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 | 5 | X134112.87-143840.2 | chandra | ccd2 | 414.915 | 144.306 | 90.8125 | 15.3382 | 0.0193428 | 0.00326701 | 7.55594 | 1 | 0.290795 | 0.290795 | 0 | 1.25288 | F | F | 4.98e+20 | 2.45929e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X134127.45-144845.2 | chandra | ccd1 | 587.643 | 234.214 | 20.1372 | 4.79587 | 0.00429207 | 0.0010222 | 39.8654 | 1 | 2.53665 | 2.08186 | 26.3528 | 9.46554 | F | F | 5.14e+20 | 6.41467e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X134055.92-143919.5 | chandra | ccd3 | 537.5 | 1053.83 | 5.94794 | 2.44949 | 0.00126687 | 0.000521725 | 11.6461 | 1 | 0.557807 | 0.492 | 131.203 | 4.27606 | F | F | 5.02e+20 | 1.58598e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X134103.39-144548.3 | chandra | ccd3 | 316.833 | 263.667 | 5.74649 | 2.4495 | 0.00122396 | 0.000521726 | 11.2516 | 1 | 1.13261 | 0.762793 | 124.071 | 6.3703 | F | F | 5.11e+20 | 1.55642e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X134101.55-143921.6 | chandra | ccd3 | 371.3 | 1049.7 | 4.90491 | 2.23607 | 0.00104471 | 0.000476268 | 9.60382 | 1 | 0.715565 | 0.492 | 0.716048 | 2.92561 | F | F | 5e+20 | 1.25863e-14 | 1 | dx | ||||
| Report | 1 | X134127.53-143758.2 | chandra | ccd0 | 1007 | 582.25 | 3.9704 | 2 | 0.000845689 | 0.000425997 | 7.28515 | 0.999985 | 0.497677 | 0.492 | 70.6701 | 3.92697 | F | F | 4.95e+20 | 0 | 1 | d | |||||
| Report | 4 | X134057.54-144253.7 | chandra | ccd3 | 489.5 | 618.5 | 3.93069 | 2 | 0.00083721 | 0.000425986 | 7.6963 | 0.999992 | 0.492 | 0.492 | 90 | 4.86243 | F | F | 5.05e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X134142.86-144359.4 | chandra | ccd1 | 133.167 | 814.833 | 2.78091 | 1.73206 | 0.000592728 | 0.000369174 | 5.50535 | 0.999856 | 0.492 | 0.492 | 45 | 8.20127 | F | F | 5.02e+20 | 7.97437e-15 | 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