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 | X155058.64-562835.2 | chandra | ccd7 | 622.228 | 376.402 | 62.7816 | 7.92348 | 0.0129536 | 0.00163484 | 65.7186 | 1 | 0.479613 | 0.479613 | 0 | 0.583574 | F | F | 1.01e+22 | 1.48998e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X155101.39-562836.9 | chandra | ccd7 | 575.916 | 372.87 | 22.891 | 4.78445 | 0.00472307 | 0.000987171 | 23.9619 | 1 | 1.06693 | 1.06693 | 0 | 0.76012 | T | F | 1.01e+22 | 5.44597e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X155052.37-562608.0 | chandra | ccd7 | 727.898 | 675.673 | 14.4786 | 3.80763 | 0.00298736 | 0.000785626 | 15.1559 | 1 | 0.60729 | 0.60729 | 0 | 3.09293 | F | F | 1.05e+22 | 3.60422e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X155047.55-562325.5 | chandra | ccd7 | 808.75 | 1005.38 | 13.9326 | 4.00003 | 0.00273221 | 0.000784412 | 14.5844 | 1 | 2.14751 | 0.707556 | 48.7317 | 5.87778 | A | F | 1.08e+22 | 3.50372e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X155119.35-562722.9 | chandra | ccd7 | 273.334 | 523.122 | 12.9771 | 3.60237 | 0.00267755 | 0.000743273 | 13.5842 | 1 | 0.730227 | 0.730227 | 0 | 3.50825 | F | F | 1e+22 | 3.1861e-14 | 1 | dsx | ||||
Report | 1 | X155052.83-563550.2 | chandra | ccd6 | 550.333 | 512.833 | 10.4016 | 3.46412 | 0.00203977 | 0.00067932 | 16.2753 | 1 | 0.626484 | 0.492 | 146.208 | 6.72177 | F | F | 9.53e+21 | 0 | 1 | dc | |||||
Report | srcpi bgdpi arf | 9 | X155055.50-562906.3 | chandra | ccd7 | 674.5 | 312.722 | 8.71513 | 3.00001 | 0.00170905 | 0.000588306 | 9.12283 | 1 | 0.492 | 0.492 | 33.9168 | 0.261186 | F | F | 1.01e+22 | 1.96616e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X155053.06-562902.0 | chandra | ccd7 | 715.611 | 321.5 | 8.71425 | 3.00001 | 0.00170888 | 0.000588306 | 9.1219 | 1 | 0.492 | 0.492 | 90 | 0.605616 | F | F | 1.02e+22 | 1.97689e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X155121.88-562746.7 | chandra | ccd7 | 230.167 | 474.167 | 5.66313 | 2.4495 | 0.00111055 | 0.00048035 | 5.92806 | 0.999953 | 0.683166 | 0.492 | 145.685 | 3.64916 | F | F | 9.96e+21 | 1.32646e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X155051.18-563148.1 | chandra | ccd6 | 578.1 | 1004.9 | 4.8741 | 2.23607 | 0.000955818 | 0.000438497 | 7.62646 | 0.999995 | 0.492 | 0.492 | 156.137 | 2.79135 | F | F | 9.93e+21 | 1.31077e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X155059.18-563733.2 | chandra | ccd6 | 443.7 | 303.5 | 6.76505 | 2.82846 | 0.00132664 | 0.000554664 | 10.5852 | 1 | 0.946926 | 0.614652 | 19.5178 | 8.41277 | A | F | 9.29e+21 | 2.12684e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X155059.76-563728.5 | chandra | ccd6 | 433.9 | 312.9 | 4.25288 | 2.23609 | 0.000833997 | 0.0004385 | 6.65445 | 0.999932 | 1.57896 | 1.00175 | 163.62 | 8.33851 | A | F | 9.29e+21 | 1.32475e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X155041.91-563646.9 | chandra | ccd6 | 733.5 | 397.333 | 5.03211 | 2.44952 | 0.000986805 | 0.000480354 | 7.87371 | 0.999995 | 2.30203 | 1.63166 | 133.314 | 7.93048 | F | F | 9.56e+21 | 1.50736e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf rmf | 6 | X155052.50-563554.6 | chandra | ccd6 | 556.23 | 504.365 | 120.918 | 10.9963 | 0.0237121 | 0.00215638 | 189.199 | 1 | 2.97309 | 2.05747 | 29.3753 | 6.80936 | F | F | 9.53e+21 | 2.69091e-13 | 1 | dscxf |
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