Andreas Faisst

California Institute of Technology

United States

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Articles (10)

Year:

2022

Year:

2022

Year:

2022

Year:

2022

Year:

2022

Year:

2022

Year:

2021

Year:

2021

Year:

2021

Year:

2020

Collaborators (3)

Nimish Hathi

Space Telescope Science Institute

UNITED STATES

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Michele Ginolfi

Research Assistant Professor

Università degli Studi di Napoli Federico II

ITALY

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Inger Jorgensen

Chief Sustainability Officer

UNITED STATES

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Andreas Faisst

Research Interests

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Articles (10)

The ALPINE-ALMA [C II] survey. Dust attenuation curves at z = 4.4–5.5

What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST

ALPINE: A Large Survey to Understand Teenage Galaxies

Joint Survey Processing. II. Stellar Proper Motions in the COSMOS Field from Hubble Space Telescope ACS and Subaru Telescope HSC Observations

Joint Survey Processing. I. Compact Oddballs in the COSMOS Field—Low-luminosity Quasars at z > 6?

Molecular Gas Excitation of the Massive Dusty Starburst CRLE and the Main-sequence Galaxy HZ10 at z = 5.7 in the COSMOS Field

The ALPINE-ALMA [CII] survey

Illuminating the Dark Side of Cosmic Star Formation Two Billion Years after the Big Bang

The Fundamental Plane of Massive Quiescent Galaxies at z ∼ 2

The ALPINE-ALMA [C II] Survey: [C II] 158 μm Emission Line Luminosity Functions at z ∼ 4–6

Collaborators (3)

Nimish Hathi

Michele Ginolfi

Inger Jorgensen

Make your next move.

Andreas Faisst

Research Interests

Explore related searches

Contact this professor

Articles (10)

The ALPINE-ALMA [C II] survey. Dust attenuation curves at z = 4.4–5.5

What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST

ALPINE: A Large Survey to Understand Teenage Galaxies

Joint Survey Processing. II. Stellar Proper Motions in the COSMOS Field from Hubble Space Telescope ACS and Subaru Telescope HSC Observations

Joint Survey Processing. I. Compact Oddballs in the COSMOS Field—Low-luminosity Quasars at z > 6?

Molecular Gas Excitation of the Massive Dusty Starburst CRLE and the Main-sequence Galaxy HZ10 at z = 5.7 in the COSMOS Field

The ALPINE-ALMA [CII] survey

Illuminating the Dark Side of Cosmic Star Formation Two Billion Years after the Big Bang

The Fundamental Plane of Massive Quiescent Galaxies at z ∼ 2

The ALPINE-ALMA [C II] Survey: [C II] 158 μm Emission Line Luminosity Functions at z ∼ 4–6

Collaborators (3)

Nimish Hathi

Michele Ginolfi

Inger Jorgensen

Make your next move.

The ALPINE-ALMA [C II] survey. Dust attenuation curves at z = 4.4–5.5