output
19962026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

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525 papers · 1 filter

astro-ph.GA2020★ 12 cited

The APOGEE Library of Infrared SSP Templates (A-LIST): High-Resolution Simple Stellar Population Spectral Models in the H-Band

Aishwarya Ashok, Gail Zasowski, Anil Seth +8

Integrated light spectroscopy from galaxies can be used to study the stellar populations that cannot be resolved into individual stars. This analysis relies on stellar population s…

astro-ph.SR2020★ 5 cited

Observing the changing surface structures of the active K giant sigma Gem with SONG

H. Korhonen, R. M. Roettenbacher, S. Gu +6

Aims: We aim to study the spot evolution and differential rotation in the magnetically active cool K-type giant star sigma Gem from broadband photometry and continuous spectroscopi…

astro-ph.SR2020★ 4 cited

Low-mass and sub-stellar eclipsing binaries in stellar clusters

Nicolas Lodieu, Ernst Paunzen, Miloslav Zejda

We highlight the importance of eclipsing double-line binaries in our understanding on star formation and evolution. We review the recent discoveries of low-mass and sub-stellar ecl…

astro-ph.SR2020★ 4 cited

Analysis of Previously Classified White Dwarf-Main Sequence Binaries Using Data from the APOGEE Survey

Kyle A. Corcoran, Hannah M. Lewis, Borja Anguiano +12

We present analyses of near-infrared, spectroscopic data from the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey for 45 previously confirmed or candidate wh…

astro-ph.EP2020★ 28 cited

GD424 -- a helium-atmosphere white dwarf with a large amount of trace hydrogen in the process of digesting a rocky planetesimal

Paula Izquierdo, Odette Toloza, Boris T. Gänsicke +5

The photospheric metal pollution of white dwarfs is now well-established as the signature of the accretion of planetary debris. However, the origin of the trace hydrogen detected i…

astro-ph.SR2020★ 30 cited

Understanding the evolution and dust formation of carbon stars in the LMC with a look at the JWST

E. Marini, F. Dell'Agli, M. A. T. Groenewegen +6

Carbon stars have been and are extensively studied, given their complex internal structure and their peculiar chemical composition, which make them living laboratories to test stel…