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 | 11 | X123755.54-012047.6 | chandra | ccd7 | 592.834 | 423.049 | 29.3283 | 5.41556 | 0.00373398 | 0.000689491 | 22.4317 | 1 | 0.528707 | 0.528707 | 0 | 1.81067 | F | F | 1.93e+20 | 2.82642e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X123725.20-012817.1 | chandra | ccd6 | 1019.41 | 425.428 | 25.7465 | 6.16138 | 0.00327796 | 0.000784448 | 10.4176 | 1 | 5.44687 | 2.88797 | 29.521 | 9.29103 | F | F | 1.95e+20 | 4.03898e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X123757.13-011843.5 | chandra | ccd7 | 544.264 | 675.32 | 18.709 | 4.32894 | 0.00238197 | 0.000551146 | 14.3096 | 1 | 0.739272 | 0.739272 | 0 | 3.14993 | F | F | 1.92e+20 | 1.84568e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 9 | X123811.57-011622.9 | chandra | ccd7 | 103.682 | 960.682 | 12.8979 | 3.87302 | 0.00164211 | 0.000493098 | 9.86492 | 1 | 1.17359 | 0.609429 | 114.178 | 7.40764 | A | F | 1.92e+20 | 2.086e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X123753.97-012040.0 | chandra | ccd7 | 640 | 438.1 | 9.74596 | 3.16228 | 0.00124082 | 0.000402609 | 7.45419 | 1 | 0.492 | 0.492 | 90 | 1.44459 | F | F | 1.93e+20 | 9.35553e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X123747.67-011500.7 | chandra | ccd7 | 832 | 1127.8 | 8.65809 | 3.1623 | 0.00110231 | 0.000402612 | 6.62213 | 0.999998 | 0.979903 | 0.889281 | 177.695 | 5.97021 | F | F | 1.9e+20 | 9.36157e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X123726.18-012314.0 | chandra | ccd6 | 989.278 | 1041.17 | 8.11104 | 3.00002 | 0.00103267 | 0.000381951 | 3.2819 | 0.998341 | 1.49485 | 0.814528 | 11.5269 | 5.97832 | A | F | 1.93e+20 | 1.34478e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X123742.91-011914.8 | chandra | ccd7 | 977.375 | 611.25 | 7.55867 | 2.82844 | 0.000962341 | 0.000360105 | 5.78125 | 0.999987 | 0.593316 | 0.492 | 33.574 | 2.19992 | F | F | 1.92e+20 | 7.35162e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X123746.37-013030.3 | chandra | ccd6 | 373.9 | 154.3 | 7.29916 | 3.16234 | 0.000929301 | 0.000402617 | 2.9534 | 0.995773 | 2.93272 | 2.36946 | 57.8619 | 9.53859 | F | F | 1.96e+20 | 1.22462e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X123746.34-012930.5 | chandra | ccd6 | 374.667 | 275.833 | 9.1612 | 3.46415 | 0.00116637 | 0.000441042 | 3.70682 | 0.999386 | 4.05967 | 1.67022 | 49.3616 | 8.54386 | A | F | 1.96e+20 | 1.45457e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X123738.18-012654.9 | chandra | ccd6 | 623.907 | 592.613 | 20.4776 | 4.52522 | 0.00260714 | 0.000576136 | 8.28567 | 1 | 2 | 1.25365 | 22.3155 | 6.45501 | F | F | 1.94e+20 | 2.98692e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X123757.75-011919.9 | chandra | ccd7 | 524.833 | 600.833 | 5.63686 | 2.4495 | 0.000717663 | 0.000311861 | 4.31135 | 0.999598 | 0.59004 | 0.492 | 32.3269 | 2.8735 | F | F | 1.92e+20 | 5.5449e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X123752.78-011618.1 | chandra | ccd7 | 676.5 | 970.5 | 3.71911 | 2.00001 | 0.000473503 | 0.000254633 | 2.84456 | 0.991795 | 0.492 | 0.492 | 90 | 4.80824 | F | F | 1.91e+20 | 3.76878e-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