CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 &lt;<i>z</i>&lt; 2.5

E. Whitaker, Katherine; Franx, Marijn; Leja, Joel; van Dokkum, Pieter; Henry, Alaina; E. Skelton, Rosalind; Fumagalli, Mattia; Momcheva, Ivelina; Brammer, Gabriel; Labbé, Ivo; J. Nelson, Erica; R. Rigby, Jane

doi:10.1088/0004-637x/795/2/104

Public

CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 <<i>z</i>< 2.5

Shared by NobleBlocks on Oct 17, 2014 • 12:00 AM UTC

Authors:

Katherine E. Whitaker

Marijn Franx

Joel Leja

Abstract

We constrain the slope of the star formation rate (SFR; log Ψ) to stellar mass (log M ∗) relation down to log (M ∗/M⊙) = 8.4 (log (M ∗/M⊙) = 9.2) at z = 0.5 (z = 2.5) with a mass-complete sample of 39,106 star-forming galaxies selected from the 3D-HST photometric catalogs, using deep photometry in t...

Subject

Physics

Astrophysics

Galaxy

Research Assistant

AI chat, annotations, notes & similar papers

Finding related papers...

Discussions

(0)

No comments yet

Be the first to share your thoughts!