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View article: The ALPINE-CRISTAL-JWST survey: Spatially resolved star formation relations at <i>z</i> ∼ 5
The ALPINE-CRISTAL-JWST survey: Spatially resolved star formation relations at <i>z</i> ∼ 5 Open
Context. Star formation governs galaxy evolution, shaping stellar mass assembly and gas consumption across cosmic time. The Kennicutt-Schmidt (KS) relation, linking the star formation rate (SFR) and gas surface densities, is fundamental to…
View article: The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim5$
The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim5$ Open
Star formation governs galaxy evolution, shaping stellar mass assembly and gas consumption across cosmic time. The Kennicutt-Schmidt (KS) relation, linking star formation rate (SFR) and gas surface densities, is fundamental to understand s…
View article: SKYSURF-10: A Novel Method for Measuring Integrated Galaxy Light
SKYSURF-10: A Novel Method for Measuring Integrated Galaxy Light Open
We describe the drizzling pipeline and contents of the drizzled database for Hubble Space Telescope Cycle 27-29 Archival Legacy project "SKYSURF," the largest archival project ever approved for Hubble. SKYSURF aims to investigate the extra…
View article: SKYSURF IX -- The Cosmic Optical and Infrared Background from Integrated Galaxy Light Measurements
SKYSURF IX -- The Cosmic Optical and Infrared Background from Integrated Galaxy Light Measurements Open
As part of the SKYSURF Hubble Space Telescope (HST) Legacy Archival program we present galaxy number counts which yield measurements of the extragalactic background light (EBL) at 15 different wavelengths. We have processed 82,752 HST imag…
View article: The ALMA-CRISTAL Survey: Weak Evidence for Star-formation-driven Outflows in <i>z</i> ∼ 5 Main-sequence Galaxies
The ALMA-CRISTAL Survey: Weak Evidence for Star-formation-driven Outflows in <i>z</i> ∼ 5 Main-sequence Galaxies Open
There is a broad consensus from theory that stellar feedback in galaxies at high redshifts is essential to their evolution, alongside conflicting evidence in the observational literature about its prevalence and efficacy. To this end, we u…
View article: The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ∼ 5.5
The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ∼ 5.5 Open
The ALMA [C II] Resolved Ism in STar-forming gALaxies (CRISTAL) survey is a Cycle 8 ALMA Large Program that studies the cold- gas component of high-redshift galaxies. Its subarcsecond-resolution observations are key to distinguishing physi…
View article: The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ∼ 5.5
The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ∼ 5.5 Open
The ALMA [C II] Resolved Ism in STar-forming gALaxies (CRISTAL) survey is a Cycle 8 ALMA Large Program that studies the cold- gas component of high-redshift galaxies. Its subarcsecond-resolution observations are key to distinguishing physi…
View article: The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ∼1 Gyr old
The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ∼1 Gyr old Open
We present the ALMA-CRISTAL survey, an ALMA Cycle 8 Large Program designed to investigate the physical properties of star-forming galaxies at 4 ≲ z ≲ 6 through spatially resolved, multiwavelength observations. This survey targets 19 star-f…
View article: <i>JWST</i> PRIMER: a lack of outshining in four normal <b> <i>z</i> = 4</b> − <b>6</b> galaxies from the ALMA-CRISTAL Survey
<i>JWST</i> PRIMER: a lack of outshining in four normal <b> <i>z</i> = 4</b> − <b>6</b> galaxies from the ALMA-CRISTAL Survey Open
We present a spatially resolved analysis of four star-forming galaxies at $z = 4.44-5.64$ using data from the JWST Public Release Imaging for Extragalactic Research (PRIMER) and ALMA-[C II] Resolved ISm in STar-forming galaxies with ALma (…
View article: ALESS-JWST: Joint (Sub)kiloparsec JWST and ALMA Imaging of <i>z</i> ~ 3 Submillimeter Galaxies Reveals Heavily Obscured Bulge Formation Events
ALESS-JWST: Joint (Sub)kiloparsec JWST and ALMA Imaging of <i>z</i> ~ 3 Submillimeter Galaxies Reveals Heavily Obscured Bulge Formation Events Open
We present JWST NIRCam imaging targeting 13 z ~ 3 infrared-luminous ( L IR ∼ 5 × 10 12 L ⊙ ) galaxies from the ALESS survey with uniquely deep, high-resolution (0 08–0 16) Atacama Large Millimeter/submillimeter Array 870 μ m im…
View article: The ALMA-CRISTAL Survey
The ALMA-CRISTAL Survey Open
We investigate the spatial extent and structure of the [C II ] line emission in a sample of 34 galaxies at z = 4 − 6 from the [C II ] Resolved ISM in STar-forming galaxies with ALMA (CRISTAL) Survey. By modeling the distribution of the [C …
View article: A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at <i>z</i> = 4.5 revealed by JWST
A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at <i>z</i> = 4.5 revealed by JWST Open
Galaxy protoclusters are sites of rapid growth, with a high density of massive galaxies driving elevated rates of star formation and accretion onto supermassive black holes. Here, we present new JWST/NIRSpec IFU observations of the J1000+0…
View article: The ALMA-CRISTAL Survey: Spatially Resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies
The ALMA-CRISTAL Survey: Spatially Resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies Open
Using a combination of Hubble Space Telescope (HST), JWST, and Atacama Large Millimeter/submillimeter Array (ALMA) data, we perform spatially resolved spectral energy distributions (SED) fitting of fourteen 4 < z < 6 ultraviolet (UV)-selec…
View article: PEARLS: Discovery of Point-source Features within Galaxies in the North Ecliptic Pole Time Domain Field
