Laura Bisigello

University of Padova

Italy

Research Interests

Explore related searches

Professors in Italy Professors in Astronomy Astronomy professors in Italy

Contact this professor

Get a free first email built on one of their papers, ready for you to edit and send yourself.

Articles (10)

Year:

2023

Year:

2023

Year:

2023

Year:

2023

Year:

2022

Year:

2022

Year:

2022

Year:

2022

Year:

2022

Year:

2021

Collaborators (16)

Pablo G. Perez-Gonzalez

Universidad Complutense de Madrid

SPAIN

View details

Nimish Hathi

Space Telescope Science Institute

UNITED STATES

View details

Mikko Pöntinen

University of Helsinki

FINLAND

View details

Benne Willem Holwerda

Associate Professor

University of Louisville

UNITED STATES

View details

Peter Behroozi

University of Arizona

UNITED STATES

View details

Emanuele Daddi

Université Paris-Saclay

FRANCE

View details

Isaac Tutusaus

Astronome adjoint (Associate professor)

FRANCE

View details

DANIELE DALLACASA

Prof.

Università degli Studi di Bologna Dipartimento di Fisica e Astronomia

ITALY

View details

Marc Huertas-Company

Universidad de la Laguna

SPAIN

View details

Ghassem Gozaliasl

Aalto University

FINLAND

View details

Rafael Toledo-Moreo

Universidad Politécnica de Cartagena

SPAIN

View details

Maarten Baes

Professor

Universiteit Gent

BELGIUM

View details

Allan Hornstrup

Technical University of Denmark

DENMARK

View details

G Yang

University of Groningen

NETHERLANDS

View details

Chiara SIRIGNANO

Associate Professor

University of Padua

ITALY

View details

Claudia Maraston

Academic, Professor, Professor of Astrophysics

University of Portsmouth

UNITED KINGDOM

View details

ApplyKite TwinLearns as you apply

Make your next move.

Prepare your application

Review drafts before you send them.

Laura Bisigello

Research Interests

Explore related searches

Contact this professor

Articles (10)

Delving deep: A population of extremely dusty dwarfs observed by JWST

CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts

Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View

Euclid preparation – XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images

A New Estimate of the Cosmic Star Formation Density from a Radio-selected Sample, and the Contribution of H-dark Galaxies at z ≥ 3

A super-linear ‘radio-AGN main sequence’ links mean radio-AGN power and galaxy stellar mass since z ∼ 3

CO in the ALMA Radio-source Catalogue (ARC): The molecular gas content of radio galaxies as a function of redshift

JWST unveils heavily obscured (active and passive) sources up to z ∼ 13

SPRITZ is sparkling: Simulated CO and [C II] luminosities

Simulating the infrared sky with a SPRITZ

Collaborators (16)

Pablo G. Perez-Gonzalez

Nimish Hathi

Mikko Pöntinen

Benne Willem Holwerda

Peter Behroozi

Emanuele Daddi

Isaac Tutusaus

DANIELE DALLACASA

Marc Huertas-Company

Ghassem Gozaliasl

Rafael Toledo-Moreo

Maarten Baes

Allan Hornstrup

G Yang

Chiara SIRIGNANO

Claudia Maraston

Make your next move.

Laura Bisigello

Research Interests

Explore related searches

Contact this professor

Articles (10)

Delving deep: A population of extremely dusty dwarfs observed by JWST

CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts

Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View

Euclid preparation – XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images

A New Estimate of the Cosmic Star Formation Density from a Radio-selected Sample, and the Contribution of H-dark Galaxies at z ≥ 3

A super-linear ‘radio-AGN main sequence’ links mean radio-AGN power and galaxy stellar mass since z ∼ 3

CO in the ALMA Radio-source Catalogue (ARC): The molecular gas content of radio galaxies as a function of redshift

JWST unveils heavily obscured (active and passive) sources up to z ∼ 13

SPRITZ is sparkling: Simulated CO and [C II] luminosities

Simulating the infrared sky with a SPRITZ

Collaborators (16)

Pablo G. Perez-Gonzalez

Nimish Hathi

Mikko Pöntinen

Benne Willem Holwerda

Peter Behroozi

Emanuele Daddi

Isaac Tutusaus

DANIELE DALLACASA

Marc Huertas-Company

Ghassem Gozaliasl

Rafael Toledo-Moreo

Maarten Baes

Allan Hornstrup

G Yang

Chiara SIRIGNANO

Claudia Maraston

Make your next move.

SPRITZ is sparkling: Simulated CO and [C II] luminosities