output
20022026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2017 · astro-ph.SRShow all

19 papers · 2 filters

astro-ph.SR2017★ 137 cited

The First APOKASC Catalog of Kepler Dwarf and Subgiant Stars

Aldo Serenelli, Jennifer Johnson, Daniel Huber +23

(Abridged) We present the first APOKASC catalog of spectroscopic and asteroseismic data for 415 dwarfs and subgiants. Asteroseismic data have been obtained by Kepler in short caden…

astro-ph.SR2017★ 49 cited

A physically motivated and empirically calibrated method to measure effective temperature, metallicity, and Ti abundance of M dwarfs

Mark J. Veyette, Philip S. Muirhead, Andrew W. Mann +3

The ability to perform detailed chemical analysis of Sun-like F-, G-, and K-type stars is a powerful tool with many applications including studying the chemical evolution of the Ga…

astro-ph.SR2017★ 41 cited

Model-independent measurement of internal stellar structure in 16 Cygni A and B

Earl P. Bellinger, Sarbani Basu, Saskia Hekker +1

We present a method for measuring internal stellar structure based on asteroseismology that we call "inversions for agreement." The method accounts for imprecise estimates of stell…

astro-ph.SR2017★ 69 cited

Predicting Stellar Angular Diameters from , , , Photometry

Arthur D. Adams, Tabetha S. Boyajian, Kaspar von Braun

Determining the physical properties of microlensing events depends on having accurate angular sizes of the source star. Using long-baseline optical interferometry we are able to me…

astro-ph.SR2017★ 2 cited

An analytic mean-field -dynamo with a force-free corona

Alfio Bonanno, Fabio Del Sordo

Stellar dynamos are affected by boundary conditions imposed by stellar coronae. Under some approximations it is possible to find analytical solutions. Interior dynamo models often…

astro-ph.SR2017★ 108 cited

PLATO as it is: a legacy mission for Galactic archaeology

A. Miglio, C. Chiappini, B. Mosser +102

Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy.…