papers

Publications (17)

astro-ph.GA2010

Magnetic Fields Structures and Turbulent Components in the Star Forming Molecular Clouds OMC-2 and OMC-3

Frederick Poidevin, Pierre Bastien, Brenda C. Matthews

The SCUBA polarized 850 microns thermal emission data of the region OMC-2 in Orion A are added to and homogeneously reduced with data already available in the region OMC-3. The dat…

astro-ph.GA2020

Cosmic Amorphous Dust Model as the Origin of Anomalous Microwave Emission

Masashi Nashimoto, Makoto Hattor, Frederick Poidevin +1

We have shown that the thermal emission of the amorphous dust composed of amorphous silicate dust (a-Si) and amorphous carbon dust (a-C) provides excellent fit both to the observed…

astro-ph.HE2023

Follow-up survey for the binary black hole merger GW200224_222234 using Subaru/HSC and GTC/OSIRIS

Takayuki Ohgami, Josefa Becerra Gonzalez, Nozomu Tominaga +19

The LIGO/Virgo detected a gravitational wave (GW) event, named GW200224_222234 (a.k.a. S200224ca) and classified as a binary-black-hole coalescence, on February 24, 2020. Given its…

astro-ph.HE2026

AT 2024wpp: the most luminous fast-evolving optical transient linked to the merger explosion of a black-hole binary

Jialian Liu, Bao Wang, Xiaofeng Wang +48

Fast blue optical transients (FBOTs) represent one of the most exotic astrophysical transients, exhibiting unusually strong emission across X-ray, optical, and radio wavelengths. T…

astro-ph.GA2017

Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud

Fabio P. Santos, Peter A. R. Ade, Francesco E. Angile +27

We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at submillimeter (sub-mm) wave…

astro-ph.GA2013

SCUPOL Magnetic Field Analysis

Frederick Poidevin, Diego Falceta-Goncalves, Grzegorz Kowal +2

We present an extensive analysis of the 850 microns polarization maps of the SCUPOL Catalog produced by Matthews et al. (2009), focusing exclusively on the molecular clouds and sta…

astro-ph.GA2023

First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formation

Derek Ward-Thompson, Janik Karoly, Kate Pattle +155

We present BISTRO Survey 850 μm dust emission polarisation observations of the L1495A-B10 region of the Taurus molecular cloud, taken at the JCMT. We observe a roughly triangular…

astro-ph.GA2023

Evolution of the Mass-Metallicity Relation from Redshift to the Local Universe

Danial Langeroodi, Jens Hjorth, Wenlei Chen +17

A tight positive correlation between the stellar mass and the gas-phase metallicity of galaxies has been observed at low redshifts. The redshift evolution of this correlation can s…

astro-ph.GA2024

A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey

Jintai Wu, Keping Qiu, Frederick Poidevin +152

As part of the BISTRO survey, we present JCMT 850 m polarimetric observations towards the Orion Integral-Shaped Filament (ISF) that covers three portions known as OMC-1, OMC-2,…

astro-ph.GA2022

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

Abdurro'uf, Katherine Accetta, Conny Aerts +337

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete…

astro-ph.GA2020

Magnetism Science with the Square Kilometre Array

George Heald, Sui Ann Mao, Valentina Vacca +41

The Square Kilometre Array (SKA) will answer fundamental questions about the origin, evolution, properties, and influence of magnetic fields throughout the Universe. Magnetic field…

astro-ph.GA2023

A Magnified Compact Galaxy at Redshift 9.51 with Strong Nebular Emission Lines

Hayley Williams, Patrick L. Kelly, Wenlei Chen +21

Ultraviolet light from early galaxies is thought to have ionized gas in the intergalactic medium. However, there are few observational constraints on this epoch because of the fain…

astro-ph.GA2023

The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43

Janik Karoly, Derek Ward-Thompson, Kate Pattle +155

We present observations of polarized dust emission at 850 m from the L43 molecular cloud which sits in the Ophiuchus cloud complex. The data were taken using SCUBA-2/POL-2 on t…

astro-ph.HE2023

QUIJOTE scientific results -- XIII. Intensity and polarization study of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9

Carlos Hugo López-Caraballo, Beatriz Ruiz-Granados, Ricardo Genova Santos +21

We use the new QUIJOTE-MFI wide survey (11, 13, 17 and 19 GHz) to produce spectral energy distributions (SEDs), on an angular scale of 1 deg, of the supernova remnants (SNRs) CTB 8…

astro-ph.GA2022

The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

Tao-Chung Ching, Keping Qiu, Di Li +154

We present 850 m dust polarization observations of the massive DR21 filament from the B-fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter…

astro-ph.GA2025

The JCMT BISTRO Survey: Magnetic Fields Align with Orbital Structure in the Galactic Center

Janik Karoly, Derek Ward-Thompson, Kate Pattle +29

We present the magnetic field in the dense material of the Central Molecular Zone (CMZ) of the Milky Way, traced in 850 m polarized dust emission as part of the James Clerk Max…

astro-ph.IM2013

Empirical modelling of the BLASTPol achromatic half-wave plate for precision submillimetre polarimetry

Lorenzo Moncelsi, Peter Ade, Francesco Elio Angile +18

A cryogenic achromatic half-wave plate (HWP) for submillimetre astronomical polarimetry has been designed, manufactured, tested, and deployed in the Balloon-borne Large-Aperture Su…