Relativistic corrections to Sunyaev-Zeldovich effect Virtual Observatory Resource

Authors
  1. Itoh N.
  2. Nozawa S.
  3. Published by
    CDS
Abstract

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.

Keywords
  1. Galaxy clusters
  2. Astronomical models
Bibliographic source Bibcode
2004A&A...417..827I
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/417/827
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/417/827
Document Object Identifer DOI
doi:10.26093/cds/vizier.34170827

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/417/827
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/417/827
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/417/827
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2004-06-08T22:24:15Z
Resource record created
2004-06-08T22:24:15Z
Created
2017-06-21T08:22:12Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr