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The main sequence of star forming galaxies II. A non evolving slope at the high mass end
P. Popesso, L. Morselli, A. Concas +11
By using the deepest available mid and far infrared surveys in the CANDELS, GOODS and COSMOS fields we study the evolution of the Main Sequence (MS) of star forming galaxies (SFGs)…
Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors
Francesco Valentino, Masayuki Tanaka, Iary Davidzon +18
We report two secure () and one tentative () spectroscopic confirmations of massive and quiescent galaxies through -band observations with Keck/MO…
Bringing manifold learning and dimensionality reduction to SED fitters
Shoubaneh Hemmati, Peter Capak, Milad Pourrahmani +8
We show unsupervised machine learning techniques are a valuable tool for both visualizing and computationally accelerating the estimation of galaxy physical properties from photome…
The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
William I. Cowley, Karina I. Caputi, Smaran Deshmukh +6
In this work, we use measurements of galaxy stellar mass and two-point angular correlation functions to constrain the stellar-to-halo mass ratios (SHMRs) of passive and \np\ galaxi…