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 | X045708.29+452749.3 | chandra | ccd6 | 201.659 | 891.724 | 503.116 | 22.5536 | 0.185172 | 0.00830083 | 213.596 | 1 | 3.51958 | 2.811 | 48.3151 | 7.9116 | F | F | 5.47e+21 | 2.7706e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X045635.18+453241.8 | chandra | ccd5 | 544.269 | 591.115 | 10.1821 | 3.60561 | 0.00373866 | 0.0013239 | 16.4334 | 1 | 4.63475 | 2.77739 | 108.317 | 13.492 | A | F | 5.46e+21 | 5.26766e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X045633.21+453043.4 | chandra | ccd5 | 586.732 | 350.587 | 48.3518 | 8.30683 | 0.0177537 | 0.00305009 | 78.0371 | 1 | 6.18738 | 5.0308 | 119.323 | 11.7962 | F | F | 5.49e+21 | 2.36414e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X045705.77+451803.6 | chandra | ccd7 | 692.667 | 719.833 | 5.87302 | 2.44949 | 0.00215644 | 0.000899401 | 9.815 | 1 | 0.492 | 0.492 | 10.4272 | 2.09907 | F | F | 5.54e+21 | 2.16995e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X045717.39+452004.8 | chandra | ccd7 | 443.7 | 966.3 | 4.89877 | 2.23607 | 0.00179872 | 0.000821037 | 8.18683 | 0.999998 | 0.492 | 0.492 | 87.1447 | 2.83249 | F | F | 5.51e+21 | 1.82043e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X045642.27+451734.3 | chandra | ccd7 | 1196.75 | 660.5 | 3.92173 | 2 | 0.00143998 | 0.000734358 | 6.55401 | 0.999964 | 0.492 | 0.492 | 145.278 | 4.13407 | F | F | 5.58e+21 | 2.75984e-14 | 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