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Redshift measurement through star formation

Lindholmer, Mikkel O.; Pimbblet, Kevin A.

Authors

Mikkel O. Lindholmer



Abstract

© ESO 2019. In this work we use the property that, on average, star formation rate increases with redshift for objects with the same mass - the so called galaxy main sequence - to measure the redshift of galaxy clusters. We use the fact that the general galaxy population forms both a quenched and a star-forming sequence, and we locate these ridges in the SFR-M⋆ plane with galaxies taken from the Sloan Digital Sky Survey in discrete redshift bins. We fitted the evolution of the galaxy main sequence with redshift using a new method and then subsequently apply our method to a suite of X-ray selected galaxy clusters in an attempt to create a new distance measurement to clusters based on their galaxy main sequence. We demonstrate that although it is possible in several galaxy clusters to measure the main sequences, the derived distance and redshift from our galaxy main sequence fitting technique has an accuracy of σz  =  ±0.017 ⋅  (z  +  1) and is only accurate up to z  ≈  0.2.

Journal Article Type Article
Publication Date Aug 23, 2019
Journal Astronomy and Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 629
Article Number A7
APA6 Citation Lindholmer, M. O., & Pimbblet, K. A. (2019). Redshift measurement through star formation. Astronomy and Astrophysics, 629, https://doi.org/10.1051/0004-6361/201833046
DOI https://doi.org/10.1051/0004-6361/201833046
Keywords methods: observational; galaxies: clusters: general

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