Search Publications

The MUSE Deep Lensed Field on the Hubble Frontier Field MACS J0416. Star-forming complexes at cosmological distances
DOI: 10.1051/0004-6361/202039466 Bibcode: 2021A&A...646A..57V

Treu, T.; Castellano, M.; Pentericci, L. +21 more

Context. A census of faint and tiny star forming complexes at high redshift is key to improving our understanding of reionizing sources, galaxy growth, and the formation of globular clusters.
Aims: We present the MUSE Deep Lensed Field (MDLF) program, which is aimed at unveiling the very faint population of high redshift sources that are magn…

2021 Astronomy and Astrophysics
eHST 63
The Hubble constant from eight time-delay galaxy lenses
DOI: 10.1093/mnras/staa3603 Bibcode: 2021MNRAS.501..784D

Saha, Prasenjit; Williams, Liliya L. R.; Denzel, Philipp +1 more

We present a determination of the Hubble constant from the joint, free-form analysis of eight strongly, quadruply lensing systems. In the concordance cosmology, we find $H_0{} = 71.8^{+3.9}_{-3.3}\, \mathrm{km}\, \mathrm{s}^{-1}\, \mathrm{Mpc}^{-1}{}{}$ with a precision of $4.97{{\ \rm per\ cent}}$. This is in agreement with the latest measurement…

2021 Monthly Notices of the Royal Astronomical Society
eHST 63
Luminosity Functions and Host-to-host Scatter of Dwarf Satellite Systems in the Local Volume
DOI: 10.3847/1538-4357/abd039 Bibcode: 2021ApJ...908..109C

Greene, Jenny E.; Beaton, Rachael L.; Peter, Annika H. G. +2 more

Low-mass satellites around Milky Way (MW)-like galaxies are important probes of small-scale structure and galaxy formation. However, confirmation of satellite candidates with distance measurements remains a key barrier to fast progress in the Local Volume (LV). We measure the surface brightness fluctuation distances to recently cataloged candidate…

2021 The Astrophysical Journal
eHST 63
Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3
DOI: 10.3847/1538-3881/ac273e Bibcode: 2021AJ....162..301B

Currie, Thayne; Dupuy, Trent J.; Bowler, Brendan P. +8 more

We present comprehensive orbital analyses and dynamical masses for the substellar companions Gl 229 B, Gl 758 B, HD 13724 B, HD 19467 B, HD 33632 Ab, and HD 72946 B. Our dynamical fits incorporate radial velocities, relative astrometry, and, most importantly, calibrated Hipparcos-Gaia EDR3 accelerations. For HD 33632 A and HD 72946 we perform thre…

2021 The Astronomical Journal
Gaia Hipparcos eHST 62
Solar structure and evolution
DOI: 10.1007/s41116-020-00028-3 Bibcode: 2021LRSP...18....2C

Christensen-Dalsgaard, Jørgen

The Sun provides a critical benchmark for the general study of stellar structure and evolution. Also, knowledge about the internal properties of the Sun is important for the understanding of solar atmospheric phenomena, including the solar magnetic cycle. Here I provide a brief overview of the theory of stellar structure and evolution, including t…

2021 Living Reviews in Solar Physics
SOHO Ulysses 62
The ANTARES Astronomical Time-domain Event Broker
DOI: 10.3847/1538-3881/abd703 Bibcode: 2021AJ....161..107M

Lee, Chien-Hsiu; Scott, Adam; Matheson, Thomas +17 more

We describe the Arizona-NOIRLab Temporal Analysis and Response to Events System (ANTARES), a software instrument designed to process large-scale streams of astronomical time-domain alerts. With the advent of large-format CCDs on wide-field imaging telescopes, time-domain surveys now routinely discover tens of thousands of new events each night, mo…

2021 The Astronomical Journal
Gaia 62
Redshift evolution of the underlying type Ia supernova stretch distribution
DOI: 10.1051/0004-6361/202038447 Bibcode: 2021A&A...649A..74N

Smith, M.; Aldering, G.; Nordin, J. +7 more

The detailed nature of type Ia supernovae (SNe Ia) remains uncertain, and as survey statistics increase, the question of astrophysical systematic uncertainties arises, notably that of the evolution of SN Ia populations. We study the dependence on redshift of the SN Ia SALT2.4 light-curve stretch, which is a purely intrinsic SN property, to probe i…

2021 Astronomy and Astrophysics
eHST 62
Turbulent Generation of Magnetic Switchbacks in the Alfvénic Solar Wind
DOI: 10.3847/1538-4357/abfdbc Bibcode: 2021ApJ...915...52S

Cranmer, Steven R.; Shoda, Munehito; Chandran, Benjamin D. G.

One of the most important early results from the Parker Solar Probe (PSP) is the ubiquitous presence of magnetic switchbacks, whose origin is under debate. Using a three-dimensional direct numerical simulation of the equations of compressible magnetohydrodynamics from the corona to 40 solar radii, we investigate whether magnetic switchbacks emerge…

2021 The Astrophysical Journal
PROBA-2 62
Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars
DOI: 10.1103/PhysRevLett.126.021102 Bibcode: 2021PhRvL.126b1102B

Buschmann, Malte; Safdi, Benjamin R.; Dessert, Christopher +1 more

Axions may be produced thermally inside the cores of neutron stars (NSs), escape the stars due to their feeble interactions with matter, and subsequently convert into x rays in the magnetic fields surrounding the stars. We show that a recently discovered excess of hard x-ray emission in the 2-8 keV energy range from the nearby magnificent seven is…

2021 Physical Review Letters
XMM-Newton 62
The search for failed supernovae with the Large Binocular Telescope: a new candidate and the failed SN fraction with 11 yr of data
DOI: 10.1093/mnras/stab2605 Bibcode: 2021MNRAS.508..516N

Kochanek, C. S.; Stanek, K. Z.; Adams, S. M. +5 more

We present updated results of the Large Binocular Telescope Search for Failed Supernovae. This search monitors luminous stars in 27 nearby galaxies with a current baseline of 11 yr of data. We re-discover the failed supernova (SN) candidate N6946-BH1 as well as a new candidate, M101-OC1. M101-OC1 is a blue supergiant that rapidly disappears in opt…

2021 Monthly Notices of the Royal Astronomical Society
eHST 62