output
20092026
most citedJADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty

361 citations

Showing astro-ph.COShow all

14 papers · 1 filter

astro-ph.CO2026

Cluster number counts in dark energy model with energy and momentum coupling to dark matter

Chattree Wongsangwal, Khamphee Karwan, Stharporn Sapa +1

The influences on the cluster number counts from the coupling between dark energy and dark matter with momentum transfer are investigated. We find that the extrapolated linear dens…

astro-ph.CO2024★ 1 cited

A novel analysis of contamination in Lyman-break galaxy samples at : spatial correlation with intermediate-redshift galaxies at

Miftahul Hilmi, Nicha Leethochawalit, Michele Trenti +1

Potential contamination from low/intermediate-redshift galaxies, such as objects with a prominent Balmer break, affects the photometric selection of high-redshift galaxies through…

astro-ph.CO2024★ 10 cited

Exploration of the polarization angle variability of the Crab Nebula with POLARBEAR and its application to the search for axion-like particles

Shunsuke Adachi, Tylor Adkins, Carlo Baccigalupi +23

The Crab Nebula, also known as Tau A, is a polarized astronomical source at millimeter wavelengths. It has been used as a stable light source for polarization angle calibration in…

astro-ph.CO2023★ 5 cited

Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation

Piyabut Burikham, Teeraparb Chantavat, Pongsapat Boonaom

We present constraints on the extended Starobinsky and Weyl gravity model of inflation using updated available observational data. The data includes cosmic microwave background (CM…

astro-ph.CO2023★ 19 cited

Constraints on axion-like polarization oscillations in the cosmic microwave background with POLARBEAR

The POLARBEAR Collaboration, Shunsuke Adachi, Tylor Adkins +29

Very light pseudoscalar fields, often referred to as axions, are compelling dark matter candidates and can potentially be detected through their coupling to the electromagnetic fie…

astro-ph.CO2022★ 28 cited

Improved upper limit on degree-scale CMB B-mode polarization power from the 670 square-degree POLARBEAR survey

The POLARBEAR Collaboration, S. Adachi, T. Adkins +51

We report an improved measurement of the degree-scale cosmic microwave background -mode angular-power spectrum over 670 square-degree sky area at 150 GHz with POLARBEAR. In the…

astro-ph.CO2021

Primordial gravitational waves from excited states

Jacopo Fumagalli, Gonzalo A. Palma, Sébastien Renaux-Petel +3

We show that a scalar excited state with large occupation numbers during inflation leads to an enhancement of tensor modes and a characteristic pattern of order-one oscillations in…

astro-ph.CO2020★ 37 cited

A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data

S. Adachi, M. A. O. Aguilar Faúndez, K. Arnold +53

We report a measurement of the E-mode polarization power spectrum of the cosmic microwave background (CMB) using 150 GHz data taken from July 2014 to December 2016 with the POLARBE…

astro-ph.CO2019★ 24 cited

Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation

Anirut Phriksee, Eric Jullo, Marceau Limousin +5

We present the weak lensing analysis of 279 CODEX clusters using imaging data from 4200 of the DECam Legacy Survey (DECaLS) Data Release 3. The cluster sample resu…

astro-ph.CO2017★ 27 cited

Void profile from Planck lensing potential map

Teeraparb Chantavat, Utane Sawangwit, Benjamin D. Wandelt

We use the lensing potential map from Planck CMB lensing reconstruction analysis and the "Public Cosmic Void Catalog" to measure the stacked void lensing potential. In this profile…

astro-ph.CO2014★ 23 cited

Cosmological parameter constraints from CMB lensing with cosmic voids

Teeraparb Chantavat, Utane Sawangwit, P. M. Sutter +1

We investigate the potential of using cosmic voids as a probe to constrain cosmological parameters through the gravitational lensing effect of the cosmic microwave background (CMB)…

astro-ph.CO2012★ 26 cited

Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82

Nikolaos Nikoloudakis, Tom Shanks, Utane Sawangwit

We present a clustering analysis of Luminous Red Galaxies in SDSS Stripe 82. We study the angular 2-point correlation function, of 130,000 LRG candidates via colour-cut selections…

astro-ph.CO2011★ 5 cited

Testing the WMAP cosmology via Planck radio catalogues

J. R. Whitbourn, T. Shanks, U. Sawangwit

The prime evidence underpinning the standard LCDM cosmological model is the CMB power spectrum as observed by WMAP and other microwave experiments. But Sawangwit & Shanks (2010) ha…

astro-ph.CO2010★ 27 cited

Observational constraints on phantom power-law cosmology

Chakkrit Kaeonikhom, Burin Gumjudpai, Emmanuel N. Saridakis

We investigate phantom cosmology in which the scale factor is a power law, and we use cosmological observations from Cosmic Microwave Background (CMB), Baryon Acoustic Oscillations…