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 | X051903.90-611626.1 | chandra | ccd3 | 390.993 | 904.663 | 121.322 | 11.4793 | 0.0247657 | 0.00234329 | 37.5259 | 1 | 3.38604 | 2.55783 | 22.2662 | 9.25569 | F | F | 2.33e+20 | 3.62977e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 4 | X052019.52-611534.0 | chandra | ccd7 | 523.992 | 431.346 | 110.88 | 11.0635 | 0.0226338 | 0.00225838 | 33.4542 | 1 | 0.390216 | 0.390216 | 0 | 0.155055 | F | F | 2.43e+20 | 1.91556e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X051907.07-611746.9 | chandra | ccd3 | 343.342 | 740.342 | 17.2259 | 4.35893 | 0.00351635 | 0.000889794 | 5.32811 | 0.999995 | 2.46392 | 1.51414 | 127.863 | 9.12152 | A | F | 2.34e+20 | 5.00959e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X051943.36-611109.9 | chandra | ccd7 | 1054.78 | 967 | 16.1386 | 4.24267 | 0.00329435 | 0.000866048 | 4.86928 | 0.999988 | 1.42793 | 0.922772 | 77.7696 | 6.20415 | A | F | 2.35e+20 | 2.64451e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X051947.76-611318.7 | chandra | ccd7 | 990.137 | 705.98 | 12.9831 | 4.84064 | 0.00265022 | 0.000988112 | 3.91721 | 0.999545 | 0.842862 | 0.842862 | 0 | 4.50064 | F | F | 2.36e+20 | 2.06887e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X052029.31-611059.5 | chandra | ccd7 | 379.7 | 988.8 | 9.67979 | 3.16228 | 0.00197592 | 0.000645512 | 2.92055 | 0.995397 | 0.948875 | 0.492 | 24.2175 | 4.59943 | A | F | 2.4e+20 | 1.73603e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X051948.35-612256.9 | chandra | ccd2 | 301.611 | 941.167 | 8.1081 | 3.00002 | 0.00165513 | 0.000612403 | 13.2147 | 1 | 1.50802 | 0.657483 | 31.6005 | 8.41769 | A | F | 2.44e+20 | 2.35631e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X052014.82-611546.9 | chandra | ccd7 | 592.357 | 404.643 | 6.85746 | 2.64575 | 0.0013998 | 0.000540073 | 2.069 | 0.968162 | 0.601111 | 0.492 | 27.504 | 0.752421 | T | F | 2.43e+20 | 1.04616e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X052021.36-611744.7 | chandra | ccd6 | 1081.5 | 1014.33 | 5.81447 | 2.44949 | 0.00118691 | 0.000500015 | 9.0494 | 1 | 0.604601 | 0.492 | 6.15401 | 2.27917 | F | F | 2.46e+20 | 1.29321e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X052055.21-611629.5 | chandra | ccd6 | 585.5 | 1166.5 | 3.90588 | 2 | 0.000797306 | 0.00040826 | 6.07895 | 0.999929 | 0.611917 | 0.492 | 71.565 | 4.29482 | F | F | 2.51e+20 | 9.20032e-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