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 | 9 | X113151.58-123158.7 | chandra | ccd7 | 397.829 | 218.711 | 14358.4 | 121.579 | 0.583194 | 0.00493815 | 987.37 | 1 | 0.720994 | 0.378681 | 80.5868 | 0.259347 | A | F | 3.42e+20 | 4.96233e-12 | 1 | dscxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X113151.48-123158.7 | chandra | ccd7 | 400.701 | 218.837 | 15913.3 | 126.148 | 0.646348 | 0.00512373 | 1094.29 | 1 | 1.26639 | 1.26639 | 0 | 0.281505 | T | F | 3.42e+20 | 4.81211e-12 | 1 | dscx | ||||
| Report | srcpi bgdpi arf | 3 | X113145.69-123458.4 | chandra | ccd6 | 137.977 | 799.385 | 29.1221 | 5.39649 | 0.00118285 | 0.000219189 | 23.1088 | 1 | 0.981334 | 0.74477 | 66.0812 | 3.10849 | F | F | 3.43e+20 | 1.25105e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X113107.35-123146.6 | chandra | ccd2 | 336.69 | 214.31 | 14.747 | 4.58267 | 0.000598977 | 0.000186134 | 12.0638 | 1 | 2.41514 | 1.71736 | 1.64504 | 10.8392 | F | F | 3.35e+20 | 8.43706e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X113137.92-123819.4 | chandra | ccd6 | 368.6 | 390.5 | 8.00146 | 3.16233 | 0.000324994 | 0.000128444 | 6.34928 | 0.999993 | 1.5546 | 0.750864 | 52.0385 | 6.95744 | A | F | 3.44e+20 | 4.32972e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X113142.09-123642.6 | chandra | ccd6 | 244.7 | 587.1 | 4.70624 | 2.23608 | 0.000191153 | 9.08223e-05 | 3.73447 | 0.998719 | 0.492235 | 0.492 | 170.783 | 5.05617 | F | F | 3.44e+20 | 2.18171e-15 | 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