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 | X174718.28-304110.1 | chandra | ccd0 | 153.321 | 184.423 | 36.4957 | 6.24503 | 0.0168961 | 0.00289121 | 78.5225 | 1 | 2.74476 | 2.26441 | 172.384 | 8.93863 | F | F | 8.87e+21 | 2.88985e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X174651.24-304527.2 | chandra | ccd1 | 717.4 | 668.6 | 9.91571 | 3.16228 | 0.0045906 | 0.00146402 | 21.0082 | 1 | 0.674179 | 0.492 | 63.7843 | 5.10323 | F | F | 9.06e+21 | 6.7364e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X174657.41-304806.0 | chandra | ccd1 | 556.167 | 345.722 | 8.74355 | 3.00001 | 0.00404793 | 0.00138889 | 18.5247 | 1 | 1.16416 | 0.521485 | 91.0671 | 8.02705 | A | F | 8.86e+21 | 6.43645e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X174637.34-303833.1 | chandra | ccd2 | 222.7 | 328.5 | 4.94088 | 2.23607 | 0.00228744 | 0.00103522 | 10.4897 | 1 | 0.492 | 0.492 | 2.41162e-08 | 2.86902 | F | T | 9.53e+21 | 3.49795e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X174635.57-304817.3 | chandra | ccd1 | 1128.1 | 323.1 | 4.77359 | 2.23608 | 0.00220999 | 0.00103522 | 10.1137 | 0.999996 | 0.749259 | 0.492 | 38.8676 | 6.87521 | A | F | 9.14e+21 | 3.55011e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X174636.48-303741.8 | chandra | ccd2 | 245.25 | 432.75 | 3.95319 | 2 | 0.00183018 | 0.000925925 | 8.3928 | 0.999996 | 0.492 | 0.492 | 45 | 3.7211 | F | F | 9.58e+21 | 2.80695e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X174613.82-304429.6 | chandra | ccd3 | 639 | 642.5 | 3.94797 | 2 | 0.00182776 | 0.000925925 | 8.40082 | 0.999996 | 0.492 | 0.492 | 63.4349 | 5.80407 | F | F | 9.56e+21 | 2.87944e-14 | 1 | dx | ||||
| Report | 3 | X174625.51-304733.6 | chandra | ccd3 | 332.5 | 268.75 | 3.90471 | 2 | 0.00180773 | 0.000925925 | 8.30877 | 0.999996 | 0.889076 | 0.492 | 13.7255 | 6.59842 | A | F | 9.3e+21 | 0 | 1 | d | |||||
| Report | 3 | X174615.18-303654.3 | chandra | ccd2 | 804 | 529 | 3.89744 | 2 | 0.00180437 | 0.000925926 | 8.27445 | 0.999996 | 0.871177 | 0.492 | 165.473 | 6.46566 | A | F | 9.88e+21 | 0 | 1 | d | |||||
| Report | 4 | X174633.03-303422.3 | chandra | ccd2 | 335.75 | 838.25 | 3.866 | 2 | 0.00178981 | 0.000925926 | 8.2077 | 0.999996 | 0.493356 | 0.492 | 36.4486 | 7.09037 | F | F | 9.75e+21 | 0 | 1 | d | |||||
| Report | 2 | X174623.26-303758.3 | chandra | ccd2 | 592.167 | 399.167 | 2.95539 | 1.73205 | 0.00136823 | 0.000801874 | 6.27443 | 0.999915 | 0.492 | 0.492 | 16.845 | 4.5008 | F | F | 9.74e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X174635.73-303404.1 | chandra | ccd2 | 264.833 | 875.167 | 2.76628 | 1.73206 | 0.00128068 | 0.000801877 | 5.87294 | 0.998457 | 0.628177 | 0.492 | 85.2688 | 7.35162 | F | F | 9.73e+21 | 2.20793e-14 | 1 | dx | ||||
| Report | 2 | X174627.08-304724.9 | chandra | ccd3 | 291.5 | 286.5 | 0.991386 | 1 | 0.000458974 | 0.000462962 | 2.10955 | 0.978922 | 0.492 | 0.492 | 90 | 6.34559 | F | F | 9.28e+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