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 | X153437.91-020036.0 | chandra | ccd7 | 434.826 | 300.216 | 81.853 | 9.34115 | 0.0262485 | 0.0029955 | 35.2108 | 1 | 1.50783 | 0.750194 | 325.38 | 5.18571 | F | F | 7.04e+20 | 1.78367e-13 | 1 | dsx | ||||
Report | 4 | X153439.05-015139.6 | chandra | ccd6 | 797.031 | 405.562 | 10.7064 | 3.27206 | 0.0034333 | 0.00104928 | 24.2646 | 1 | 0.988131 | 0.328064 | 27.1858 | 3.91422 | F | F | 6.98e+20 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 3 | X153431.92-014741.1 | chandra | ccd6 | 1013.7 | 889.8 | 9.46813 | 3.16229 | 0.00303621 | 0.00101407 | 21.4582 | 1 | 1.28576 | 0.758805 | 114.216 | 7.8157 | A | F | 6.94e+20 | 3.24596e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X153510.43-015754.2 | chandra | ccd2 | 1022.28 | 342.611 | 8.16465 | 3.00002 | 0.00261821 | 0.000962035 | 18.8557 | 1 | 1.82273 | 1.28323 | 168.982 | 9.13028 | F | F | 7.06e+20 | 3.13505e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X153441.18-015720.5 | chandra | ccd7 | 334.5 | 697.072 | 6.81924 | 2.64576 | 0.00218677 | 0.000848432 | 2.93344 | 0.996142 | 0.666805 | 0.492 | 44.5453 | 2.40205 | F | F | 7.02e+20 | 1.37833e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X153514.11-015844.9 | chandra | ccd2 | 910.1 | 239.5 | 4.64837 | 2.23608 | 0.00149062 | 0.000717058 | 10.7351 | 0.999998 | 1.42626 | 0.91138 | 10.6118 | 10.2588 | A | F | 7.07e+20 | 1.82156e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X153439.75-015257.2 | chandra | ccd6 | 775 | 247.25 | 3.95732 | 2 | 0.00126902 | 0.000641354 | 8.96871 | 0.999998 | 0.492 | 0.492 | 142.018 | 2.74696 | F | F | 6.99e+20 | 1.178e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X153442.01-015041.9 | chandra | ccd6 | 706.167 | 522.167 | 2.96203 | 1.73205 | 0.000949853 | 0.000555429 | 6.71302 | 0.999949 | 0.492 | 0.492 | 153.435 | 5.05065 | F | F | 6.97e+20 | 9.13818e-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