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 | X170231.95-421907.7 | chandra | ccd7 | 609.692 | 202.745 | 44.9709 | 6.70603 | 0.00525896 | 0.000784213 | 43.0456 | 1 | 0.718769 | 0.537513 | 63.5268 | 2.3534 | 32 | 11.8733 | -0.458747 | 0.193298 | F | T | 1.52e+22 | 7.48578e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X170313.00-422124.0 | chandra | ccd6 | 326.316 | 705.5 | 37.2217 | 7.30476 | 0.00435275 | 0.000854229 | 27.9118 | 1 | 2.67855 | 1.22296 | 74.4216 | 7.92142 | 32.5747 | 4.76289 | -0.744875 | 0.244612 | A | F | 1.48e+22 | 7.91098e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X170136.10-421940.5 | chandra | ccd3 | 704.033 | 836.533 | 18.6872 | 6.63471 | 0.0021853 | 0.000775873 | 5.32555 | 0.999998 | 5.99974 | 4.64087 | 136.174 | 11.6404 | 11.1838 | 5.83087 | -0.314605 | 0.39908 | F | F | 1.56e+22 | 4.40855e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X170230.42-421829.2 | chandra | ccd7 | 644.297 | 281.005 | 13.5167 | 3.67829 | 0.00158066 | 0.000430145 | 12.938 | 1 | 0.391485 | 0.179585 | 22.0223 | 1.96682 | 0 | 11.9611 | 1 | 0.544534 | F | F | 1.52e+22 | 2.21597e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X170246.27-421502.7 | chandra | ccd7 | 286.1 | 700.2 | 9.70899 | 4.27872 | 0.00113538 | 0.000500359 | 17.9979 | 1 | 0.492 | 0.492 | 138.563 | 2.55519 | 9.806 | 0 | -1 | 0.622541 | F | F | 1.51e+22 | 1.67991e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X170235.15-421045.8 | chandra | ccd7 | 537.2 | 1222.4 | 9.02068 | 4.27872 | 0.00105489 | 0.000500359 | 9.11541 | 1 | 1.81983 | 0.657749 | 151.184 | 6.24885 | 3.78577 | 5.32672 | 0.169102 | 0.480429 | A | F | 1.53e+22 | 1.60615e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X170202.78-423108.7 | chandra | ccd2 | 726.214 | 230.214 | 5.39603 | 3.78388 | 0.000631019 | 0.000442492 | 4.26065 | 0.999735 | 3.07461 | 1.71307 | 81.9568 | 15.5203 | 2.52824 | 2.91496 | 0.0710457 | 0.705114 | A | F | 1.52e+22 | 1.43649e-14 | 1 | dx |
| Report | 3 | X170245.90-421500.1 | chandra | ccd7 | 294.5 | 705.5 | 4.92043 | 2.23607 | 0.000575403 | 0.000261489 | 4.70978 | 0.999858 | 0.492 | 0.492 | 90 | 2.54528 | F | F | 1.51e+22 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X170247.91-421750.7 | chandra | ccd6 | 891.25 | 1139.75 | 4.91531 | 3.39792 | 0.000574803 | 0.000397357 | 16.8899 | 1 | 0.492 | 0.492 | 16.0027 | 2.12546 | 0 | 4.91531 | 1 | 0.992474 | F | F | 1.51e+22 | 9.35985e-15 | 1 | dx |
| Report | 8 | X170232.48-421925.2 | chandra | ccd7 | 597.167 | 166.833 | 2.89174 | 1.73206 | 0.000338164 | 0.000202549 | 2.76794 | 0.974885 | 0.492 | 0.492 | 0 | 2.58346 | F | F | 1.52e+22 | 0 | 1 | d | |||||
| Report | 6 | X170210.39-421504.7 | chandra | ccd7 | 1095.83 | 695.833 | 2.8589 | 1.73206 | 0.000334324 | 0.000202549 | 2.73651 | 0.974885 | 0.492 | 0.492 | 94.7312 | 5.34799 | F | F | 1.54e+22 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 7 | X170231.76-421157.6 | chandra | ccd7 | 613.833 | 1076.5 | 4.66123 | 3.39792 | 0.00054509 | 0.000397357 | 8.0084 | 0.999998 | 0.492 | 0.492 | 180 | 5.14511 | 2 | 2.66123 | 0.141857 | 0.747448 | F | F | 1.53e+22 | 7.97188e-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