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 | X131957.03-351055.6 | chandra | ccd7 | 834.021 | 1015.5 | 32.4723 | 6.02229 | 0.00949016 | 0.00176004 | 16.6675 | 1 | 0.697 | 0.482805 | 242.319 | 3.45273 | 19.9414 | 12 | -0.248624 | 0.217583 | F | F | 4.35e+20 | 7.68493e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X132034.08-351144.2 | chandra | ccd6 | 774.25 | 370.125 | 7.94632 | 3.95804 | 0.00232232 | 0.00115674 | 34.2957 | 1 | 0.776315 | 0.492 | 14.7518 | 4.40536 | 6 | 1.94632 | -0.510134 | 0.565093 | A | F | 4.47e+20 | 2.79828e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X132013.20-351126.1 | chandra | ccd7 | 430.625 | 953 | 7.92271 | 3.95804 | 0.00231542 | 0.00115674 | 28.4979 | 1 | 0.539489 | 0.492 | 153.688 | 0.81105 | 0 | 7.92271 | 1 | 0.714005 | F | F | 4.4e+20 | 1.75619e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X132011.57-352644.1 | chandra | ccd3 | 986 | 322.125 | 7.32881 | 3.95804 | 0.00214185 | 0.00115674 | 8.94565 | 1 | 4.37757 | 1.82631 | 47.2782 | 14.4983 | 3.82337 | 2.54077 | -0.201536 | 0.613658 | A | F | 4.27e+20 | 3.37371e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X132026.69-350938.4 | chandra | ccd6 | 958.167 | 625.833 | 8.83061 | 4.1225 | 0.00258076 | 0.0012048 | 21.4561 | 1 | 0.492 | 0.492 | 45 | 3.87025 | 6.91531 | 1.91531 | -0.566212 | 0.541658 | F | F | 4.45e+20 | 2.94703e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X132054.34-350834.0 | chandra | ccd6 | 268.875 | 755.875 | 7.41362 | 3.95804 | 0.00216664 | 0.00115674 | 9.68146 | 1 | 2.96129 | 1.28173 | 8.59538 | 9.27535 | 3.67016 | 3.81676 | 0.0195802 | 0.534368 | A | F | 4.55e+20 | 2.67586e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X132042.93-351922.9 | chandra | ccd2 | 1115.07 | 722.5 | 6.62099 | 3.78388 | 0.00193499 | 0.00110584 | 10.7547 | 1 | 2.88827 | 0.994522 | 44.7185 | 9.44394 | 5.91254 | 0.708452 | -0.785998 | 0.73546 | A | F | 4.45e+20 | 2.63387e-14 | 1 | dx |
| Report | 6 | X132014.68-350812.6 | chandra | ccd6 | 1257.7 | 800.3 | 4.97151 | 2.23607 | 0.00145293 | 0.000653493 | 11.8651 | 1 | 0.492 | 0.492 | 45 | 4.04972 | F | F | 4.42e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X132040.84-350806.8 | chandra | ccd6 | 605.3 | 811.7 | 4.83488 | 3.39792 | 0.001413 | 0.000993044 | 11.8982 | 1 | 1.18695 | 0.771651 | 10.1882 | 7.08479 | 2.88992 | 1.94496 | -0.195446 | 0.726959 | A | F | 4.51e+20 | 1.77152e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X132016.39-351131.5 | chandra | ccd7 | 351 | 942 | 3.91531 | 3.17945 | 0.00114425 | 0.000929197 | 13.4537 | 1 | 0.492 | 0.492 | 112.5 | 1.04427 | 3 | 0.915307 | -0.532447 | 0.936375 | F | F | 4.41e+20 | 8.70939e-15 | 1 | dx |
| Report | 2 | X131959.34-352305.5 | chandra | ccd3 | 1290.17 | 766.5 | 2.95185 | 1.73205 | 0.00086268 | 0.000506194 | 7.25802 | 0.999973 | 0.627179 | 0.492 | 123.69 | 11.1873 | F | F | 4.26e+20 | 0 | 1 | d | |||||
| Report | 4 | X132014.06-350740.8 | chandra | ccd6 | 1273 | 865 | 1.97028 | 1.41421 | 0.000575817 | 0.000413306 | 4.70232 | 0.999209 | 0.492 | 0.492 | 45 | 4.56822 | F | F | 4.42e+20 | 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