Papers

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2017 Alison L. Coil

, Alexander J. Mendez

, Daniel J. Eisenstein, John Moustakas

PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2

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Angela M. Berti

, Alison L. Coil

, Peter S. Behroozi

, Daniel J. Eisenstein, Aaron D. Bray, Richard J. Cool, John Moustakas

Primus: One- And Two-Halo Galactic Conformity at 0.2

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2016 Mariska Kriek, Charlie Conroy, Pieter G. van Dokkum, Alice E. Shapley, Jieun Choi

, Naveen A. Reddy, Brian Siana, Freeke van de Voort

, Alison L. Coil, Bahram Mobasher

A massive, quiescent, population II galaxy at a redshift of 2.1

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Aleksandar M. Diamond-Stanic, Alison L. Coil

, John Moustakas

, Christy A. Tremonti, Paul H. Sell, Alexander J. Mendez

, Ryan C. Hickox

, Greg H. Rudnick

GALAXIES PROBING GALAXIES AT HIGH RESOLUTION: CO-ROTATING GAS ASSOCIATED WITH a MILKY WAY ANALOG ATz= 0.4

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Alexander J. Mendez

, Alison L. Coil

, James Aird

, Ramin A. Skibba, Aleksandar M. Diamond-Stanic, John Moustakas

, Michael R. Blanton, Richard J. Cool, Daniel J. Eisenstein, Kenneth C. Wong

, Guangtun Zhu

PRIMUS + DEEP2: CLUSTERING OF X-Ray, RADIO, AND IR-AGNs ATz∼ 0.7

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Sedona H. Price

, Mariska Kriek, Alice E. Shapley, Naveen A. Reddy, William R. Freeman, Alison L. Coil, Laura de Groot, Irene Shivaei, Brian Siana, Mojegan Azadi, Guillermo Barro, Bahram Mobasher, Ryan L. Sanders, Tom Zick

The MOSDEF SURVEY: DYNAMICAL AND BARYONIC MASSES AND KINEMATIC STRUCTURES OF STAR-FORMING GALAXIES AT 1.4 ≤z≤ 2.6

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2015 Ryan L. Sanders, Alice E. Shapley, Mariska Kriek, Naveen A. Reddy, William R. Freeman, Alison L. Coil, Brian Siana, Bahram Mobasher, Irene Shivaei, Sedona H. Price

, Laura de Groot

The MOSDEF SURVEY: ELECTRON DENSITY AND IONIZATION PARAMETER ATz∼ 2.3

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Mirko Krumpe, Takamitsu Miyaji

, Bernd Husemann, Nikos Fanidakis

, Alison L. Coil

, Hector Aceves

The Spatial Clustering Ofrosatall-Sky Survey Active Galactic Nuclei. Iv. More Massive Black Holes Reside in More Massive Dark Matter Halos

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Aaron D. Bray, Daniel J. Eisenstein, Ramin A. Skibba, Michael R. Blanton, Alison L. Coil

, Richard J. Cool, Alexander J. Mendez

, John Moustakas

, Guangtun Zhu

Primus: The Effect of Physical Scale on the Luminosity Dependence of Galaxy Clustering via Cross-Correlations

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Ramin A. Skibba, Alison L. Coil

, Alexander J. Mendez

, Michael R. Blanton, Aaron D. Bray, Richard J. Cool, Daniel J. Eisenstein, Hong Guo

, Takamitsu Miyaji

, John Moustakas

, Guangtun Zhu

Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in Primus+deep2 at 0.2

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Naveen A. Reddy, Mariska Kriek

, Alice E. Shapley, William R. Freeman, Brian Siana

, Alison L. Coil

, Bahram Mobasher, Sedona H. Price

, Ryan L. Sanders, Irene Shivaei

The MOSDEF SURVEY: MEASUREMENTS OF BALMER DECREMENTS AND THE DUST ATTENUATION CURVE AT REDSHIFTSz∼ 1.4–2.6

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Mojegan Azadi

, James Aird, Alison L. Coil

, John Moustakas

, Alexander J. Mendez

, Michael R. Blanton, Richard J. Cool, Daniel J. Eisenstein, Kenneth C. Wong

, Guangtun Zhu

Primus: The Relationship Between Star Formation and Agn Accretion

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ChangHoon Hahn

, Michael R. Blanton, John Moustakas, Alison L. Coil

, Richard J. Cool, Daniel J. Eisenstein, Ramin A. Skibba, Kenneth C. Wong, Guangtun Zhu

PRIMUS: EFFECTS OF GALAXY ENVIRONMENT ON THE QUIESCENT FRACTION EVOLUTION ATz< 0.8

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This paper was not found in any repository; the policy of its publisher is unknown or unclear.

ChangHoon Hahn, Michael R. Blanton, John Moustakas

, Alison L. Coil, Richard J. Cool, Daniel J. Eisenstein, Ramin A. Skibba, Kenneth C. Wong, Guangtun Zhu

PRIMUS: Effects of Galaxy Environment on the Quiescent Fraction Evolution at z 〈 0.8

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Mariska Kriek

, Alice E. Shapley, Naveen A. Reddy, Brian Siana

, Alison L. Coil, Bahram Mobasher, William R. Freeman, Laura de Groot, Sedona H. Price, Ryan Sanders, Irene Shivaei

, Gabriel B. Brammer

, Ivelina G. Momcheva, Rosalind E. Skelton

, Pieter G. van Dokkum

and 9 other authors

The MOSFIRE DEEP EVOLUTION FIELD (MOSDEF) SURVEY: REST-FRAME OPTICAL SPECTROSCOPY FOR ∼1500 H -SELECTED GALAXIES AT $1.37⩽ Z⩽ 3.8$

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