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 | 1 | X025838.08-571118.4 | chandra | ccd1 | 1211.93 | 761.429 | 27.5906 | 6.3619 | 0.00549545 | 0.00126715 | 43.1218 | 1 | 1.82252 | 0.881162 | 84.2852 | 7.46313 | 23.9181 | 3.67249 | -0.733787 | 0.287046 | A | F | 1.29e+20 | 8.07679e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X025932.74-571704.4 | chandra | ccd3 | 679.017 | 1025.26 | 22.9383 | 4.98632 | 0.00456884 | 0.000993172 | 23.3806 | 1 | 1.02636 | 0.312146 | 238.239 | 4.93334 | 15 | 5.94851 | -0.432083 | 0.295911 | A | F | 1.26e+20 | 5.80612e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X025849.00-572327.3 | chandra | ccd2 | 454.356 | 604.673 | 12.0383 | 4.08022 | 0.00239926 | 0.000813197 | 5.60687 | 0.999993 | 1.58411 | 0.434479 | 11.2101 | 5.28244 | 8.88389 | 4.90711 | -0.28836 | 0.367743 | F | F | 1.32e+20 | 3.19483e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X025807.50-571517.2 | chandra | ccd0 | 729.667 | 651.083 | 11.3798 | 4.57071 | 0.00226661 | 0.000910386 | 14.4505 | 1 | 1.36406 | 1.11008 | 175.673 | 7.38363 | 4.79328 | 6.58656 | 0.157584 | 0.409706 | F | F | 1.33e+20 | 3.18496e-14 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X025918.60-571730.9 | chandra | ccd3 | 912.01 | 971.825 | 9.7576 | 3.12372 | 0.00194351 | 0.000622179 | 9.94574 | 1 | 0.623898 | 0.30502 | 359.928 | 2.97057 | 9 | 1.9586 | -0.642546 | 0.484205 | F | F | 1.28e+20 | 2.34729e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X025846.96-571943.1 | chandra | ccd2 | 487.611 | 1059.83 | 8.86511 | 4.1225 | 0.00176683 | 0.000821619 | 24.1375 | 1 | 0.618323 | 0.492 | 103.403 | 1.99914 | 6 | 2.86511 | -0.353621 | 0.498004 | F | F | 1.31e+20 | 2.15248e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X025924.90-571718.5 | chandra | ccd3 | 807.75 | 996.375 | 7.84773 | 3.95804 | 0.0015631 | 0.000788355 | 20.111 | 1 | 0.547364 | 0.492 | 62.5417 | 3.84549 | 3 | 4.84773 | 0.235448 | 0.523639 | F | F | 1.27e+20 | 1.92837e-14 | 1 | dx |
Report | srcpi bgdpi arf | 6 | X025908.59-571542.5 | chandra | ccd1 | 708.357 | 224.929 | 6.70729 | 3.78388 | 0.00133594 | 0.000753666 | 12.3973 | 1 | 0.570057 | 0.492 | 61.1378 | 3.00062 | 4.85364 | 1.85364 | -0.447275 | 0.625279 | F | F | 1.28e+20 | 1.59281e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X025937.22-572425.7 | chandra | ccd3 | 606.928 | 127.643 | 6.76272 | 3.78388 | 0.00134699 | 0.000753666 | 13.8833 | 1 | 1.09898 | 0.769999 | 141.264 | 8.15002 | 4.94068 | 1.82204 | -0.461152 | 0.623403 | F | F | 1.28e+20 | 2.03132e-14 | 1 | dx |
Report | 8 | X025836.01-572029.6 | chandra | ccd2 | 667.667 | 965.167 | 5.96968 | 2.44949 | 0.00118976 | 0.000488186 | 2.7804 | 0.992107 | 0.492 | 0.492 | 147.757 | 3.62477 | F | F | 1.32e+20 | 0 | 1 | d | |||||
Report | 4 | X025854.18-572121.2 | chandra | ccd2 | 368.833 | 860.5 | 5.91354 | 2.44949 | 0.00117858 | 0.000488186 | 2.75425 | 0.992107 | 0.552968 | 0.492 | 151.845 | 3.08507 | F | F | 1.31e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X025855.73-571331.3 | chandra | ccd1 | 920.333 | 491.5 | 5.76872 | 3.59808 | 0.001149 | 0.000716658 | 11.9953 | 1 | 0.540945 | 0.492 | 106.603 | 4.78176 | 1 | 4.76872 | 0.653303 | 0.754901 | F | F | 1.28e+20 | 1.43007e-14 | 1 | dx |
Report | srcpi bgdpi arf | 6 | X025806.96-572249.2 | chandra | ccd2 | 1144.83 | 680.333 | 6.41489 | 3.78388 | 0.00127849 | 0.000754132 | 8.38629 | 1 | 1.31256 | 0.907001 | 27.7209 | 8.1688 | 5.70744 | 1.70744 | -0.539455 | 0.612943 | F | F | 1.36e+20 | 1.86096e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X025953.77-572116.4 | chandra | ccd3 | 333.7 | 511.7 | 4.7928 | 3.39792 | 0.00095462 | 0.00067679 | 10.5291 | 1 | 1.03056 | 0.630548 | 90 | 8.1696 | 0.896399 | 3.8964 | 0.625939 | 0.849091 | A | F | 1.26e+20 | 1.40801e-14 | 1 | dx |
Report | 6 | X025935.64-571803.0 | chandra | ccd3 | 631 | 905.5 | 3.95352 | 2 | 0.000787455 | 0.000398356 | 4.02975 | 0.996883 | 0.492 | 0.492 | 37.9819 | 5.17166 | F | F | 1.26e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X025908.87-571639.2 | chandra | ccd1 | 703.75 | 109.5 | 3.91531 | 3.17945 | 0.000779843 | 0.000633277 | 13.4537 | 1 | 0.492 | 0.492 | 90 | 2.26082 | 2 | 1.91531 | -0.0216313 | 0.82671 | F | F | 1.28e+20 | 9.18469e-15 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X025917.50-571358.0 | chandra | ccd1 | 561.167 | 437.167 | 2.85346 | 2.93649 | 0.000568346 | 0.000584885 | 7.45397 | 0.999983 | 0.569535 | 0.492 | 126.65 | 5.11481 | 0.926728 | -0.0732718 | -1 | 3.68416 | F | F | 1.27e+20 | 7.12417e-15 | 1 | dx |
Report | 2 | X025827.89-571620.7 | chandra | ccd0 | 393.167 | 522.833 | 2.94053 | 1.73205 | 0.000585689 | 0.000344987 | 5.0773 | 0.999596 | 0.492 | 0.492 | 4.73116 | 4.43803 | F | F | 1.32e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X025832.41-571752.0 | chandra | ccd0 | 318.5 | 337.3 | 4.92115 | 3.39792 | 0.000980184 | 0.00067679 | 17.5249 | 1 | 0.529275 | 0.492 | 163.997 | 3.40144 | 4 | 0.921147 | -0.625637 | 0.826833 | F | F | 1.32e+20 | 1.29597e-14 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X025853.21-571256.9 | chandra | ccd1 | 962 | 561.5 | 3.91531 | 3.17945 | 0.000779843 | 0.000633277 | 13.4537 | 1 | 0.492 | 0.492 | 180 | 5.38033 | 1 | 2.91531 | 0.489184 | 0.920111 | F | F | 1.28e+20 | 1.00798e-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