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 | 2 | X110850.49-510232.5 | chandra | ccd3 | 970.547 | 275.994 | 17.9419 | 4.23579 | 0.00494236 | 0.00116681 | 37.1643 | 1 | 0.657106 | 0.311702 | 240.831 | 3.12891 | F | F | 1.79e+21 | 5.70397e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X110823.52-510527.7 | chandra | ccd2 | 979.722 | 770.611 | 8.86885 | 3 | 0.00244305 | 0.000826392 | 17.3939 | 1 | 0.518376 | 0.492 | 124.23 | 4.71398 | F | F | 1.8e+21 | 2.80212e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X110900.23-505523.9 | chandra | ccd3 | 781.833 | 1146.33 | 5.81764 | 2.44949 | 0.00160255 | 0.000674747 | 12.0505 | 1 | 0.980936 | 0.558912 | 63.8351 | 7.03554 | A | F | 1.76e+21 | 2.03034e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X110846.36-510323.9 | chandra | ccd2 | 542.3 | 1022.1 | 4.95147 | 2.23607 | 0.00136395 | 0.000615956 | 9.711 | 1 | 0.492 | 0.492 | 18.4349 | 3.17211 | F | F | 1.79e+21 | 1.5531e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X110834.30-505747.1 | chandra | ccd1 | 429.3 | 297.7 | 4.94246 | 2.23607 | 0.00136147 | 0.000615956 | 10.419 | 1 | 0.492 | 0.492 | 87.1447 | 3.21687 | F | F | 1.78e+21 | 1.52908e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X110847.98-510420.2 | chandra | ccd2 | 511.25 | 907.75 | 3.94923 | 2 | 0.00108787 | 0.000550928 | 7.74538 | 0.999992 | 0.513971 | 0.492 | 24.1832 | 4.0701 | F | F | 1.79e+21 | 1.27449e-14 | 1 | dx | ||||
| Report | 2 | X110836.89-510833.2 | chandra | ccd2 | 723.75 | 393.5 | 3.84044 | 2.00001 | 0.0010579 | 0.000550929 | 7.53202 | 0.999992 | 0.866517 | 0.492 | 33.5632 | 7.57885 | A | F | 1.81e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X110818.52-510458.3 | chandra | ccd2 | 1075.5 | 830.167 | 2.98347 | 1.73205 | 0.000821838 | 0.000477117 | 5.8513 | 0.999845 | 0.492 | 0.492 | 90 | 4.59305 | F | F | 1.8e+21 | 9.34607e-15 | 1 | dx | ||||
| Report | 2 | X110805.56-505559.8 | chandra | ccd1 | 981.5 | 515.5 | 1.91014 | 1.41422 | 0.000526174 | 0.000389565 | 4.02668 | 0.998394 | 0.492 | 0.492 | 180 | 6.62589 | F | F | 1.77e+21 | 0 | 1 | d | |||||
| Report | 3 | X110816.28-505816.6 | chandra | ccd1 | 775.25 | 237.75 | 3.969 | 2 | 0.00109332 | 0.000550928 | 8.36688 | 0.999996 | 0.493356 | 0.492 | 36.4486 | 3.80392 | F | F | 1.78e+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