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 | X132938.63+582505.7 | chandra | ccd7 | 737.504 | 152.048 | 1538.69 | 39.8624 | 0.170615 | 0.00442006 | 365.087 | 1 | 0.414784 | 0.379837 | 83.0876 | 0.53061 | F | F | 1.75e+20 | 6.99665e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 5 | X132940.24+582454.1 | chandra | ccd7 | 711.757 | 128.521 | 33.8458 | 6.06736 | 0.00375292 | 0.000672766 | 8.03063 | 1 | 0.379601 | 0.379601 | 0 | 0.721346 | F | F | 1.75e+20 | 2.25777e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X132940.48+583625.5 | chandra | ccd3 | 171.019 | 472.278 | 16.6021 | 5.19632 | 0.00184089 | 0.000576181 | 22.1572 | 1 | 4.91246 | 3.85712 | 35.358 | 11.5065 | F | F | 1.75e+20 | 2.36787e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X132942.69+582515.0 | chandra | ccd7 | 672.786 | 170.969 | 11.165 | 3.34141 | 0.00123801 | 0.000370507 | 2.64913 | 0.991259 | 0.295272 | 0.295272 | 0 | 1.08335 | F | F | 1.75e+20 | 7.45154e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X132911.61+582423.1 | chandra | ccd6 | 162.5 | 356.25 | 3.90778 | 2 | 0.000433304 | 0.000221765 | 4.75641 | 0.999332 | 0.492 | 0.492 | 55.278 | 3.08041 | F | F | 1.7e+20 | 4.01777e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X132851.79+582315.5 | chandra | ccd6 | 479.5 | 219.5 | 1.93708 | 1.41422 | 0.000214788 | 0.000156812 | 2.35775 | 0.96883 | 0.492 | 0.492 | 180 | 5.87376 | F | F | 1.66e+20 | 2.10468e-15 | 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