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 | 1 | X042412.58+144529.0 | xmm | mos1 | 316.175 | 313.362 | 232.298 | 22.284 | 0.251419 | 0.0241182 | 15.0206 | 1 | 5.06076 | 4.16415 | 48.865 | 1.67413 | F | F | 3.54441 | 0 | 1 | ds | ||||
| Report | srcpi bgdpi | 1 | X042412.70+144528.6 | xmm | mos2 | 315.791 | 313.259 | 206.153 | 21.208 | 0.24644 | 0.0253526 | 13.2077 | 1 | 6.37163 | 4.5699 | 12.0168 | 1.66726 | F | F | 3.54455 | 0 | 1 | dbs | ||||
| Report | srcpi bgdpi | 2 | X042350.60+145519.6 | xmm | mos2 | 389.387 | 448.985 | 122.941 | 15.2449 | 0.0745799 | 0.00924809 | 7.87647 | 1 | 10.875 | 10.875 | 0 | 12.7519 | F | F | 3.50995 | 0 | 1 | d | ||||
| Report | srcpi bgdpi | 2 | X042350.63+145515.7 | xmm | mos1 | 389.285 | 448.248 | 67.5648 | 16.7821 | 0.0731262 | 0.0181634 | 4.3688 | 0.999985 | 9.30984 | 9.30984 | 0 | 12.751 | F | F | 3.50996 | 0 | 1 | ds | ||||
| Report | srcpi bgdpi | 1 | X042350.47+145518.7 | xmm | pn | 389.825 | 448.947 | 33.2995 | 7.52785 | 0.151589 | 0.0342689 | 4.29392 | 0.999968 | 4.16577 | 4.16577 | 0 | 12.7666 | F | F | 3.51071 | 0 | 1 | ds | ||||
| Report | srcpi bgdpi | 2 | X042412.61+144529.0 | xmm | pn | 316.078 | 313.366 | 180.133 | 16.6447 | 0.820018 | 0.0757714 | 23.2279 | 1 | 5.51317 | 5.51317 | 0 | 1.67699 | F | F | 3.54445 | 0 | 1 | ds |
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 - 10.00 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), A = 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