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 | 1 | X175356.82-290110.9 | chandra | ccd1 | 255.301 | 964.754 | 31.9744 | 6.20354 | 0.0164325 | 0.00318816 | 12.5322 | 1 | 1.81194 | 1.81194 | 0 | 8.21955 | 21.4073 | 12.4073 | -0.266157 | 0.214218 | F | F | 6.24e+21 | 2.53144e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X175334.91-291004.8 | chandra | ccd0 | 757.667 | 911.667 | 5.90734 | 3.59808 | 0.00303588 | 0.00184911 | 19.4067 | 1 | 1.19426 | 0.65348 | 1.08463 | 7.10289 | 1.90734 | 4 | 0.354247 | 0.654736 | A | F | 6.27e+21 | 4.40628e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175419.98-290532.0 | chandra | ccd3 | 691.5 | 522.5 | 4.92512 | 3.39792 | 0.0025311 | 0.00174625 | 17.9981 | 1 | 0.556815 | 0.492 | 55.9007 | 4.53029 | 5 | 0 | -1 | 0.975663 | F | F | 5.85e+21 | 3.65036e-14 | 1 | dx |
| Report | 2 | X175420.54-291049.2 | chandra | ccd2 | 591.9 | 908.7 | 4.95196 | 2.23607 | 0.0025449 | 0.00114915 | 11.1358 | 1 | 0.710629 | 0.492 | 16.287 | 3.40244 | F | F | 5.69e+21 | 0 | 1 | d | |||||
| Report | 2 | X175421.81-290822.9 | chandra | ccd3 | 643 | 175 | 3.96451 | 2 | 0.00203743 | 0.00102783 | 8.47507 | 0.999997 | 0.492 | 0.492 | 112.5 | 3.28284 | F | F | 5.74e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X175425.26-291403.1 | chandra | ccd2 | 466.5 | 514.5 | 3.96445 | 3.17945 | 0.0020374 | 0.00163397 | 21.0274 | 1 | 1.17208 | 0.492 | 75.3211 | 6.34871 | 2 | 1.96445 | -0.00896626 | 0.816304 | A | F | 5.53e+21 | 2.93512e-14 | 1 | dx |
| Report | 4 | X175412.23-290915.6 | chandra | ccd3 | 898.167 | 68.1667 | 2.99486 | 1.73205 | 0.00153911 | 0.00089013 | 6.40221 | 0.99992 | 0.492 | 0.492 | 90 | 1.12686 | F | F | 5.83e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X175408.45-291126.1 | chandra | ccd2 | 913.833 | 833.833 | 2.91531 | 2.93649 | 0.00149823 | 0.00150911 | 10.0175 | 0.999998 | 0.492 | 0.492 | 45 | 2.36422 | 0.915307 | 2 | 0.372068 | 1.09797 | F | F | 5.82e+21 | 2.09824e-14 | 1 | dx |
| Report | 3 | X175405.46-291421.1 | chandra | ccd2 | 993.5 | 478.167 | 2.97478 | 1.73205 | 0.00152879 | 0.000890131 | 6.68955 | 0.999946 | 0.54799 | 0.492 | 56.9812 | 5.27567 | F | F | 5.77e+21 | 0 | 1 | d | |||||
| Report | 2 | X175355.44-291125.3 | chandra | ccd0 | 211.167 | 748.5 | 2.95282 | 1.73205 | 0.0015175 | 0.000890131 | 6.64159 | 0.999946 | 0.492 | 0.492 | 118.155 | 3.4573 | F | F | 5.98e+21 | 0 | 1 | d | |||||
| Report | 3 | X175408.52-290357.7 | chandra | ccd3 | 996.833 | 714.167 | 2.95178 | 1.73205 | 0.00151697 | 0.000890131 | 6.31012 | 0.99992 | 0.492 | 0.492 | 163.155 | 5.13542 | F | F | 6.02e+21 | 0 | 1 | d | |||||
| Report | 4 | X175434.59-291420.1 | chandra | ccd2 | 218.5 | 479.833 | 2.93394 | 1.73205 | 0.0015078 | 0.000890131 | 6.59771 | 0.999946 | 1.21764 | 0.602575 | 9.46232 | 7.96474 | A | F | 5.4e+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