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 | 4 | X010950.91-125322.4 | chandra | ccd3 | 478.847 | 1142.16 | 191.435 | 14.0733 | 0.202653 | 0.014898 | 74.3938 | 1 | 0.468356 | 0.468356 | 0 | 0.764433 | F | F | 1.86e+20 | 2.53123e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X011011.67-124458.9 | chandra | ccd0 | 362.864 | 847.773 | 9.9388 | 3.31665 | 0.0104857 | 0.00349915 | 45.8939 | 1 | 2.99019 | 2.08854 | 45.7463 | 9.04225 | F | F | 1.89e+20 | 1.38778e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X010940.74-130121.0 | chandra | ccd3 | 780.357 | 168.786 | 6.74547 | 2.64576 | 0.00714075 | 0.0028008 | 2.62136 | 0.991745 | 2.31512 | 0.993469 | 51.762 | 9.11263 | A | F | 1.83e+20 | 1.00894e-13 | 1 | dx | ||||
| Report | 3 | X010927.26-125539.9 | chandra | ccd3 | 1180.9 | 861.9 | 4.88928 | 2.23607 | 0.00517579 | 0.0023671 | 1.90003 | 0.961938 | 1.32912 | 0.509428 | 124.407 | 6.76562 | A | F | 1.83e+20 | 0 | 1 | d | |||||
| Report | 2 | X011002.83-124858.2 | chandra | ccd0 | 625.833 | 361.5 | 2.98713 | 1.73205 | 0.0031515 | 0.00182736 | 13.7935 | 1 | 0.678423 | 0.492 | 118.155 | 4.52449 | F | F | 1.88e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X010858.30-124953.8 | chandra | ccd6 | 267.167 | 1055.83 | 2.38347 | 1.7321 | 0.00251463 | 0.00182741 | 10.4797 | 0.999978 | 4.15772 | 2.33824 | 163.826 | 13.4186 | A | F | 1.84e+20 | 4.30001e-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