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Multimass modelling of milky way globular clusters - II. Present-day black hole populations
Hénault-Brunet, V.; Gieles, M.; Baumgardt, H. +2 more
Populations of stellar-mass black holes (BHs) in globular clusters (GCs) influence their dynamical evolution and have important implications on one of the main formation channels for gravitational wave sources. Inferring the size of these populations remains difficult, however. In this work, multimass models of 34 Milky Way GCs, first presented in…
The Search for Failed Supernovae with the Large Binocular Telescope: The Mid-infrared Counterpart to N6946-BH1
Kochanek, Christopher S.; Neustadt, Jack M. M.; Stanek, Krzysztof Z.
We present JWST MIRI 5.6, 10, and 21 µm observations of the candidate failed supernova N6946-BH1 along with Hubble Space Telescope (HST) WFPC/IR 1.1 and 1.6 µm data and ongoing optical monitoring data with the Large Binocular Telescope. There is a very red, dusty source at the location of the candidate, which has only ∼10%–15% of the l…
Implications of the Stellar Mass Density of High-z Massive Galaxies from JWST on Warm Dark Matter
Gong, Yan; Chen, Xuelei; Lin, Hengjie +1 more
A significant excess of the stellar mass density at high redshift has been discovered from the early data release of James Webb Space Telescope (JWST), and it may require a high star formation efficiency. However, this will lead to large number density of ionizing photons in the epoch of reionization (EoR), so that the reionization history will be…
Searching for Strong Gravitational Lenses
Hezaveh, Yashar; Courbin, Frédéric; Leung, Calvin +9 more
Strong gravitational lenses provide unique laboratories for cosmological and astrophysical investigations, but they must first be discovered - a task that can be met with significant contamination by other astrophysical objects and asterisms. Here we review strong lens searches, covering various sources (quasars, galaxies, supernovae, FRBs, GRBs, …
A Census from JWST of Extreme Emission-line Galaxies Spanning the Epoch of Reionization in CEERS
Papovich, Casey; Finkelstein, Steven L.; Barro, Guillermo +30 more
We present a sample of 1165 extreme emission-line galaxies (EELGs) at 4 < z < 9 selected using James Webb Space Telescope (JWST) NIRCam photometry in the Cosmic Evolution Early Release Science (CEERS) program. We use a simple method to photometrically identify EELGs with Hβ + [O III] (combined) or Hα emission of observed-frame equivalent wid…
First Constraints on the Epoch of Reionization Using the Non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and Herschel-SPIRE Observations
Ade, P. A. R.; Benabed, K.; Bouchet, F. R. +123 more
We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel'dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and Herschel-SPIRE experiments over a
SN 2021adxl: A luminous nearby interacting supernova in an extremely low-metallicity environment
Drake, A. J.; Sollerman, J.; Fransson, C. +17 more
SN 2021adxl is a slowly evolving, luminous, Type IIn supernova with asymmetric emission line profiles, similar to the well-studied SN 2010jl. We present extensive optical, near-ultraviolet, and near-infrared photometry and spectroscopy covering ∼1.5 years post discovery. SN 2021adxl occurred in an unusual environment, atop a vigorously star-formin…
Structure, kinematics, and time evolution of the Galactic warp from Classical Cepheids
Antoja, Teresa; Aguilar, Luis; Ramos, Pau +3 more
The warp is a well-known undulation of the Milky Way disc. Its structure has been widely studied, but only since Gaia DR2 has it been possible to reveal its kinematic signature beyond the solar neighbourhood. In this work, we present an analysis of the warp traced by Classical Cepheids by means of a Fourier decomposition of their height (Z) and, f…
Measuring the initial-final mass relation using wide double white dwarf binaries from Gaia DR3
Littlefair, S. P.; Hollands, M. A.; Parsons, S. G.
The initial-final mass relation (IFMR) maps the masses of main-sequence stars to their white dwarf descendants. The most common approach to measure the IFMR has been to use white dwarfs in clusters. However, it has been shown that wide double white dwarfs can also be used to measure the IFMR using a Bayesian approach. We have observed a large samp…
X-Shooting ULLYSES: Massive stars at low metallicity. II. DR1: Advanced optical data products for the Magellanic Clouds
Hamann, W. -R.; Blomme, R.; Mehner, A. +34 more
Context. The XShootU project aims to obtain ground-based optical to near-infrared spectroscopy of all targets observed by the Hubble Space Telescope (HST) under the Director's Discretionary program ULLYSES. Using the medium-resolution spectrograph X-shooter, spectra of 235 OB and Wolf-Rayet (WR) stars in subsolar metallicity environments have been…