Sinclaire M. Manning
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View article: An Upper Limit of 10<sup>6</sup> <i>M</i> <sub>⊙</sub> in Dust from ALMA Observations in 60 Little Red Dots
An Upper Limit of 10<sup>6</sup> <i>M</i> <sub>⊙</sub> in Dust from ALMA Observations in 60 Little Red Dots Open
By virtue of their red color, the dust in little red dots (LRDs) has been thought to be of appreciable influence, whether that dust is distributed in a torus around a compact active galactic nucleus or diffuse in the interstellar medium of…
View article: JWST+ALMA reveal the ISM kinematics and stellar structure of MAMBO-9, a merging pair of DSFGs in an overdense environment at $z=5.85$
JWST+ALMA reveal the ISM kinematics and stellar structure of MAMBO-9, a merging pair of DSFGs in an overdense environment at $z=5.85$ Open
We present high-resolution ALMA [CII] 158 micron observations and JWST/NIRCam+MIRI imaging of MAMBO-9, a pair of optically-dark, dusty star-forming galaxies at $z=5.85$. MAMBO-9 is among the most massive, gas-rich, and actively star-formin…
View article: An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots
An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots Open
By virtue of their red color, the dust in little red dots (LRDs) has been thought to be of appreciable influence, whether that dust is distributed in a torus around a compact active galactic nucleus (AGN) or diffuse in the interstellar med…
View article: SCUBADive II: Searching for $z>4$ Dust-Obscured Galaxies via F150W-Dropouts in COSMOS-Web
SCUBADive II: Searching for $z>4$ Dust-Obscured Galaxies via F150W-Dropouts in COSMOS-Web Open
The relative fraction of obscured galaxies at $z>4$ compared to lower redshifts remains highly uncertain as accurate bookkeeping of the dust-obscured component proves difficult. We address this shortcoming with SCUBADive, a compilation of …
View article: RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at <i>z</i> ∼ 2
RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at <i>z</i> ∼ 2 Open
The dearth of high-quality spectroscopy of dusty star-forming galaxies (DSFGs)—the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe—greatly hinders our ability to interpret their physical proces…
View article: SCUBADive. I. JWST+ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web
SCUBADive. I. JWST+ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web Open
JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of submillimeter galaxies, revealing detail that was previously inaccessible. In this work, we construct a sample of 289 submillimeter galax…
View article: The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam Open
We present the PANORAMIC survey, a pure parallel extragalactic imaging program with JWST/NIRCam observed during Cycle 1. The survey obtained ∼530 square arcmin of NIRCam imaging from 1–5 μ m, totaling ∼192 hr of science integration time. T…
View article: Dust in Little Red Dots
Dust in Little Red Dots Open
JWST has revealed a ubiquitous population of “little red dots” (LRDs) at z ≳ 4, selected via their red rest-frame optical emission and compact morphologies. They are thought to be reddened by dust, whether in tori of active galactic nuclei…
View article: RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\sim2$
RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\sim2$ Open
The dearth of high quality spectroscopy of dusty star-forming galaxies (DSFGs) -- the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe -- greatly hinders our ability to interpret their physical …
View article: The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam Open
We present the PANORAMIC survey, a pure parallel extragalactic imaging program with NIRCam observed during JWST Cycle 1. The survey obtained $\sim$530 sq arcmin of NIRCam imaging from 1-5$μ$m, totaling $\sim$192 hours of science integratio…
View article: The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5$σ$ Source Catalog and Redshift Distribution
The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5$σ$ Source Catalog and Redshift Distribution Open
One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At $z>3$, these galaxies are increasingly rare, and difficult to identify…
View article: SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web
SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web Open
JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter gala…
View article: Dust in Little Red Dots
Dust in Little Red Dots Open
JWST has revealed a ubiquitous population of ``little red dots'' (LRDs) at $z\gtrsim4$, selected via their red rest-frame optical emission and compact morphologies. They are thought to be reddened by dust, whether in tori of active galacti…
View article: Uncovering a Massive z ∼ 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
Uncovering a Massive z ∼ 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web Open
In this Letter, we report the discovery of the highest redshift, heavily obscured, radio-loud (RL) active galactic nucleus (AGN) candidate selected using JWST NIRCam/MIRI, mid-IR, submillimeter, and radio imaging in the COSMOS-Web field. U…
View article: A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web
A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web Open
