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Galactosynthesis predictions at high redshift

Buchalter, Ari and Jimenez, Raul and Kamionkowski, Marc (2001) Galactosynthesis predictions at high redshift. Monthly Notices of the Royal Astronomical Society, 328 (2). pp. 520-526. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200527-135432922

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Abstract

We predict the Tully–Fisher (TF) and surface-brightness–magnitude relations for disc galaxies at z = 3 and discuss the origin of these scaling relations and their scatter. We find that both halo dynamics and the star formation history play important roles, and we show that the variation of the TF relation with redshift can be a potentially powerful discriminator of galaxy-formation models. In particular, the TF relation at high redshift might be used to break parameter degeneracies among galactosynthesis models at z = 0, as well as to constrain the redshift distribution of collapsing dark-matter haloes, the star formation history and baryon fraction in the disc and the distribution of halo spins.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1046/j.1365-8711.2001.04895.xDOIArticle
http://adsabs.harvard.edu/doi/10.1046/j.1365-8711.2001.04895.xADSArticle
https://arxiv.org/abs/astro-ph/0102025arXivDiscussion Paper
ORCID:
AuthorORCID
Kamionkowski, Marc0000-0001-7018-2055
Additional Information:© 2001 RAS. Received: 08 August 2001. Accepted: 08 August 2001. Published: 01 December 2001. We wish to acknowledge C. C. Steidel and K. A. Adelberger for helpful discussions. We also wish to thank the referee, Vladimir A. Avila–Reese, for useful suggestions and comments, specially regarding the M/L ratios of the model. This work was supported by grants NSF-AST-0096023, NSF-AST-9900866, NSF-AST-9618537, NASA NAG5-8506, and DoE DE-FG03-92-ER40701.
Funders:
Funding AgencyGrant Number
NSFAST-0096023
NSFAST-9900866
NSFAST-9618537
NASANAG5-8506
Department of Energy (DOE)DE-FG03-92-ER40701
Subject Keywords:galaxies: formation – galaxies: kinematics and dynamics – galaxies: spiral – cosmology: theory.
Issue or Number:2
Record Number:CaltechAUTHORS:20200527-135432922
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200527-135432922
Official Citation:Ari Buchalter, Raul Jimenez, Marc Kamionkowski, Galactosynthesis predictions at high redshift, Monthly Notices of the Royal Astronomical Society, Volume 328, Issue 2, December 2001, Pages 520–526, https://doi.org/10.1046/j.1365-8711.2001.04895.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103500
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:01 Jun 2020 15:16
Last Modified:01 Jun 2020 15:16

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