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 rmf | 1 | X130617.83-482745.4 | chandra | ccd7 | 131.106 | 316.1 | 3472.03 | 59.9975 | 0.298464 | 0.00515753 | 662.911 | 1 | 0.398557 | 0.398557 | 0 | 0.678758 | F | T | 1.26e+21 | 1.0295e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 8 | X130616.54-482747.9 | chandra | ccd7 | 157.263 | 311.086 | 1519.73 | 39.4874 | 0.13064 | 0.00339443 | 290.16 | 1 | 0.394803 | 0.394803 | 0 | 0.588524 | F | T | 1.26e+21 | 8.34825e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X130618.68-482715.7 | chandra | ccd7 | 113.855 | 376.605 | 96.7929 | 10.1616 | 0.00832054 | 0.000873516 | 18.4806 | 1 | 0.375715 | 0.375715 | 0 | 1.19282 | F | F | 1.26e+21 | 5.33914e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X130611.35-482725.2 | chandra | ccd7 | 262.065 | 357.32 | 75.7945 | 8.95274 | 0.00651546 | 0.000769598 | 14.4714 | 1 | 0.356834 | 0.356834 | 0 | 1.2652 | F | F | 1.26e+21 | 4.16762e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X130616.54-482227.9 | chandra | ccd7 | 157.167 | 961.48 | 36.3164 | 6.02631 | 0.00312184 | 0.000518035 | 6.93385 | 1 | 1.62519 | 1.62519 | 0 | 5.92044 | F | F | 1.24e+21 | 2.15077e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X130614.52-482500.7 | chandra | ccd7 | 198.105 | 650.986 | 31.4146 | 6.28351 | 0.00270047 | 0.000540144 | 5.99795 | 1 | 0.680773 | 0.680773 | 0 | 3.38991 | F | F | 1.25e+21 | 1.77346e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X130619.45-483829.9 | chandra | ccd6 | 171 | 36.75 | 18.8304 | 5.29164 | 0.00154551 | 0.000434314 | 16.9334 | 1 | 5.84621 | 2.04251 | 179.15 | 10.1263 | A | T | 1.3e+21 | 1.70293e-14 | 1 | dpx | ||||
| Report | srcpi bgdpi arf | 3 | X130613.74-482716.2 | chandra | ccd7 | 213.832 | 375.491 | 15.1487 | 4.59246 | 0.00130222 | 0.00039478 | 2.89232 | 0.996424 | 0.362053 | 0.362053 | 0 | 1.19222 | F | F | 1.26e+21 | 8.33882e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X130617.53-483535.9 | chandra | ccd6 | 210.261 | 390.942 | 31.2598 | 5.68924 | 0.00256567 | 0.000466948 | 28.1106 | 1 | 4.52494 | 2.0583 | 80.8848 | 7.17381 | A | F | 1.29e+21 | 2.77903e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X130619.41-483115.0 | chandra | ccd6 | 171.7 | 920.7 | 4.7176 | 2.23608 | 0.000387199 | 0.000183527 | 4.24234 | 0.998258 | 0.585769 | 0.492 | 45 | 2.91091 | F | F | 1.28e+21 | 3.53703e-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