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 | X174714.90-261647.9 | chandra | ccd0 | 443.286 | 1052.29 | 12.1115 | 3.74169 | 0.00562308 | 0.00173718 | 18.8884 | 1 | 3.10563 | 1.93513 | 172.877 | 9.8865 | A | F | 7.9e+21 | 9.32104e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X174625.44-263133.8 | chandra | ccd3 | 586.409 | 86.7727 | 9.00176 | 3.31667 | 0.00418534 | 0.00154208 | 15.7412 | 1 | 2.88244 | 1.98986 | 106.705 | 8.69129 | F | F | 7.61e+21 | 8.76497e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X174616.48-262432.5 | chandra | ccd3 | 831.611 | 942.944 | 8.46806 | 3.00001 | 0.0039372 | 0.00139484 | 14.8079 | 1 | 1.41897 | 1.08648 | 121.304 | 6.37216 | F | F | 7.23e+21 | 6.00335e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X174629.06-262610.7 | chandra | ccd3 | 488 | 743.625 | 7.93006 | 2.82843 | 0.00368705 | 0.00131507 | 13.8671 | 1 | 0.492 | 0.492 | 37.0703 | 4.1333 | F | T | 7.46e+21 | 5.25966e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X174634.20-263106.3 | chandra | ccd3 | 347.357 | 142.786 | 6.53942 | 2.64576 | 0.00304048 | 0.00123014 | 11.4353 | 1 | 1.30636 | 0.492 | 31.3381 | 7.46029 | A | T | 7.72e+21 | 4.60973e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X174653.14-262016.9 | chandra | ccd0 | 1038.5 | 627.833 | 5.88423 | 2.44949 | 0.00273191 | 0.00113724 | 9.17674 | 1 | 0.592588 | 0.492 | 118.155 | 4.18854 | F | F | 7.57e+21 | 4.13971e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X174713.12-262622.4 | chandra | ccd1 | 333.167 | 903.5 | 5.71875 | 2.4495 | 0.00265891 | 0.00113888 | 7.08621 | 0.999994 | 0.492 | 0.492 | 90 | 6.74814 | F | F | 8.12e+21 | 4.27175e-14 | 1 | dx | ||||
Report | 4 | X174633.42-262314.3 | chandra | ccd2 | 553.1 | 84.1001 | 4.96738 | 2.23607 | 0.00230624 | 0.00103816 | 9.56596 | 1 | 0.492 | 0.492 | 45 | 2.68022 | F | T | 7.4e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 7 | X174637.49-262759.3 | chandra | ccd3 | 257.7 | 522.9 | 4.94786 | 2.23607 | 0.00230049 | 0.00103965 | 8.65222 | 0.999999 | 0.492 | 0.492 | 166.717 | 4.2821 | F | T | 7.66e+21 | 3.23786e-14 | 1 | dx | ||||
Report | 6 | X174629.59-263113.6 | chandra | ccd3 | 473.25 | 128 | 3.86357 | 2 | 0.00179636 | 0.000929895 | 6.75615 | 0.999976 | 0.497677 | 0.492 | 19.3299 | 7.96031 | F | F | 7.66e+21 | 0 | 1 | d | |||||
Report | 2 | X174629.73-261840.8 | chandra | ccd2 | 654 | 640 | 3.84368 | 2.00001 | 0.00178453 | 0.000928557 | 7.40199 | 0.999991 | 0.557273 | 0.492 | 172.982 | 6.33568 | F | F | 7.27e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 5 | X174633.58-262512.9 | chandra | ccd3 | 364.5 | 861.167 | 2.94436 | 1.73205 | 0.00136897 | 0.000805312 | 5.14874 | 0.999633 | 0.492 | 0.492 | 90 | 2.78371 | F | F | 7.48e+21 | 1.90651e-14 | 1 | dx | ||||
Report | 1 | X174615.61-261945.4 | chandra | ccd2 | 1039.83 | 508.5 | 2.89427 | 1.73205 | 0.00134375 | 0.000804153 | 5.57366 | 0.999822 | 0.492 | 0.492 | 3.1007e-08 | 7.82272 | F | F | 7.12e+21 | 0 | 1 | d | |||||
Report | 3 | X174630.18-262205.3 | chandra | ccd2 | 641.5 | 224.5 | 0.97327 | 1 | 0.000451867 | 0.000464278 | 1.87428 | 0.969564 | 0.492 | 0.492 | 90 | 3.81812 | F | T | 7.34e+21 | 0 | 1 | d |
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