publication . Preprint . Article . 2018

COFFE: a code for the full-sky relativistic galaxy correlation function

Camille Bonvin; Ruth Durrer;
Open Access English
  • Published: 18 Oct 2018
Abstract
Comment: Code available at https://github.com/JCGoran/coffe
Subjects
arXiv: Astrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: Astrophysics - Cosmology and Nongalactic Astrophysics, Astronomy and Astrophysics
60 references, page 1 of 4

[1] D. H. Jones et al., “The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures,” Mon. Not. Roy. Astron. Soc. 399 (2009) 683, arXiv:0903.5451 [astro-ph.CO].

[2] T. Davis, C. Blake, D. Parkinson, S. Riemer-Sørensen, G. B. Poole, M. Scrimgeour, E. Kazin, F. Beutler, K. Glazebrook, M. Drinkwater, W. Couch, and WiggleZ Dark Energy Survey Team, “The WiggleZ Dark Energy Survey: Final Results,” in American Astronomical Society Meeting Abstracts #221, vol. 221 of American Astronomical Society Meeting Abstracts, p. 106.02. Jan., 2013.

[3] S. Alam, F. D. Albareti, C. Allende Prieto, F. Anders, S. F. Anderson, T. Anderton, B. H. Andrews, E. Armengaud, É. Aubourg, S. Bailey, and et al., “The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III,” ApJS 219 (July, 2015) 12, arXiv:1501.00963 [astro-ph.IM].

[4] F. D. Albareti, C. Allende Prieto, A. Almeida, F. Anders, S. Anderson, B. H. Andrews, A. Aragón-Salamanca, M. Argudo-Fernández, E. Armengaud, E. Aubourg, and et al., “The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory,” ApJS 233 (Dec., 2017) 25, arXiv:1608.02013.

[5] R. Laureijs, J. Amiaux, S. Arduini, J. . Auguères, J. Brinchmann, R. Cole, M. Cropper, C. Dabin, L. Duvet, A. Ealet, and et al., “Euclid Definition Study Report,” ArXiv e-prints (Oct., 2011) , arXiv:1110.3193 [astro-ph.CO].

[6] SKA Cosmology SWG Collaboration, R. Maartens, F. B. Abdalla, M. Jarvis, and M. G. Santos, “Overview of Cosmology with the SKA,” PoS AASKA14 (2015) 016, arXiv:1501.04076 [astro-ph.CO].

[7] Planck Collaboration, R. Adam et al., “Planck 2015 results. I. Overview of products and scientific results,” Astron. Astrophys. 594 (2016) A1, arXiv:1502.01582 [astro-ph.CO].

[8] Planck Collaboration, P. A. R. Ade et al., “Planck 2015 results. XIII. Cosmological parameters,” Astron. Astrophys. 594 (2016) A13, arXiv:1502.01589 [astro-ph.CO].

[9] A. Lewis, A. Challinor, and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys.J. 538 (2000) 473-476, arXiv:astro-ph/9911177 [astro-ph]. [OpenAIRE]

[10] D. Blas, J. Lesgourgues, and T. Tram, “The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes,” JCAP 1107 (2011) 034, arXiv:1104.2933 [astro-ph.CO]. [OpenAIRE]

[11] A. Challinor and A. Lewis, “Linear power spectrum of observed source number counts,” Phys. Rev. D 84 no. 4, (Aug., 2011) 043516, arXiv:1105.5292 [astro-ph.CO].

[12] E. Di Dio, F. Montanari, J. Lesgourgues, and R. Durrer, “The CLASSgal code for Relativistic Cosmological Large Scale Structure,” JCAP 1311 (2013) 044, arXiv:1307.1459 [astro-ph.CO]. [OpenAIRE]

[13] J. Yoo, A. L. Fitzpatrick, and M. Zaldarriaga, “New perspective on galaxy clustering as a cosmological probe: General relativistic effects,” Phys. Rev. D 80 no. 8, (Oct., 2009) 083514, arXiv:0907.0707 [astro-ph.CO].

[14] C. Bonvin and R. Durrer, “What galaxy surveys really measure,” Phys. Rev. D84 (2011) 063505, arXiv:1105.5280 [astro-ph.CO]. [OpenAIRE]

[15] A. Challinor and A. Lewis, “The linear power spectrum of observed source number counts,” Phys.Rev. D84 (2011) 043516, arXiv:1105.5292 [astro-ph.CO].

