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 | X175542.20-283919.6 | chandra | ccd1 | 861.357 | 663.929 | 19.9755 | 5.66369 | 0.0102548 | 0.00290756 | 19.7356 | 1 | 3.42252 | 1.72537 | 15.3162 | 9.12279 | 5.61583 | 14.3597 | 0.43773 | 0.310965 | A | F | 5.69e+21 | 1.51752e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175640.14-283725.2 | chandra | ccd3 | 360.115 | 997.654 | 13.0699 | 4.84057 | 0.00670942 | 0.0024849 | 13.5523 | 1 | 3.16068 | 2.67069 | 153.396 | 9.27187 | 5.3561 | 8.64228 | 0.234754 | 0.366894 | F | F | 5.02e+21 | 1.01546e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X175603.65-284239.8 | chandra | ccd1 | 287.5 | 257.5 | 9.83061 | 4.27872 | 0.00504673 | 0.00219656 | 23.8859 | 1 | 0.492 | 0.492 | 45 | 3.36912 | 1.91531 | 7.91531 | 0.610338 | 0.514425 | F | F | 5.28e+21 | 6.41376e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X175630.00-284416.0 | chandra | ccd3 | 631.833 | 163 | 5.91531 | 3.59808 | 0.00303661 | 0.00184706 | 20.326 | 1 | 0.492 | 0.492 | 45.7956 | 3.31741 | 3 | 2.91531 | -0.0143177 | 0.616388 | F | F | 4.82e+21 | 3.98179e-14 | 1 | dx |
| Report | 5 | X175634.59-284356.2 | chandra | ccd3 | 509.167 | 203 | 5.94736 | 2.44949 | 0.00305306 | 0.00125744 | 13.8972 | 1 | 0.551825 | 0.492 | 46.193 | 4.36927 | F | F | 4.79e+21 | 0 | 1 | d | |||||
| Report | 1 | X175618.64-284540.1 | chandra | ccd2 | 833.5 | 1012.1 | 4.96662 | 2.23607 | 0.00254966 | 0.0011479 | 12.2133 | 1 | 0.492 | 0.492 | 119.518 | 1.0866 | F | F | 4.93e+21 | 0 | 1 | d | |||||
| Report | 4 | X175617.95-284204.5 | chandra | ccd3 | 953.9 | 430.3 | 4.96596 | 2.23607 | 0.00254926 | 0.00114788 | 11.604 | 1 | 0.492 | 0.492 | 144.217 | 2.88964 | F | F | 5.1e+21 | 0 | 1 | d | |||||
| Report | 2 | X175614.58-284402.6 | chandra | ccd3 | 1044.17 | 190.167 | 2.97775 | 1.73205 | 0.00152862 | 0.000889145 | 6.95813 | 0.999959 | 0.492 | 0.492 | 45 | 0.863172 | F | F | 5.06e+21 | 0 | 1 | d | |||||
| Report | 3 | X175632.38-284251.4 | chandra | ccd3 | 568.167 | 334.833 | 2.97467 | 1.73205 | 0.00152704 | 0.000889145 | 6.95093 | 0.999959 | 0.492 | 0.492 | 45 | 4.29453 | F | F | 4.86e+21 | 0 | 1 | d | |||||
| Report | 1 | X175558.14-284658.4 | chandra | ccd0 | 348.5 | 765.833 | 2.97388 | 1.73205 | 0.00152673 | 0.0008892 | 7.09048 | 0.999965 | 0.492 | 0.492 | 90 | 4.26608 | F | F | 5.19e+21 | 0 | 1 | d | |||||
| Report | 2 | X175607.07-284734.8 | chandra | ccd0 | 109.722 | 691.944 | 8.97268 | 3 | 0.0046064 | 0.00154014 | 21.3931 | 1 | 0.492 | 0.492 | 131.709 | 3.2127 | F | F | 5.03e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X175557.49-284427.3 | chandra | ccd1 | 451.833 | 38.8335 | 2.91531 | 2.93649 | 0.00149663 | 0.0015075 | 10.0175 | 0.999998 | 0.492 | 0.492 | 90 | 3.89414 | -0.0846933 | 3 | 1 | 1.41421 | F | F | 5.29e+21 | 1.93609e-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