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 | X123049.02+122329.8 | chandra | ccd7 | 817.703 | 120.765 | 264.551 | 32.6866 | 0.0567191 | 0.00700793 | 9.38905 | 1 | 1.21137 | 1.21137 | 0 | 0.303771 | T | F | 1.94e+20 | 3.71776e-13 | 1 | dbscxf | ||||
Report | srcpi bgdpi arf rmf | 2 | X123048.88+122330.9 | chandra | ccd7 | 821.333 | 122.442 | 100.927 | 13.1912 | 0.0216384 | 0.00282816 | 3.58195 | 0.999771 | 0.660356 | 0.492 | 122.821 | 0.284934 | T | F | 1.94e+20 | 1.60122e-13 | 1 | dcx | ||||
Report | srcpi bgdpi arf rmf | 3 | X123048.63+122332.4 | chandra | ccd7 | 829.316 | 126.071 | 893.456 | 40.6301 | 0.191554 | 0.00871098 | 31.7092 | 1 | 0.497161 | 0.497161 | 0 | 0.268531 | F | F | 1.93e+20 | 1.41675e-12 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 4 | X123048.16+122335.6 | chandra | ccd7 | 843.298 | 132.498 | 135.174 | 26.1806 | 0.0289808 | 0.00561303 | 4.7974 | 0.999999 | 1.5 | 1.5 | 0 | 0.283399 | T | F | 1.93e+20 | 2.14242e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X123047.26+122342.2 | chandra | ccd7 | 870.202 | 145.891 | 59.7632 | 26.1298 | 0.0128131 | 0.00560216 | 2.12103 | 0.981906 | 1.5 | 1.5 | 354.373 | 0.438456 | T | F | 1.93e+20 | 9.4884e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 7 | X123049.40+122328.3 | chandra | ccd7 | 806.542 | 117.707 | 3165.39 | 66.3363 | 0.678651 | 0.0142223 | 112.341 | 1 | 0.558169 | 0.558169 | 0 | 0.357464 | F | F | 1.94e+20 | 5.01702e-12 | 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