19.6k citations
- Center for Astrophysics Harvard & SmithsonianUS436 papers
- University of MichiganUS426 papers
- Centre National de la Recherche ScientifiqueFR391 papers
- Fermi National Accelerator LaboratoryUS385 papers
- University of Illinois Urbana-ChampaignUS385 papers
- The Ohio State UniversityUS367 papers
- University of ChicagoUS363 papers
- Kavli Institute for Particle Astrophysics and CosmologyUS360 papers
- Stanford UniversityUS342 papers
- SLAC National Accelerator LaboratoryUS338 papers
- University College LondonGB334 papers
- National Center for Supercomputing ApplicationsUS329 papers
22 papers · 1 filter
The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
G. Munoz-Sanchez, M. Kalitsounaki, S. de Wit +8
Red Supergiants (RSGs) are cool, evolved massive stars in their final evolutionary stage before exploding as a supernova. However, the evolution and fate of the most luminous RSGs…
Discovery and Spectroscopic Confirmation of Aquarius III: A Low-Mass Milky Way Satellite Galaxy
W. Cerny, A. Chiti, M. Geha +37
We present the discovery of Aquarius III, an ultra-faint Milky Way satellite galaxy identified in the second data release of the DECam Local Volume Exploration (DELVE) survey. Base…
TOI-5005 b: A super-Neptune in the savanna near the ridge
A. Castro-González, J. Lillo-Box, D. J. Armstrong +38
The Neptunian desert and savanna have recently been found to be separated by a ridge, an overdensity of planets in the period range of 3-5 days. These features are thought…
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves
N. Monsalves, M. Jaque Arancibia, A. Bayo +4
In recent years the amount of publicly available astronomical data has increased exponentially, with a remarkable example being large scale multiepoch photometric surveys. This wea…
Properties of outer solar system pebbles during planetesimal formation from meteor observations
Peter Jenniskens, Paul R. Estrada, Stuart Pilorz +42
In the late stages of accretion leading up to the formation of planetesimals, particles grew to pebbles the size of 1-mm to tens of cm. That is the same size range that dominates t…
The effect of dynamical states on galaxy clusters populations. I. Classification of dynamical states
S. Véliz Astudillo, E. R. Carrasco, J. L. Nilo Castellón +2
While the influence of galaxy clusters on galaxy evolution is relatively well-understood, the impact of the dynamical states of these clusters is less clear. This paper series expl…