Göran Östlin

Stockholm University

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Articles (18)

Collaborators (8)

Rachel Somerville

Harvard-Smithsonian Center for Astrophysics

UNITED STATES

Thomas R. Greve

Technical University of Denmark

Pablo G. Perez-Gonzalez

Universidad Complutense de Madrid

John Cannon

Professor of Astronomy

Macalester College

UNITED STATES

M. S. Oey

University of Michigan

UNITED STATES

Edmund Hodges-Kluck

University of Michigan

UNITED STATES

Steven L Finkelstein

University of Texas at Austin

UNITED STATES

Steven Gillman

Technical University of Denmark

Göran Östlin

Research Interests

Explore related searches

Contact this professor

Articles (18)

Collaborators (8)

Rachel Somerville

Thomas R. Greve

Pablo G. Perez-Gonzalez

John Cannon

M. S. Oey

Edmund Hodges-Kluck

Steven L Finkelstein

Steven Gillman

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Göran Östlin

Research Interests

Explore related searches

Contact this professor

Articles (18)

The Rise of the Galactic Empire: Ultraviolet Luminosity Functions at z ∼ 17 and z ∼ 25 Estimated with the MIDIS+NGDEEP Ultra-deep JWST/NIRCam Data Set

FEAST: JWST/NIRCam View of the Resolved Stellar Populations of the Interacting Dwarf Galaxies NGC 4485 and NGC 4490

Spatially resolved Hα emission in B14-65666: Compact starbursts, ionizing efficiency, and gas kinematics in an advanced merger at the Epoch of Reionization

MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field

The Emergence of the Star Formation Main Sequence with Redshift Unfolded by JWST

The Lyman Alpha Reference Sample

The Lyman alpha reference sample

Haro 11: The Spatially Resolved Lyman Continuum Sources

Disentangling the X-ray variability in the Lyman continuum emitter Haro 11

MIDIS: JWST/MIRI Reveals the Stellar Structure of ALMA-selected Galaxies in the Hubble Ultra Deep Field at Cosmic Noon

MIDIS: The Relation between Strong (Hβ + [O iii]) Emission, Star Formation, and Burstiness around the Epoch of Reionization

MIDIS: Unveiling the Role of Strong Hα Emitters During the Epoch of Reionization with JWST

A mature quasar at cosmic dawn revealed by JWST rest-frame infrared spectroscopy

MIDIS: JWST NIRCam and MIRI Unveil the Stellar Population Properties of Lyα Emitters and Lyman-break Galaxies at z ≃ 3–7

JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at z = 4.05

MIDIS: Strong (Hβ+[O iii]) and Hα Emitters at Redshift z ≃ 7–8 Unveiled with JWST NIRCam and MIRI Imaging in the Hubble eXtreme Deep Field

Life beyond 30: Probing the −20 < M UV < −17 Luminosity Function at 8 < z < 13 with the NIRCam Parallel Field of the MIRI Deep Survey

The Lyα Reference Sample. XIV. Lyα Imaging of 45 Low-redshift Star-forming Galaxies and Inferences on Global Emission

Collaborators (8)

Rachel Somerville

Thomas R. Greve

Pablo G. Perez-Gonzalez

John Cannon

M. S. Oey

Edmund Hodges-Kluck

Steven L Finkelstein

Steven Gillman

How do I reach out?

Meet Kite AI