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 rmf | 1 | X023437.38-084713.0 | chandra | ccd7 | 158.251 | 766.313 | 131.775 | 15.6579 | 0.00580952 | 0.000690305 | 8.46068 | 1 | 1.73182 | 1.73182 | 0 | 0.240023 | T | F | 3.17e+20 | 4.53645e-14 | 1 | dpcbsxf | ||||
Report | srcpi bgdpi arf | 2 | X023436.95-084710.2 | chandra | ccd7 | 170.686 | 771.616 | 50.088 | 7.93736 | 0.00220821 | 0.00034993 | 3.21593 | 0.999077 | 0.610715 | 0.492 | 34.2035 | 0.239097 | F | F | 3.17e+20 | 1.64894e-14 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 3 | X023436.35-084705.8 | chandra | ccd7 | 189.274 | 781.05 | 80.2084 | 10.5077 | 0.00353611 | 0.000463249 | 5.14982 | 1 | 1.5 | 0.430478 | 329.237 | 0.297484 | A | F | 3.17e+20 | 2.64291e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 4 | X023436.24-084704.9 | chandra | ccd7 | 192.801 | 782.938 | 98.9919 | 9.94947 | 0.00436421 | 0.000438638 | 6.35582 | 1 | 1.30884 | 1.30884 | 0 | 0.34479 | T | F | 3.17e+20 | 3.45525e-14 | 1 | dcsx | ||||
Report | srcpi bgdpi arf rmf | 5 | X023437.83-084716.5 | chandra | ccd7 | 144.739 | 759.304 | 33429.9 | 188.755 | 1.47381 | 0.00832154 | 2146.38 | 1 | 0.436424 | 0.436424 | 0 | 0.295555 | F | F | 3.17e+20 | 1.09895e-11 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 7 | X023438.56-084721.9 | chandra | ccd7 | 122.659 | 748.376 | 69.5923 | 12.6977 | 0.00306808 | 0.000559799 | 4.46821 | 0.999992 | 1.5 | 0.315869 | 333.256 | 0.449113 | A | F | 3.17e+20 | 2.28767e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 8 | X023438.49-084721.7 | chandra | ccd7 | 124.767 | 748.767 | 65.776 | 14.7863 | 0.00289984 | 0.000651878 | 4.22318 | 0.999976 | 1.45688 | 1.45688 | 0 | 0.404985 | T | F | 3.17e+20 | 2.16231e-14 | 1 | dscbx | ||||
Report | srcpi bgdpi arf | 9 | X023437.27-084712.5 | chandra | ccd7 | 161.672 | 767.391 | 98.9172 | 14.9441 | 0.00436092 | 0.000658833 | 6.35103 | 1 | 1.5 | 0.4006 | 334.93 | 0.231848 | A | F | 3.17e+20 | 3.25374e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 10 | X023437.07-084711.2 | chandra | ccd7 | 167.675 | 770.002 | 97.5859 | 12.8609 | 0.00430223 | 0.000566992 | 6.26555 | 1 | 1.5 | 1.5 | 0 | 0.234625 | T | F | 3.17e+20 | 3.21115e-14 | 1 | dbscx | ||||
Report | srcpi bgdpi arf | 11 | X023436.69-084708.2 | chandra | ccd7 | 179.245 | 776.193 | 55.6525 | 11.5846 | 0.00245352 | 0.000510723 | 3.5732 | 0.999744 | 1.5 | 0.392586 | 333.24 | 0.259865 | A | F | 3.17e+20 | 1.83417e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 12 | X023435.92-084702.5 | chandra | ccd7 | 202.346 | 787.758 | 65.8898 | 8.67008 | 0.00290485 | 0.000382234 | 4.23049 | 0.999976 | 1.80023 | 0.464397 | 330.764 | 0.411019 | A | F | 3.17e+20 | 3.25733e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 13 | X023439.42-084728.2 | chandra | ccd7 | 96.723 | 735.575 | 52.3066 | 7.36758 | 0.00230602 | 0.000324812 | 3.35837 | 0.999391 | 1.9369 | 0.589826 | 338.617 | 0.678497 | A | F | 3.17e+20 | 3.65252e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 15 | X023438.91-084724.4 | chandra | ccd7 | 112.108 | 743.197 | 71.9913 | 10.6916 | 0.00317385 | 0.000471356 | 4.62224 | 0.999995 | 1.80023 | 0.278218 | 334.746 | 0.546576 | A | F | 3.17e+20 | 2.36726e-14 | 1 | dsx |
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