0.492 | 90 | 5.4224 | F | F | 7.18e+20 | 1.02665e-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