60 references, page 1 of 4
Abstract
Comment: Code available at https://github.com/JCGoran/coffe
Subjects
arXiv: Astrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: Astrophysics - Cosmology and Nongalactic Astrophysics, Astronomy and Astrophysics
60 references, page 1 of 4

[1] D. H. Jones et al., “The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures,” Mon. Not. Roy. Astron. Soc. 399 (2009) 683, arXiv:0903.5451 [astro-ph.CO].

[2] T. Davis, C. Blake, D. Parkinson, S. Riemer-Sørensen, G. B. Poole, M. Scrimgeour, E. Kazin, F. Beutler, K. Glazebrook, M. Drinkwater, W. Couch, and WiggleZ Dark Energy Survey Team, “The WiggleZ Dark Energy Survey: Final Results,” in American Astronomical Society Meeting Abstracts #221, vol. 221 of American Astronomical Society Meeting Abstracts, p. 106.02. Jan., 2013.

[3] S. Alam, F. D. Albareti, C. Allende Prieto, F. Anders, S. F. Anderson, T. Anderton, B. H. Andrews, E. Armengaud, É. Aubourg, S. Bailey, and et al., “The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III,” ApJS 219 (July, 2015) 12, arXiv:1501.00963 [astro-ph.IM].

[4] F. D. Albareti, C. Allende Prieto, A. Almeida, F. Anders, S. Anderson, B. H. Andrews, A. Aragón-Salamanca, M. Argudo-Fernández, E. Armengaud, E. Aubourg, and et al., “The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory,” ApJS 233 (Dec., 2017) 25, arXiv:1608.02013.

[5] R. Laureijs, J. Amiaux, S. Arduini, J. . Auguères, J. Brinchmann, R. Cole, M. Cropper, C. Dabin, L. Duvet, A. Ealet, and et al., “Euclid Definition Study Report,” ArXiv e-prints (Oct., 2011) , arXiv:1110.3193 [astro-ph.CO].

[6] SKA Cosmology SWG Collaboration, R. Maartens, F. B. Abdalla, M. Jarvis, and M. G. Santos, “Overview of Cosmology with the SKA,” PoS AASKA14 (2015) 016, arXiv:1501.04076 [astro-ph.CO].

[7] Planck Collaboration, R. Adam et al., “Planck 2015 results. I. Overview of products and scientific results,” Astron. Astrophys. 594 (2016) A1, arXiv:1502.01582 [astro-ph.CO].

[8] Planck Collaboration, P. A. R. Ade et al., “Planck 2015 results. XIII. Cosmological parameters,” Astron. Astrophys. 594 (2016) A13, arXiv:1502.01589 [astro-ph.CO].

[9] A. Lewis, A. Challinor, and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys.J. 538 (2000) 473-476, arXiv:astro-ph/9911177 [astro-ph]. [OpenAIRE]

[10] D. Blas, J. Lesgourgues, and T. Tram, “The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes,” JCAP 1107 (2011) 034, arXiv:1104.2933 [astro-ph.CO]. [OpenAIRE]

[11] A. Challinor and A. Lewis, “Linear power spectrum of observed source number counts,” Phys. Rev. D 84 no. 4, (Aug., 2011) 043516, arXiv:1105.5292 [astro-ph.CO].

[12] E. Di Dio, F. Montanari, J. Lesgourgues, and R. Durrer, “The CLASSgal code for Relativistic Cosmological Large Scale Structure,” JCAP 1311 (2013) 044, arXiv:1307.1459 [astro-ph.CO]. [OpenAIRE]

[13] J. Yoo, A. L. Fitzpatrick, and M. Zaldarriaga, “New perspective on galaxy clustering as a cosmological probe: General relativistic effects,” Phys. Rev. D 80 no. 8, (Oct., 2009) 083514, arXiv:0907.0707 [astro-ph.CO].

[14] C. Bonvin and R. Durrer, “What galaxy surveys really measure,” Phys. Rev. D84 (2011) 063505, arXiv:1105.5280 [astro-ph.CO]. [OpenAIRE]

[15] A. Challinor and A. Lewis, “The linear power spectrum of observed source number counts,” Phys.Rev. D84 (2011) 043516, arXiv:1105.5292 [astro-ph.CO].

60 references, page 1 of 4
Powered by OpenAIRE Research Graph
Any information missing or wrong?Report an Issue