A growing number of far-infrared (FIR) bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z > 4 dusty, star-forming galaxies. Cycle 1 JWST surveys are now detecting their rest-frame o…
View article: Uncovering a Massive z~7.7 Galaxy Hosting a Heavily Obscured Radio-Loud QSO Candidate in COSMOS-Web
Uncovering a Massive z~7.7 Galaxy Hosting a Heavily Obscured Radio-Loud QSO Candidate in COSMOS-Web Open
In this letter, we report the discovery of the highest redshift, heavily obscured, radio-loud AGN candidate selected using JWST NIRCam/MIRI, mid-IR, sub-mm, and radio imaging in the COSMOS-Web field. Using multi-frequency radio observation…
View article: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
COSMOS-Web: An Overview of the JWST Cosmic Origins Survey Open
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg 2 NIRCam imaging survey…
View article: A Near-Infrared Faint, Far-Infrared-Luminous Dusty Galaxy at z~5 in COSMOS-Web
A Near-Infrared Faint, Far-Infrared-Luminous Dusty Galaxy at z~5 in COSMOS-Web Open
A growing number of far-infrared bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z>4 dusty, star-forming galaxies. Cycle 1 JWST surveys are now detecting their rest-frame optical l…
View article: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
COSMOS-Web: An Overview of the JWST Cosmic Origins Survey Open
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg$^2$ NIRCam imaging su…
View article: Probing Cold Gas in a Massive, Compact Star-forming Galaxy at z = 6
Probing Cold Gas in a Massive, Compact Star-forming Galaxy at z = 6 Open
Observations of low-order 12 C 16 O transitions represent the most direct way to study galaxies’ cold molecular gas, the fuel of star formation. Here we present the first detection of CO( J = 2 → 1) in a galaxy lying on the main-sequence o…
View article: Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies
Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies Open
The 2 mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was designed to detect high-redshift ( z ≳ 4), massive, dusty star-forming galaxies (DSFGs). Here we present two likely high-redshift sources, identified in the survey, w…
View article: Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies
Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies Open
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 Mapping Obscuration to Reionization with ALMA (MORA) survey c…
View article: Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies Open
The 2mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was designed to detect high redshift ($z\gtrsim4$), massive, dusty star-forming galaxies (DSFGs). Here we present two, likely high redshift sources, identified in the surv…
View article: The Physical Drivers of the Luminosity-weighted Dust Temperatures in High-redshift Galaxies
The Physical Drivers of the Luminosity-weighted Dust Temperatures in High-redshift Galaxies Open
The underlying distribution of galaxies’ dust spectral energy distributions (SEDs) (i.e., their spectra reradiated by dust from rest-frame ∼3 μ m to 3 mm) remains relatively unconstrained owing to a dearth of far-IR/(sub)millimeter data fo…
View article: The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years
The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years Open
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 contiguous survey to date (184 arcmin(2)) and the only at 2 mm t…
View article: The e-MERLIN SuperCLASS legacy survey : photometric redshifts and characteristics of spatially resolved [mu] Jy radio sources
The e-MERLIN SuperCLASS legacy survey : photometric redshifts and characteristics of spatially resolved [mu] Jy radio sources Open
We present optical and near-infrared imaging covering a ~1.53 deg² region in the Super-Cluster Assisted Shear Survey (SuperCLASS) field, which aims to make the first robust weak lensing measurement at radio wavelengths. We derive photometr…
View article: SuperCLASS – III. Weak lensing from radio and optical observations in Data Release 1
SuperCLASS – III. Weak lensing from radio and optical observations in Data Release 1 Open
We describe the first results on weak gravitational lensing from the SuperCLASS survey: the first survey specifically designed to measure the weak lensing effect in radio-wavelength data, both alone and in cross-correlation with optical da…
View article: SuperCLASS – I. The super cluster assisted shear survey: Project overview and data release 1
SuperCLASS – I. The super cluster assisted shear survey: Project overview and data release 1 Open
The SuperCLuster Assisted Shear Survey (SuperCLASS) is a legacy programme using the e-MERLIN interferometric array. The aim is to observe the sky at L-band (1.4 GHz) to a r.m.s. of $7\, \mu {\rm Jy}\,$beam−1 over an area of $\sim 1\, {\rm …
View article: SuperCLASS – II. Photometric redshifts and characteristics of spatially resolved <i>μ</i>Jy radio sources
SuperCLASS – II. Photometric redshifts and characteristics of spatially resolved <i>μ</i>Jy radio sources Open
We present optical and near-infrared imaging covering a ∼1.53 deg2 region in the Super-Cluster Assisted Shear Survey (SuperCLASS) field, which aims to make the first robust weak lensing measurement at radio wavelengths. We derive photometr…