activity
20202026
most citedCOMAP Early Science: I. Overview

64 citations · 422 across the 34 of their papers we have counts for

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26 papers · 1 filter

astro-ph.CO2026

Cosmoglobe DR2. VI. Disentangling hot and cold thermal dust emission with Planck HFI

R. M. Sullivan, E. Gjerløw, M. Galloway +20

We present a four-component high-resolution model of thermal dust emission for microwave and sub-mm frequencies derived from Planck HFI, WHAM and Gaia. The resulting high-resolutio…

astro-ph.CO2026

Cosmoglobe DR2. IV. Modelling starlight in DIRBE with Gaia and WISE

M. Galloway, E. Gjerløw, M. San +20

We present a model of starlight emission in the Diffuse Infrared Background Explorer (DIRBE) data between 1.25 and 25m based on \textit{Gaia} and WISE measurements. We include…

astro-ph.CO2026

Cosmoglobe DR2. VII. Towards a concordance model of large-scale thermal dust emission for microwave and infrared frequencies

E. Gjerløw, R. M. Sullivan, R. Aurvik +20

We fit a four-component thermal dust model to COBE-DIRBE data between 3.5 and 240 micron within the global Bayesian end-to-end Cosmoglobe DR2 reanalysis. Following a companion anal…

astro-ph.CO2026

Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBE

E. Gjerløw, R. M. Sullivan, R. Aurvik +20

We fit five tracers of thermal dust emission to ten Planck HFI and COBE-DIRBE frequency maps between 353 GHz and 25 THz, aiming to map the relative importance of each physical host…

astro-ph.CO2025★ 1 cited

COMAP Pathfinder -- Season 2 results IV. A stack on eBOSS/DESI quasars

D. A. Dunne, K. A. Cleary, J. G. S. Lunde +16

We present a stack of data from the second season of the CO Mapping Array Project (COMAP) Pathfinder on the positions of quasars from eBOSS and DESI. COMAP is a Line Intensity Mapp…

astro-ph.CO2025★ 4 cited

Three-Dimensional Stacking as a Line Intensity Mapping Statistic

D. A. Dunne, K. A. Cleary, P. C. Breysse +9

Line-intensity mapping (LIM) is a growing technique that measures the integrated spectral-line emission from unresolved galaxies over a three-dimensional region of the Universe. Al…

astro-ph.CO2024

Cosmoglobe DR2. I. Global Bayesian analysis of COBE-DIRBE

D. J. Watts, M. Galloway, E. Gjerløw +14

We present the first global Bayesian analysis of the time-ordered DIRBE data within the Cosmoglobe framework, building on the same methodology that has previously been successfully…

astro-ph.CO2024

Cosmoglobe DR2. III. Improved modelling of zodiacal light with COBE-DIRBE through global Bayesian analysis

M. San, A. Bonato, M. Galloway +20

We present an improved zodiacal light (ZL) model for COBE-DIRBE derived through global Bayesian analysis within the Cosmoglobe Data Release 2 framework. The parametric form of the…

astro-ph.CO2024★ 4 cited

COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"

D. T. Chung, P. C. Breysse, K. A. Cleary +24

The Carbon monOxide Mapping Array Project (COMAP) Pathfinder survey continues to demonstrate the feasibility of line-intensity mapping using high-redshift carbon monoxide (CO) line…

astro-ph.CO2024★ 5 cited

COMAP Pathfinder -- Season 2 results II. Updated constraints on the CO(1-0) power spectrum

N. -O. Stutzer, J. G. S. Lunde, P. C. Breysse +24

We present updated constraints on the cosmological 3D power spectrum of carbon monoxide CO(1-0) emission in the redshift range -. The constraints are derived from the two…

astro-ph.CO2024★ 7 cited

COMAP Pathfinder -- Season 2 results I. Improved data selection and processing

J. G. S. Lunde, N. -O. Stutzer, P. C. Breysse +24

The CO Mapping Array Project (COMAP) Pathfinder is performing line intensity mapping of CO emission to trace the distribution of unresolved galaxies at redshift . We pres…

astro-ph.CO2024

Cosmoglobe DR2. II. CIB monopole measurements from COBE-DIRBE through global Bayesian analysis

