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 | 2 | X085201.39-461753.3 | chandra | ccd2 | 56.3374 | 251.632 | 454.506 | 21.7541 | 0.151746 | 0.00726304 | 105.003 | 1 | 0.642982 | 0.47701 | 58.9779 | 2.3505 | F | T | 8.57e+21 | 1.27436e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X085226.31-462232.7 | chandra | ccd1 | 569.7 | 728.9 | 4.88531 | 2.23607 | 0.00163105 | 0.000746555 | 6.23765 | 0.999956 | 0.600211 | 0.492 | 66.1987 | 5.00527 | F | F | 8.46e+21 | 2.33375e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X085149.72-462039.6 | chandra | ccd3 | 296.5 | 951.1 | 4.85602 | 2.23607 | 0.00162128 | 0.000746555 | 5.52246 | 0.999846 | 0.492 | 0.492 | 34.0993 | 1.92142 | F | F | 8.46e+21 | 2.25086e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X085120.51-462407.5 | chandra | ccd3 | 910.5 | 527.7 | 4.68684 | 2.23608 | 0.00156479 | 0.000746556 | 5.33006 | 0.999846 | 0.5904 | 0.492 | 90 | 7.93206 | F | T | 8.25e+21 | 2.47601e-14 | 1 | dx | ||||
| Report | 2 | X085212.52-462220.6 | chandra | ccd1 | 859.75 | 753.75 | 3.86461 | 2 | 0.00129027 | 0.000667739 | 4.9344 | 0.999564 | 0.492 | 0.492 | 71.565 | 2.94863 | F | T | 8.45e+21 | 0 | 1 | d | |||||
| Report | 3 | X085207.92-462220.6 | chandra | ccd1 | 956.5 | 753.833 | 2.90035 | 1.73205 | 0.000968336 | 0.000578279 | 3.70322 | 0.99637 | 0.492 | 0.492 | 28.155 | 2.46007 | F | F | 8.44e+21 | 0 | 1 | d | |||||
| Report | 1 | X085159.65-462810.9 | chandra | ccd3 | 87.5 | 33.8333 | 2.74985 | 1.73206 | 0.000918088 | 0.000578282 | 3.12724 | 0.99191 | 0.621484 | 0.492 | 14.3052 | 7.94878 | F | F | 8.23e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X085242.85-462333.5 | chandra | ccd1 | 222.1 | 604.7 | 4.66109 | 2.23608 | 0.00155619 | 0.000746557 | 5.95137 | 0.999956 | 0.761252 | 0.492 | 100.462 | 8.01431 | A | F | 8.45e+21 | 2.38352e-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