Distributions of flux ratios fitted with Gaussian profiles: pn vs ... Smallish azimuthal angle dependence at low energies. Batch effect not so strong here ? ...
F.J.Carrera, J. Ebrero Instituto de Fisica de Cantabria. G. Lamer AIP-Potsdam ... Empirical sensitivity maps calculation (see Carrera 07) 11. 2.0-12. 1.7. 0.5-2.0. 24 ...
Astrometry and EPIC flux cross-calibration in. 2XMMp/2XMM. Silvia Mateos. R. Saxton, S. Sembay and the. XMM-Newton Survey Science Centre. 2XMMp astrometry ...
martin still, christopher brindle, mat page, vladimir yershov, alice breeveld, houri ziaeepour ... queries before then: martin still mds@mssl.ucl.ac.uk ...
Jenny Carter (jac48@star.le.ac.uk) 3rd EPIC BG WG Meeting. MPE, ... Jenny Carter, University of Leicester. Andy Read, University of Leicester. XMM. EPIC ...
INTEGRAL IBIS Survey (Bassani et al., 2006) sensitivity ... INTEGRAL IBIS Survey (Sazonov et al., 2006) ... INTEGRAL IBIS AGN Survey (Beckmann et al., 2006) ...
Evolution with decaying and re ... A model based on field-dependent decay of the magnetic moment of NSs can provide an evolutionary ... Initially the toroidal field ...
Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...
Isolated Neutron Stars. Intro. Stars in the Galaxy Prediction ... Good old classics The old zoo of neutron stars Rocket experiments Sco X-1 UHURU Accretion in close ...
HST, Spitzer, VLA, GALEX, CFHT LS blah blah blah 'AEGIS' ApJL special issue (~20 ... AGN contribution to the total luminosity of the universe (c.f. stars) ...
and the XMM-Newton Survey Science Centre. Department of Physics and Astronomy, ... All 119 XMM-Newton observations with overlap on the original area covered by the ...