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 | 4 | X060550.38-354031.9 | chandra | ccd3 | 455.362 | 270.91 | 23.8886 | 5.07869 | 0.00478792 | 0.00101791 | 17.31 | 1 | 2.2623 | 1.10935 | 131.141 | 7.84052 | 15.9585 | 6.46025 | -0.423674 | 0.285769 | F | F | 4.76e+20 | 6.57293e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X060624.78-353102.1 | chandra | ccd1 | 585.417 | 1115.08 | 12.9256 | 4.7081 | 0.00259066 | 0.000943635 | 47.3939 | 1 | 0.953081 | 0.837248 | 104.451 | 6.45376 | 3 | 10.9256 | 0.569139 | 0.402635 | F | F | 4.58e+20 | 3.45622e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X060525.58-354002.2 | chandra | ccd3 | 1069.32 | 330.409 | 10.5142 | 4.42783 | 0.00210731 | 0.000887446 | 15.0858 | 1 | 3.38639 | 1.07933 | 64.5654 | 9.33738 | 4.94603 | 5.56822 | 0.0591759 | 0.425319 | A | F | 4.56e+20 | 4.45065e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X060609.07-353813.8 | chandra | ccd1 | 975.875 | 238 | 7.76866 | 3.95804 | 0.00155706 | 0.000793302 | 16.1519 | 1 | 1.09736 | 0.599598 | 139.565 | 6.2798 | 5 | 2.76866 | -0.287223 | 0.535707 | A | F | 4.8e+20 | 2.24516e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X060634.73-353503.6 | chandra | ccd1 | 339.5 | 623.786 | 6.63336 | 3.78388 | 0.00132951 | 0.000758396 | 10.9551 | 1 | 2.25973 | 1.22312 | 151.405 | 8.57038 | 1.86251 | 4.77085 | 0.438441 | 0.630183 | A | F | 4.83e+20 | 1.8457e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X060534.62-353308.2 | chandra | ccd2 | 513.1 | 195.1 | 6.91531 | 3.78388 | 0.00138601 | 0.00075839 | 23.7622 | 1 | 0.492 | 0.492 | 53.677 | 3.99881 | 6 | 0.915307 | -0.735281 | 0.687162 | F | F | 4.34e+20 | 1.99516e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X060557.42-353835.4 | chandra | ccd3 | 280.5 | 507.25 | 3.91531 | 3.17945 | 0.000784724 | 0.00063724 | 13.4537 | 1 | 0.492 | 0.492 | 28.9973 | 5.89801 | 2.91531 | 1 | -0.489184 | 0.920111 | F | F | 4.73e+20 | 9.9476e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X060552.72-353703.8 | chandra | ccd3 | 397 | 693.5 | 3.91531 | 3.17945 | 0.000784724 | 0.00063724 | 13.4537 | 1 | 0.492 | 0.492 | 180 | 4.34374 | 2 | 1.91531 | -0.0216313 | 0.82671 | F | F | 4.64e+20 | 9.96504e-15 | 1 | dx |
| Report | 5 | X060609.81-353645.7 | chandra | ccd1 | 957.5 | 417 | 3.95187 | 2 | 0.000792066 | 0.000400856 | 7.9598 | 0.999994 | 0.492 | 0.492 | 31.7175 | 5.13545 | F | F | 4.74e+20 | 0 | 1 | d | |||||
| Report | 1 | X060551.69-352737.5 | chandra | ccd0 | 1078.75 | 566.5 | 3.93562 | 2 | 0.000788814 | 0.00040086 | 7.39999 | 0.999988 | 0.863988 | 0.492 | 144.325 | 5.12955 | A | F | 4.28e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X060606.88-352939.7 | chandra | ccd0 | 702.198 | 318.437 | 50.5979 | 7.11322 | 0.0101414 | 0.00142571 | 95.1372 | 1 | 1.15374 | 0.524138 | 32.0328 | 4.00712 | 29.9615 | 16.7308 | -0.283361 | 0.176482 | A | F | 4.43e+20 | 1.2177e-13 | 1 | dsx |
| Report | 1 | X060529.39-352706.3 | chandra | ccd2 | 643.5 | 930.5 | 3.84655 | 2 | 0.000770949 | 0.000400854 | 7.54564 | 0.999992 | 0.785439 | 0.579838 | 82.9819 | 7.55447 | F | F | 4.13e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X060625.56-353128.6 | chandra | ccd1 | 566.167 | 1061.17 | 2.79505 | 2.93649 | 0.000560206 | 0.000588555 | 6.17394 | 0.999938 | 0.813027 | 0.492 | 113.645 | 6.50718 | 2 | 0.846286 | -0.40534 | 1.1373 | A | F | 4.59e+20 | 7.45637e-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