CEERS key paper. I. An early look into the first 500 Myr of galaxy formation with JWST

SL Finkelstein, MB Bagley, HC Ferguson… - The Astrophysical …, 2023 - iopscience.iop.org
We present an investigation into the first 500 Myr of galaxy evolution from the Cosmic
Evolution Early Release Science (CEERS) survey. CEERS, one of 13 JWST ERS programs …

Hidden little monsters: spectroscopic identification of low-mass, broad-line AGNs at z> 5 with CEERS

DD Kocevski, M Onoue, K Inayoshi… - The Astrophysical …, 2023 - iopscience.iop.org
We report on the discovery of two low-luminosity, broad-line active galactic nuclei (AGNs) at
z> 5 identified using JWST NIRSpec spectroscopy from the Cosmic Evolution Early Release …

The art of measuring physical parameters in galaxies: a critical assessment of spectral energy distribution fitting techniques

C Pacifici, KG Iyer, B Mobasher… - The Astrophysical …, 2023 - iopscience.iop.org
The study of galaxy evolution hinges on our ability to interpret multiwavelength galaxy
observations in terms of their physical properties. To do this, we rely on spectral energy …

A dusty compact object bridging galaxies and quasars at cosmic dawn

S Fujimoto, GB Brammer, D Watson, GE Magdis… - Nature, 2022 - nature.com
Understanding how super-massive black holes form and grow in the early Universe has
become a major challenge, since it was discovered that luminous quasars existed only 700 …

The evolution of the IR luminosity function and dust-obscured star formation over the past 13 billion years

JA Zavala, CM Casey, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the first results from the Mapping Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …

The ALPINE-ALMA [CII] survey-The nature, luminosity function, and star formation history of dusty galaxies up to z≃ 6

C Gruppioni, M Béthermin, F Loiacono… - Astronomy & …, 2020 - aanda.org
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …

The [C ii] emission as a molecular gas mass tracer in galaxies at low and high redshifts

A Zanella, E Daddi, G Magdis… - Monthly Notices of …, 2018 - academic.oup.com
We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …

The CANDELS/SHARDS multiwavelength catalog in GOODS-N: photometry, photometric redshifts, stellar masses, emission-line fluxes, and star formation rates

G Barro, PG Pérez-González, A Cava… - The Astrophysical …, 2019 - iopscience.iop.org
We present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field
containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts …

The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to z∼ 5

SK Leslie, E Schinnerer, D Liu, B Magnelli… - The Astrophysical …, 2020 - iopscience.iop.org
The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies

CM Casey, JA Zavala, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …