Abstract
Large scale flows have been a challenging feature of cosmography ever since galaxy scaling relations came on the scene 40 years ago. The next generation of surveys will offer a serious test of the standard cosmology.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
Notes
http://www.6dfgs.net (Jones et al. 2009).
H. Feldman presented velocity correlation tensor data at the 2016 Large Scale Flows meeting at ICISE.
Based on the density field of Erdoğdu et al. (2006).
For an up to date 3D model see https://skfb.ly/Iy7R by M. Hudson.
References
Ade, P., et al.: Astron. Astrophys. 561, 97 (2014)
Albrecht, A., et al.: astro-ph/0609591 (2006)
Bernyk, M., et al.: Astrophys. J. Suppl. Ser. 223, 9 (2014)
Campbell, L., et al.: Mon. Not. R. Astron. Soc. 443, 1231 (2014)
Carroll, S., et al.: Phys. Rev. D 70, 043528 (2004)
Davis, M., et al.: Mon. Not. R. Astron. Soc. 413, 2906 (2011)
Dressler, A.: ASP Conf. Ser. 15, 19 (1991)
Erdoğdu, P., et al.: Mon. Not. R. Astron. Soc. 373, 45 (2006)
Feldman, H., et al.: Mon. Not. R. Astron. Soc. 407, 2328 (2010)
Johnson, A., et al.: Mon. Not. R. Astron. Soc. 444, 3926 (2014)
Jones, D.H., et al.: Mon. Not. R. Astron. Soc. 399, 683 (2009)
Joyce, A., et al.: Ann. Rev. Nucl. Phys. Sci. 66, 95 (2016)
Kashlinsky, A., et al.: Astrophys. J. 732, 1 (2011)
Kong, X., Su, S.: IAU Symp. 262, 295 (2010)
Kraan-Korteweg, R., et al.: Mon. Not. R. Astron. Soc. 466, L29 (2017)
Lagattuta, D., et al.: Astrophys. J. (2016, in press)
Leclercq, F., et al.: arXiv:1512.02242 (2015)
Ma, Y.-Z., Scott, D.: Astron. Geophys. 55(3), 3.33 (2014)
Magoulas, C. et al.: IAUS 308, 336 (2016)
Moster, B., et al.: Astrophys. J. 710, 903 (2010)
Mould, J.: arXiv:1403.1623 [astro-ph] (2014)
Mould, J., et al.: Astrophys. Space Sci. 357, 162 (2015)
Said, K., et al.: Mon. Not. R. Astron. Soc. 462, 3386 (2016)
Seiler, J., Parkinson, D.: Mon. Not. R. Astron. Soc. 462, 75 (2016)
Springob, C., et al.: Mon. Not. R. Astron. Soc. 456, 1886 (2016)
Tully, R.B.: Astron. J. 149, 171 (2015)
Tully, R.B., et al.: Nature 513, 71 (2014)
Tully, R.B., et al.: Astron. J. 152, 50 (2016)
Acknowledgements
Participants in the recent Large Scale Flows conference would like to thank Roland Triay and ICISE in Vietnam. I acknowledge NEDFootnote 8 and thank Lucas Macri and Pirin Erdoğdu for making data available. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. Data used in this work was generated using Swinburne University’s Theoretical Astrophysical Observatory (TAO). TAO is part of the Australian All-Sky Virtual Observatory (ASVO) and is freely accessible at https://tao.asvo.org.au. The Millennium Simulation was carried out by the Virgo Supercomputing Consortium at the Computing Centre of the Max Planck Society in Garching. It is publicly available at http://www.mpa-garching.mpg.de/Millennium/. The Semi-Analytic Galaxy Evolution (SAGE) model used in this work is a publicly available codebase that runs on the dark matter halo trees of a cosmological N-body simulation. It is available for download at https://github.com/darrencroton/sage.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Mould, J. Modified gravity and large scale flows, a review. Astrophys Space Sci 362, 25 (2017). https://doi.org/10.1007/s10509-017-3005-3
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10509-017-3005-3