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 | X102821.97+484136.0 | chandra | ccd7 | 54.961 | 126.071 | 97.3846 | 11.0259 | 0.00418491 | 0.000473817 | 33.1489 | 1 | 2.0057 | 2.0057 | 0 | 6.22473 | F | F | 1.06e+20 | 4.34049e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X102803.91+484727.5 | chandra | ccd7 | 418.388 | 840.483 | 30.9065 | 6.0837 | 0.00132814 | 0.000261435 | 10.5203 | 1 | 0.338669 | 0.338669 | 0 | 0.366421 | F | F | 1.03e+20 | 9.67804e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X102804.09+484703.1 | chandra | ccd7 | 414.167 | 790.405 | 19.5122 | 4.5826 | 0.000838495 | 0.000196928 | 6.64178 | 1 | 0.492 | 0.492 | 4.49462 | 0.0572041 | F | T | 1.04e+20 | 6.07795e-15 | 1 | dpx | ||||
Report | srcpi bgdpi arf | 5 | X102806.33+484649.0 | chandra | ccd7 | 369.214 | 761.643 | 5.97653 | 2.64577 | 0.000256829 | 0.000113697 | 2.03436 | 0.969307 | 0.492 | 0.492 | 171.323 | 0.43729 | F | F | 1.04e+20 | 1.85867e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X102804.75+484712.7 | chandra | ccd7 | 401.366 | 810.443 | 11.2992 | 4.04609 | 0.000485562 | 0.000173873 | 3.84615 | 0.999357 | 0.490162 | 0.490162 | 0 | 0.136647 | F | F | 1.04e+20 | 3.53352e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 9 | X102812.00+484419.0 | chandra | ccd7 | 255.663 | 457.322 | 13.4094 | 4.35927 | 0.000576241 | 0.000187331 | 4.56445 | 0.999964 | 0.682622 | 0.682622 | 0 | 3.05677 | F | F | 1.05e+20 | 4.25734e-15 | 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