PEARLS: Discovery of Point-source Features within Galaxies in the North Ecliptic Pole Time Domain Field Open
The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as seen in the longer-wavelength filters. We visually identified a sample of 66 gala…
View article: The ALMA-CRISTAL survey
The ALMA-CRISTAL survey Open
We present the morphological parameters and global properties of dust-obscured star formation in typical star-forming galaxies at z = 4–6. Among 26 galaxies composed of 20 galaxies observed by the Cycle-8 ALMA Large Program, CRISTAL, and 6…
View article: JWST PRIMER: A lack of outshining in four normal z =4-6 galaxies from the ALMA-CRISTAL Survey
JWST PRIMER: A lack of outshining in four normal z =4-6 galaxies from the ALMA-CRISTAL Survey Open
We present a spatially resolved analysis of four star-forming galaxies at $z = 4.44-5.64$ using data from the JWST PRIMER and ALMA-CRISTAL surveys to probe the stellar and inter-stellar medium properties on the sub-kpc scale. In the $1-5\,…
View article: The ALMA-CRISTAL Survey: Spatially-resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies
The ALMA-CRISTAL Survey: Spatially-resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies Open
Using a combination of HST, JWST, and ALMA data, we perform spatially resolved spectral energy distributions (SED) fitting of fourteen 4
View article: The ALMA-CRISTAL Survey: Spatial extent of [CII] line emission in star-forming galaxies at $z=4-6$
The ALMA-CRISTAL Survey: Spatial extent of [CII] line emission in star-forming galaxies at $z=4-6$ Open
We investigate the spatial extent and structure of the [CII] line emission in a sample of 34 galaxies at $z=4-6$ from the ALMA-CRISTAL Survey. By modeling the [CII] line emission in the interferometric visibility, we derive the effective r…
View article: Star Formation, Nebulae, and Active Galactic Nuclei in CLASH Brightest Cluster Galaxies. I. Dependence on Core Entropy of Intracluster Medium
Star Formation, Nebulae, and Active Galactic Nuclei in CLASH Brightest Cluster Galaxies. I. Dependence on Core Entropy of Intracluster Medium Open
We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of the intracluster medium (ICM). Our work is based on the 25 c…
View article: JWST’s PEARLS: Resolved study of the stellar and dust components in starburst galaxies at cosmic noon
JWST’s PEARLS: Resolved study of the stellar and dust components in starburst galaxies at cosmic noon Open
Dusty star-forming galaxies (DSFGs) significantly contribute to the stellar buildup in galaxies during “cosmic noon,” the peak epoch of cosmic star formation. Major mergers and gas accretion are often invoked to explain DSFGs’ prodigious s…
View article: ALESS-JWST: Joint (sub-)kiloparsec JWST and ALMA imaging of $z\sim3$ submillimeter galaxies reveals heavily obscured bulge formation events
ALESS-JWST: Joint (sub-)kiloparsec JWST and ALMA imaging of $z\sim3$ submillimeter galaxies reveals heavily obscured bulge formation events Open
We present JWST NIRCam imaging targeting 13 $z\sim3$ infrared-luminous ($L_{\rm IR}\sim5\times10^{12}L_{\odot}$) galaxies from the ALESS survey with uniquely deep, high-resolution (0.08$''$$-$0.16$''$) ALMA 870$μ$m imaging. The 2.0$-$4.4$μ…
View article: A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST Open
Galaxy protoclusters are sites of rapid growth, with a high density of massive galaxies driving elevated rates of star formation and accretion onto supermassive black holes. Here, we present new JWST/NIRSpec IFU observations of the J1000+0…
View article: Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy
Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy Open
A bright ( m F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, d…
View article: JWST NEP TDF NIRCam
JWST NEP TDF NIRCam Open
The first public 0.9-4.4{\\mu}m NIRCam images of the North Ecliptic Pole (NEP)\nTime Domain Field (TDF) uncovered galaxies displaying point-source features in\ntheir cores as seen in the longer wavelength filters. We visually identified a\…
View article: ProPane: image warping with fire
ProPane: image warping with fire Open
In this paper, we introduce the software package propane, written for the r data analysis language. propane combines the full range of wcslib projections with the C++ image manipulation routines provided by the cimg library. propane offers…
View article: The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6 Open
We present the morphological parameters and global properties of dust-obscured star formation in typical star-forming galaxies at z=4-6. Among 26 galaxies composed of 20 galaxies observed by the Cycle-8 ALMA Large Program, CRISTAL, and six…
View article: ProPane: Image Warping with Fire
ProPane: Image Warping with Fire Open
In this paper we introduce the software package ProPane, written for the R data analysis language. ProPane combines the full range of wcslib projections with the C++ image manipulation routines provided by the CImg library. ProPane offers …
View article: JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results
JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results Open
We give an overview and describe the rationale, methods, and first results from NIRCam images of the JWST “Prime Extragalactic Areas for Reionization and Lensing Science” (PEARLS) project. PEARLS uses up to eight NIRCam filters to survey s…
View article: JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results
JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results Open
We give an overview and describe the rationale, methods, and first results from NIRCam images of the JWST "Prime Extragalactic Areas for Reionization and Lensing Science" ("PEARLS") project. PEARLS uses up to eight NIRCam filters to survey…