Relativistic corrections to Sunyaev-Zeldovich effect

DOI

These tables contain numerical values for the distortion of the spectral intensity {Delta}I/y defined by the equation {Delta}I/y = 1/y * X^3^/(e^X^-1) * {Delta}n(X)/n0(X) = X^3^/(e^X^-1)F({theta}e,X) The spectral intensity is the function of two variables X and {theta}e. Here X={omega}/k_B_T_0_, {omega} being the photon angular frequency and k_B_T_0_ being the thermal energy of CMB photons, and {theta}e=k_B_Te/m_e_c^2^, k_B_Te being the thermal energy of the electrons and m_e_*c^2^ being the electron rest energy (T_0_ is the temperature of the cosmic microwave background radiation). In these tables, the range for X is taken as 0<X<20 and the range for {theta}e is taken as 0.002<{theta}e<0.100.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34170827
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/417/827
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/417/827
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/417/827
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/417/827
Provenance
Creator Itoh N.; Nozawa S.
Publisher CDS
Publication Year 2004
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics