The Daily Brew
Selected astro-ph abstracts for Wednesday 2023 May 17
- Cold New Early Dark Energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients
Juan S. Cruz, Florian Niedermann, Martin S. Sloth
[ arXiv:2305.08895v1 | PDF File ]
- Planting a Lyman alpha forest on AbacusSummit
Boryana Hadzhiyska, Andreu Font-Ribera, Andrei Cuceu, Solène Chabanier, Jessica Nicole Aguilar, David Brooks, Axel de la Macorra, Peter Doel, Daniel J. Eisenstein, Jaime E. Forero-Romero, Satya Gontcho A Gontcho, Klaus Honscheid, Robert Kehoe, Martin Landriau, Marc Manera, Ramon Miquel, Jundan Nie, Will Percival, Graziano Rossi, Michael Schubnell, Gregory Tarlé, Zhimin Zhou
[ arXiv:2305.08899v1 | PDF File ]
- Neutron star kicks and implications for their rotation at birth
Giacomo Fragione, Abraham Loeb
[ arXiv:2305.08920v1 | PDF File ]
- SILVERRUSH. XIII. A Catalog of 20,567 Ly$\alpha$ Emitters at $z=2-7$ Identified in the Full-Depth Data of the Subaru/HSC-SSP and CHORUS Surveys
Satoshi Kikuta, Masami Ouchi, Takatoshi Shibuya, Yongming Liang, Hiroya Umeda, Akinori Matsumoto, Kazuhiro Shimasaku, Yuichi Harikane, Yoshiaki Ono, Akio K. Inoue, Satoshi Yamanaka, Haruka Kusakabe, Rieko Momose, Nobunari Kashikawa, Yuichi Matsuda, Chien-Hsiu Lee
[ arXiv:2305.08921v1 | PDF File ]
- A hot super-Earth planet in the WASP-84 planetary system
G. Maciejewski, J. Golonka, W.Łoboda, J. Ohlert, M. Fernandez, F. Aceituno
[ arXiv:2305.09177v1 | PDF File ]
- The First Results of Distributed Peer Review at ESO Show Promising Outcomes
Tereza Jerabkova, Ferdinando Patat, Francesca Primas, Dario Dorigo, Fabio Sogni, Lucas Astolfi, Thomas Bierwirth, Michael Pruemm
[ arXiv:2305.09277v1 | PDF File ]
- Emission line variability of young 10-30 Mjup companions : I. The case of GQ Lup b and GSC 06214-00210 b
Dorian Demars (1), Mickael Bonnefoy (1), Catherine Dougados (1), Yuhiko Aoyama (2, 3 and 4), Thanawuth Thanathibodee (5 and 6), Gabriel-Dominique Marleau (7, 8, 9 and 10), Pascal Tremblin (11), Philippe Delorme (1), Paulina Palma-Bifani (12), Simon Petrus (13 and 14), Brendan P. Bowler (15), Gael Chauvin (12 and 1), Anne-Marie Lagrange (16 and 1) ((1) Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France, (2) Institute for Advanced Study, Tsinghua University, Beijing, People's Republic of China, (3) Department of Astronomy, Tsinghua University, Beijing, People's Republic of China, (4) Department of Earth and Planetary Science, The University of Tokyo, Japan, (5) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA, (6) Institute for Astrophysical Research and Department of Astronomy, Boston University, Boston, MA, USA, (7) Fakultät für Physik, Universität Duisburg-Essen, Tübingen, Germany, (9) Physikalisches Institut, Universität Bern, Bern, Switzerland, (10) Max-Planck-Institut für Astronomie, Heidelberg, Germany, (11) Maison de la Simulation, CEA, CNRS, Univ. Paris-Sud, UVSQ, Université Paris-Saclay, Gif-sur-Yvette, France, (12) Université Côte d'Azur, OCA, Lagrange CNRS, Nice, France, (13) Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Av. Gran Bretaña, Valparaíso, Chile, (14) Núcleo Milenio Formación Planetaria - NPF, Universidad de Valparaíso, Av., Valparaíso, Chile, (15) Department of Astronomy, The University of Texas at Austin, Austin, TX, USA, (16) LESIA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, Univ. Paris Diderot, Sorbonne Paris Cité, Meudon, France)
[ arXiv:2305.09460v1 | PDF File ]
- The Period Distribution of Hot Jupiters is Not Dependent on Host Star Metallicity
Samuel W. Yee, Joshua N. Winn
[ arXiv:2305.09488v1 | PDF File ]
brew.pl Version 2.5.2 [2022-03-22]