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 | 4 | X111802.78-042408.9 | chandra | ccd3 | 1021.53 | 442.33 | 38.9037 | 6.23728 | 0.0076188 | 0.00122149 | 68.4812 | 1 | 0.569365 | 0.372405 | 15.8879 | 2.12838 | F | F | 3.76e+20 | 8.77085e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X111758.76-043300.7 | chandra | ccd2 | 911.869 | 382.5 | 30.0875 | 5.48521 | 0.00589226 | 0.00107421 | 53.6814 | 1 | 2.36448 | 1.52445 | 220.486 | 6.9451 | F | F | 3.68e+20 | 8.27166e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X111817.87-043342.7 | chandra | ccd2 | 331.177 | 297.109 | 13.818 | 3.71726 | 0.00270608 | 0.000727978 | 24.6537 | 1 | 3.56117 | 1.97404 | 336.384 | 8.95409 | F | F | 3.73e+20 | 4.0377e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X111811.71-042728.1 | chandra | ccd2 | 517.611 | 1058.06 | 8.87515 | 3 | 0.00173808 | 0.00058751 | 15.8348 | 1 | 0.533472 | 0.492 | 114.985 | 3.44963 | F | F | 3.76e+20 | 2.13453e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X111821.17-041946.5 | chandra | ccd3 | 462.056 | 975.167 | 8.09747 | 3.00002 | 0.00158578 | 0.000587513 | 14.2538 | 1 | 1.26774 | 0.886896 | 61.6497 | 8.36261 | F | F | 3.86e+20 | 2.28616e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X111825.65-042537.9 | chandra | ccd3 | 325.833 | 260.833 | 5.67966 | 2.4495 | 0.00111228 | 0.000479701 | 9.99775 | 1 | 0.744336 | 0.492 | 34.4194 | 6.64111 | A | F | 3.82e+20 | 1.55604e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X111752.29-043227.1 | chandra | ccd2 | 1107.83 | 450.167 | 5.66034 | 2.4495 | 0.0011085 | 0.000479701 | 10.099 | 0.999999 | 1.40086 | 0.930979 | 171.158 | 6.6057 | A | F | 3.66e+20 | 1.55948e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X111826.82-042659.1 | chandra | ccd3 | 290.5 | 95.8333 | 5.55281 | 2.4495 | 0.00108744 | 0.000479702 | 9.77447 | 0.999999 | 0.848796 | 0.492 | 97.8543 | 6.97759 | A | F | 3.81e+20 | 1.51906e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X111752.12-042242.4 | chandra | ccd1 | 322.1 | 377.7 | 4.89939 | 2.23607 | 0.000960646 | 0.000438437 | 8.96718 | 0.999999 | 0.492 | 0.492 | 83.7356 | 3.77928 | F | F | 3.75e+20 | 1.15223e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X111745.33-042906.4 | chandra | ccd0 | 298.5 | 617.1 | 4.90062 | 2.23607 | 0.00095972 | 0.000437904 | 9.17571 | 0.999999 | 0.645911 | 0.492 | 161.736 | 4.57934 | F | F | 3.67e+20 | 1.17702e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X111745.47-043348.6 | chandra | ccd0 | 294.25 | 43.5 | 6.97408 | 2.82846 | 0.00136578 | 0.000553916 | 13.058 | 1 | 2.86329 | 1.1655 | 93.7172 | 8.45378 | A | F | 3.63e+20 | 2.58942e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X111721.44-042632.7 | chandra | ccd0 | 1024.83 | 929.5 | 2.59043 | 1.73206 | 0.0005073 | 0.000339201 | 4.85021 | 0.996872 | 1.37992 | 0.759584 | 12.1139 | 9.39169 | A | F | 3.65e+20 | 1.2649e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X111741.44-043212.7 | chandra | ccd0 | 416.773 | 238.5 | 21.2823 | 4.69042 | 0.00416785 | 0.000918556 | 39.848 | 1 | 1.55764 | 0.996196 | 89.5053 | 7.5547 | A | F | 3.63e+20 | 5.92772e-14 | 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