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Andreas L. Faisst
Researcher at California Institute of Technology
Publications - 154
Citations - 6086
Andreas L. Faisst is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 40, co-authored 126 publications receiving 4648 citations. Previous affiliations of Andreas L. Faisst include École Polytechnique Fédérale de Lausanne.
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Journal ArticleDOI
The COSMOS2015 galaxy stellar mass function . Thirteen billion years of stellar mass assembly in ten snapshots
I. Davidzon,I. Davidzon,O. Ilbert,Clotilde Laigle,Jean Coupon,H. J. McCracken,Ivan Delvecchio,D. Masters,Peter Capak,Bau-Ching Hsieh,O. Le Fevre,L. Tresse,Matthieu Béthermin,Yu-Yen Chang,Yu-Yen Chang,Andreas L. Faisst,E. Le Floc'h,Charles L. Steinhardt,Sune Toft,Herve Aussel,C. Dubois,G. Hasinger,Mara Salvato,D. B. Sanders,Nick Scoville,John D. Silverman +25 more
TL;DR: In this paper, the stellar mass function (SMF) and stellar mass density of galaxies in the COSMOS field up to 6.5 were measured with a Schechter function, correcting for Eddington bias.
Journal ArticleDOI
The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
I. Davidzon,Mara Salvato,Yu-Yen Chang,Charles L. Steinhardt,S. Toft,Peter Capak,O. Le Fevre,John D. Silverman,Ivan Delvecchio,M. Bethermin,C. Laigle,D. Masters,L. Tresse,G. Hasinger,Nick Scoville,C. Dubois,E. Le Floc'h,H. Aussel,Jean Coupon,Andreas L. Faisst,H. J. McCracken,O. Ilbert,D. B. Sanders,Bau-Ching Hsieh +23 more
TL;DR: In this article, the stellar mass function (SMF) of galaxies in the COSMOS field up to 2.5 was measured using a Schechter function, correcting for Eddington bias.
Journal ArticleDOI
Evolution of Galaxies and their Environments at z = 0.1 to 3 in COSMOS
Nick Scoville,Stephane Arnouts,H. Aussel,Andrew J. Benson,Angela Bongiorno,Kevin Bundy,M. A. A. Calvo,Peter Capak,Marcella Carollo,Francesca Civano,James Dunlop,M. Elvis,Andreas L. Faisst,A. Finoguenov,Hai Fu,M. Giavalisco,Qi Guo,Olivier Ilbert,A. Iovino,Masaru Kajisawa,J. Kartaltepe,A. Leauthaud,O. Le Fe`vre,E. LeFloch,S. J. Lilly,C. T-C. Liu,S. Manohar,Richard Massey,D. Masters,H. J. McCracken,Bahram Mobasher,Y. Peng,Alvio Renzini,Jason Rhodes,Mara Salvato,D. B. Sanders,B. D. Sarvestani,Claudia Scarlata,Eva Schinnerer,Kartik Sheth,Patrick L. Shopbell,V. Smolcic,Y. Taniguchi,James E. Taylor,Simon D. M. White,Lin Yan +45 more
TL;DR: In this paper, the star formation rate density (SFRD) is uniformly distributed over all environmental density percentiles, while at lower redshifts the dominant contribution is shifted to galaxies in lower density environments.
Journal ArticleDOI
The Effects of the Local Environment and Stellar Mass on Galaxy Quenching to z ~ 3
Behnam Darvish,Behnam Darvish,Bahram Mobasher,David Sobral,David Sobral,David Sobral,Alessandro Rettura,Nick Scoville,Andreas L. Faisst,Peter Capak +9 more
TL;DR: In this article, the effects of the local environment and stellar mass on galaxy properties using a mass complete sample of quiescent and star-forming systems in the COSMOS field at z ≾ 3.
Journal ArticleDOI
Mapping the galaxy color-redshift relation: optimal photometric redshift calibration strategies for cosmology surveys
Daniel Masters,Peter Capak,Daniel Stern,Olivier Ilbert,Mara Salvato,Samuel Schmidt,Giuseppe Longo,Jason Rhodes,Jason Rhodes,Stéphane Paltani,Bahram Mobasher,Henk Hoekstra,Hendrik Hildebrandt,Jean Coupon,Charles L. Steinhardt,Josh S. Speagle,Andreas L. Faisst,Adam Kalinich,Mark Brodwin,Massimo Brescia,Stefano Cavuoti +20 more
TL;DR: In this article, a self-organizing map is proposed to map the distribution of data in a high-dimensional space and projecting it onto a lower-dimensional representation, which can be used to estimate the additional spectroscopy needed to map out the color-redshift relation.