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 | 3 | X175642.52-282836.3 | chandra | ccd1 | 89.6665 | 512.5 | 5.93488 | 2.44949 | 0.00305004 | 0.00125884 | 14.3308 | 1 | 0.809254 | 0.492 | 37.6373 | 4.29124 | A | F | 5.32e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X175720.05-283249.2 | chandra | ccd3 | 134.333 | 82.8333 | 5.84649 | 3.59808 | 0.00300461 | 0.00184911 | 14.922 | 1 | 1.43147 | 0.51906 | 51.0729 | 7.22984 | 1.90789 | 3.9386 | 0.347337 | 0.660124 | A | F | 4.77e+21 | 4.43241e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X175710.24-283734.9 | chandra | ccd2 | 317.5 | 519.5 | 4.81497 | 3.39792 | 0.00247449 | 0.00174625 | 11.1936 | 1 | 0.822315 | 0.598851 | 164.518 | 6.98939 | 5 | -0.185033 | -1 | 0.975663 | F | F | 4.71e+21 | 3.55325e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X175718.08-283150.4 | chandra | ccd3 | 187.1 | 202.5 | 4.9064 | 3.39792 | 0.00252148 | 0.00174625 | 16.0368 | 1 | 1.33515 | 0.492 | 64.4749 | 6.8604 | -0.0312011 | 4.9376 | 1 | 0.987994 | A | F | 4.82e+21 | 3.66267e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X175622.54-282706.8 | chandra | ccd1 | 625.3 | 694.1 | 4.77341 | 3.39792 | 0.00245314 | 0.00174625 | 10.0279 | 1 | 1.04463 | 0.698717 | 145.036 | 7.82623 | 2.88671 | 1.88671 | -0.209494 | 0.738334 | F | F | 5.6e+21 | 3.4934e-14 | 1 | dx |
Report | 4 | X175649.24-283148.0 | chandra | ccd3 | 959.5 | 207.833 | 2.97787 | 1.73205 | 0.00153038 | 0.000890131 | 7.27008 | 0.999971 | 0.492 | 0.492 | 90 | 1.07897 | F | F | 5.14e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X175640.27-283724.8 | chandra | ccd0 | 76.5 | 465.167 | 4.91531 | 3.39792 | 0.00252606 | 0.00174625 | 16.8899 | 1 | 0.492 | 0.492 | 90 | 4.87772 | 0 | 4.91531 | 1 | 0.992474 | F | F | 5.02e+21 | 3.75895e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X175629.96-283150.9 | chandra | ccd1 | 425.833 | 116.833 | 2.83061 | 2.93649 | 0.0014547 | 0.00150911 | 6.87766 | 0.99997 | 0.492 | 0.492 | 45 | 3.88249 | -0.0846933 | 2.91531 | 1 | 1.4553 | F | F | 5.34e+21 | 1.87879e-14 | 1 | dx |
Report | 3 | X175703.28-282559.9 | chandra | ccd3 | 583.167 | 915.167 | 2.94466 | 1.73205 | 0.00151331 | 0.000890131 | 7.18902 | 0.999971 | 1.01742 | 0.492 | 25.5362 | 7.64799 | A | F | 5.19e+21 | 0 | 1 | d | |||||
Report | 4 | X175623.43-282840.7 | chandra | ccd1 | 601.167 | 503.167 | 2.89516 | 1.73205 | 0.00148787 | 0.000890132 | 6.99089 | 0.999969 | 0.492 | 0.492 | 106.845 | 6.62428 | F | F | 5.54e+21 | 0 | 1 | d | |||||
Report | 5 | X175640.71-283020.3 | chandra | ccd1 | 138 | 301 | 1.98854 | 1.41421 | 0.00102195 | 0.000726788 | 4.8017 | 0.99926 | 0.492 | 0.492 | 45 | 2.81432 | F | F | 5.28e+21 | 0 | 1 | d | |||||
Report | 2 | X175702.02-283847.3 | chandra | ccd2 | 537.5 | 372.5 | 0.975141 | 1 | 0.000501142 | 0.000513918 | 2.41667 | 0.9881 | 0.492 | 0.492 | 90 | 6.84503 | F | F | 4.73e+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