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Quasars and the intergalactic medium at cosmic dawn
Quasars at cosmic dawn provide powerful probes of the formation and growth of the earliest
supermassive black holes (SMBHs) in the Universe, their connections to galaxy and …
supermassive black holes (SMBHs) in the Universe, their connections to galaxy and …
New insights into the evolution of massive stars and their effects on our understanding of early galaxies
The observable characteristics and subsequent evolution of young stellar populations is
dominated by their massive stars. As our understanding of those massive stars and the …
dominated by their massive stars. As our understanding of those massive stars and the …
Hidden little monsters: spectroscopic identification of low-mass, broad-line AGNs at z> 5 with CEERS
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 …
z> 5 identified using JWST NIRSpec spectroscopy from the Cosmic Evolution Early Release …
CEERS key paper. I. An early look into the first 500 Myr of galaxy formation with JWST
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 …
Evolution Early Release Science (CEERS) survey. CEERS, one of 13 JWST ERS programs …
Little red dots: an abundant population of faint active galactic nuclei at z∼ 5 revealed by the EIGER and FRESCO JWST surveys
Characterizing the prevalence and properties of faint active galactic nuclei (AGNs) in the
early Universe is key for understanding the formation of supermassive black holes (SMBHs) …
early Universe is key for understanding the formation of supermassive black holes (SMBHs) …
Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z≃ 8–10
We present JWST/NIRSpec prism spectroscopy of seven galaxies selected from Cosmic
Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric …
Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric …
The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging
We reduce and analyse the available JWST ERO and ERS NIRCam imaging (SMACS0723,
GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in …
GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in …
Most of the photons that reionized the Universe came from dwarf galaxies
The identification of sources driving cosmic reionization, a major phase transition from
neutral hydrogen to ionized plasma around 600–800 Myr after the Big Bang,–, has been a …
neutral hydrogen to ionized plasma around 600–800 Myr after the Big Bang,–, has been a …
Early results from GLASS-JWST. III. Galaxy candidates at z∼ 9–15
M Castellano, A Fontana, T Treu… - The Astrophysical …, 2022 - iopscience.iop.org
We present the results of a first search for galaxy candidates at z∼ 9–15 on deep seven-
band NIRCam imaging acquired as part of the GLASS-James Webb Space Telescope …
band NIRCam imaging acquired as part of the GLASS-James Webb Space Telescope …
The complete CEERS early universe galaxy sample: a surprisingly slow evolution of the space density of bright galaxies at z∼ 8.5–14.5
We present a sample of 88 candidate z∼ 8.5–14.5 galaxies selected from the completed
NIRCam imaging from the Cosmic Evolution Early Release Science survey. These data …
NIRCam imaging from the Cosmic Evolution Early Release Science survey. These data …