D. J. Watts, M. Galloway, E. Gjerløw +13

We derive new constraints on the CIB monopole spectrum from a set of reprocessed COBE-DIRBE sky maps that have lower instrumental and astrophysical contamination than the legacy DI…

astro-ph.CO2024★ 1 cited

Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking

A. Basyrov, N. O. Stutzer, J. G. S. Lunde +4

We revisit the impact of finite time responses of bolometric detectors used for deep observations of the cosmic microwave background (CMB). Until now, bolometer transfer functions…

astro-ph.CO2023★ 24 cited

LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization

P. Campeti, E. Komatsu, C. Baccigalupi +107

We study the possibility of using the satellite -mode survey to constrain models of inflation producing specific features in CMB angular power spectra. We explore a p…

astro-ph.CO2023★ 5 cited

Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data

D. J. Watts, U. Fuskeland, R. Aurlien +18

We present the first model of full-sky polarized synchrotron emission that is derived from all WMAP and Planck LFI frequency maps. The basis of this analysis is the set of end-to-e…

astro-ph.CO2023★ 2 cited

Cosmoglobe: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations

J. R. Eskilt, K. Lee, D. J. Watts +20

We implement support for a cosmological parameter estimation algorithm as proposed by Racine et al. (2016) in Commander, and quantify its computational efficiency and cost. For a s…

astro-ph.CO2023★ 33 cited

Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data

J. R. Eskilt, D. J. Watts, R. Aurlien +28

Cosmic birefringence is a parity-violating effect that might have rotated the plane of linearly polarized light of the cosmic microwave background (CMB) by an angle since its e…

astro-ph.CO2023★ 17 cited

Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis

D. J. Watts, A. Basyrov, J. R. Eskilt +30

We present Cosmoglobe Data Release 1, which implements the first joint analysis of WMAP and Planck LFI time-ordered data, processed within a single Bayesian end-to-end framework. T…

astro-ph.CO2023★ 23 cited

Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations

U. Fuskeland, J. Aumont, R. Aurlien +114

LiteBIRD is a planned JAXA-led CMB B-mode satellite experiment aiming for launch in the late 2020s, with a primary goal of detecting the imprint of primordial inflationary gravitat…

astro-ph.CO2022★ 24 cited

BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors

K. J. Andersen, D. Herman, R. Aurlien +41

We present the intensity foreground algorithms and model employed within the BeyondPlanck analysis framework. The BeyondPlanck analysis is aimed at integrating component separation…

astro-ph.CO2021★ 64 cited

COMAP Early Science: I. Overview

Kieran A. Cleary, Jowita Borowska, Patrick C. Breysse +40

The CO Mapping Array Project (COMAP) aims to use line intensity mapping of carbon monoxide (CO) to trace the distribution and global properties of galaxies over cosmic time, back t…

astro-ph.CO2021★ 33 cited

COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization

Patrick C. Breysse, Dongwoo T. Chung, Kieran A. Cleary +29

We introduce COMAP-EoR, the next generation of the Carbon Monoxide Mapping Array Project aimed at extending CO intensity mapping to the Epoch of Reionization. COMAP-EoR supplements…

astro-ph.CO2021★ 37 cited

COMAP Early Science: V. Constraints and Forecasts at

Dongwoo T. Chung, Patrick C. Breysse, Kieran A. Cleary +34

We present the current state of models for the carbon monoxide (CO) line-intensity signal targeted by the CO Mapping Array Project (COMAP) Pathfinder in the context of its…

astro-ph.CO2021★ 27 cited

COMAP Early Science: IV. Power Spectrum Methodology and Results

Håvard T. Ihle, Jowita Borowska, Kieran A. Cleary +30

We present the power spectrum methodology used for the first-season COMAP analysis, and assess the quality of the current data set. The main results are derived through the Feed-fe…