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 | 6 | X080405.86+050649.8 | chandra | ccd7 | 195.53 | 253.438 | 1698.49 | 42.1258 | 0.180391 | 0.00447405 | 337.023 | 1 | 0.425405 | 0.425405 | 0 | 0.272471 | F | F | 3.45e+20 | 6.0255e-12 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 2 | X080405.97+051034.0 | chandra | ccd7 | 192.129 | 709.044 | 50.4047 | 7.1067 | 0.00535332 | 0.00075478 | 10.0016 | 1 | 1.0966 | 0.524587 | 316.848 | 3.92771 | F | F | 3.48e+20 | 4.13786e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X080403.50+050748.3 | chandra | ccd7 | 267.042 | 372.378 | 23.9617 | 4.89507 | 0.0025449 | 0.00051989 | 4.75461 | 0.99999 | 0.52318 | 0.52318 | 0 | 1.40269 | F | F | 3.45e+20 | 1.87573e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X080359.08+051139.0 | chandra | ccd7 | 400.909 | 840.636 | 19.0222 | 4.69045 | 0.00202029 | 0.000498157 | 3.77449 | 0.999721 | 1.65461 | 1.01837 | 3.50608 | 5.35037 | A | F | 3.48e+20 | 1.60565e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X080409.03+050414.3 | chandra | ccd6 | 380.722 | 933.833 | 8.82351 | 3 | 0.000937115 | 0.00031862 | 9.21326 | 1 | 0.680713 | 0.492 | 65.874 | 2.47595 | F | F | 3.43e+20 | 9.58248e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X080406.18+050425.3 | chandra | ccd6 | 467.333 | 956.167 | 5.85117 | 2.44949 | 0.000621433 | 0.000260152 | 6.10963 | 0.999951 | 0.492 | 0.492 | 113.021 | 2.22394 | F | F | 3.42e+20 | 6.40471e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X080411.57+050335.4 | chandra | ccd6 | 303.5 | 854.786 | 6.77135 | 2.64576 | 0.000719162 | 0.000280997 | 7.07045 | 0.999994 | 0.497465 | 0.492 | 136.635 | 3.28915 | F | F | 3.43e+20 | 7.44278e-15 | 1 | dx | ||||
Report | 4 | X080413.09+050240.5 | chandra | ccd6 | 257.5 | 743.25 | 3.91378 | 2 | 0.000415669 | 0.000212413 | 4.08666 | 0.997459 | 0.492 | 0.492 | 90 | 4.27844 | F | F | 3.42e+20 | 0 | 1 | d |
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