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 | 3 | X132127.75-633338.9 | chandra | ccd7 | 865.733 | 448.487 | 17.4694 | 4.46044 | 0.00350968 | 0.000896122 | 5.46087 | 0.999997 | 0.565129 | 0.565129 | 0 | 2.85775 | 8.91528 | 10.7458 | 0.0931052 | 0.285168 | F | F | 1.16e+22 | 4.46576e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X132141.83-633511.0 | chandra | ccd7 | 674.535 | 261.528 | 12.0219 | 7.08631 | 0.00241524 | 0.00142367 | 3.758 | 0.999596 | 0.785851 | 0.425982 | 56.754 | 1.70152 | 15.5166 | 0.943569 | -0.885351 | 0.478653 | F | F | 1.15e+22 | 3.0601e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X132023.88-633539.6 | chandra | ccd3 | 427.429 | 651.852 | 14.4948 | 5.76787 | 0.00291579 | 0.00116027 | 3.34533 | 0.999006 | 2.45027 | 2.45027 | 0 | 10.0632 | 2.15329 | 15.0686 | 0.749936 | 0.397166 | F | F | 1.17e+22 | 5.21631e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X132217.81-633557.6 | chandra | ccd6 | 675.753 | 1093.46 | 9.91228 | 3.36828 | 0.00199143 | 0.000676706 | 8.28024 | 1 | 0.756318 | 0.756318 | 0 | 3.3406 | 5.8306 | 5.8306 | 0 | 0.309192 | F | F | 1.14e+22 | 2.98087e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X132129.13-633458.2 | chandra | ccd7 | 846.766 | 287.284 | 14.9734 | 3.91001 | 0.00300822 | 0.000785536 | 4.68063 | 0.999974 | 0.938969 | 0.938969 | 0 | 2.83471 | 7.74585 | 6.66114 | -0.0752909 | 0.348036 | F | F | 1.16e+22 | 4.14825e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 17 | X132117.14-633513.6 | chandra | ccd7 | 1009.38 | 255.702 | 9.7828 | 3.12775 | 0.0019654 | 0.000628376 | 3.05807 | 0.997921 | 0.528864 | 0.528864 | 0 | 4.18426 | 2.91503 | 3.91503 | 0.146412 | 0.566503 | F | F | 1.16e+22 | 2.59745e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X132143.83-633518.7 | chandra | ccd7 | 646.833 | 245.417 | 12.7272 | 5.4441 | 0.00255694 | 0.00109374 | 5.08165 | 0.99999 | 0.777183 | 0.492 | 41.7257 | 1.63965 | 10.1212 | 2.65967 | -0.583805 | 0.495774 | A | F | 1.15e+22 | 3.24166e-14 | 1 | dx |
Report | srcpi bgdpi arf | 7 | X132140.70-633505.2 | chandra | ccd7 | 689.409 | 272.682 | 14.3325 | 5.8734 | 0.00287943 | 0.00117998 | 4.86825 | 0.999986 | 1.06707 | 0.492 | 22.7528 | 1.73773 | 12.3171 | 2.09638 | -0.709108 | 0.501723 | A | F | 1.15e+22 | 3.62994e-14 | 1 | dx |
Report | srcpi bgdpi arf | 10 | X132153.91-633420.3 | chandra | ccd7 | 510.167 | 364.083 | 3.9018 | 4.7081 | 0.000783882 | 0.000945871 | 1.29356 | 0.921094 | 0.978158 | 0.556161 | 58.6942 | 0.305356 | 4.96085 | -0.962773 | -1 | 1.35173 | A | F | 1.15e+22 | 9.82266e-15 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X132131.00-633414.5 | chandra | ccd7 | 821.125 | 375.75 | 7.80264 | 3.95804 | 0.00156757 | 0.000795182 | 17.5633 | 1 | 0.844744 | 0.492 | 177.647 | 2.47722 | 2.90132 | 5 | 0.265612 | 0.523798 | A | F | 1.16e+22 | 1.97735e-14 | 1 | dx |
Report | srcpi bgdpi arf | 16 | X132101.03-633059.6 | chandra | ccd7 | 1229.12 | 770.875 | 7.91628 | 4.1225 | 0.0015904 | 0.000828222 | 7.60435 | 1 | 1.40732 | 0.818737 | 4.57821 | 6.56208 | 2.60592 | 5.5074 | 0.357619 | 0.544837 | A | F | 1.18e+22 | 2.22421e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X132151.82-633859.5 | chandra | ccd6 | 1027.5 | 723.7 | 4.81761 | 3.39792 | 0.000967881 | 0.000682657 | 11.2807 | 1 | 0.913712 | 0.492 | 140.655 | 4.94939 | 2.86321 | 1.9544 | -0.188643 | 0.728645 | A | F | 1.14e+22 | 1.50439e-14 | 1 | dx |
Report | 4 | X132229.05-634039.3 | chandra | ccd6 | 524.167 | 520.167 | 2.79811 | 1.73206 | 0.000562153 | 0.000347978 | 2.33741 | 0.984402 | 0.492 | 0.492 | 45 | 7.71865 | F | F | 1.12e+22 | 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