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 | X084828.56+611248.1 | chandra | ccd7 | 1099.67 | 964.667 | 5.83061 | 3.59808 | 0.00378875 | 0.00233804 | 14.1669 | 1 | 0.492 | 0.492 | 19.9028 | 1.92671 | 5 | 0.915307 | -0.690529 | 0.748989 | F | F | 4.07e+20 | 2.91425e-14 | 1 | dx |
| Report | 2 | X084928.50+611016.6 | chandra | ccd7 | 218.833 | 657.5 | 2.92191 | 1.73205 | 0.00189867 | 0.00112549 | 3.37848 | 0.992775 | 1.09881 | 0.524652 | 162.123 | 5.79033 | A | F | 4.15e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X084837.91+611204.1 | chandra | ccd7 | 962.5 | 875.167 | 2.91531 | 2.93649 | 0.00189438 | 0.00190814 | 10.0175 | 0.999998 | 0.492 | 0.492 | 151.845 | 0.953304 | 3 | -0.0846933 | -1 | 1.41421 | F | F | 4.07e+20 | 1.43356e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X084852.42+610654.9 | chandra | ccd7 | 749.1 | 246.7 | 4.86278 | 3.39792 | 0.00315985 | 0.00220798 | 13.1274 | 1 | 0.850474 | 0.689137 | 37.3724 | 5.76531 | 2.93139 | 1.93139 | -0.205644 | 0.72421 | F | F | 4.09e+20 | 2.57627e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X084846.12+611234.7 | chandra | ccd7 | 842.449 | 937.816 | 42.7453 | 6.59494 | 0.0277769 | 0.00428555 | 49.4246 | 1 | 0.449264 | 0.449264 | 0 | 0.198395 | 31.9153 | 11 | -0.487362 | 0.197867 | F | F | 4.08e+20 | 2.08107e-13 | 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