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New website brought alive

by Janos Bartus on 2016-11-12

Welcome to the new PEPSI website.

News

Jan. 24, 2026
Does the solar oxygen abundance change over the solar cycle?: An investigation into activity-induced variations in the O I infrared triplet

Jan. 7, 2026
Surface image and activity-corrected orbit of the RSCVn binary HR7275: Disentangling activity tracers

Jan. 6, 2026
Untangling the Sources of Abundance Dispersion in Low-metallicity Stars. II. Neutron Capture Elements

Jan. 5, 2026
Elemental abundance pattern and temperature inversion on the dayside of HAT-P-70b observed with CARMENES and PEPSI

Nov. 27, 2025
Surface activity of a Rossby number sequence of cool Hyades stars

Nov. 22, 2025
PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-resolution Phased-resolved Spectroscopy of the Ultra-hot-Jupiter KELT-20b

Nov. 21, 2025
PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). II. Phase-resolved cross-correlation transmission spectroscopy of KELT-20b

Nov. 6, 2025
PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). III. Composition and winds in the atmosphere of TOI-1518b

May 9, 2025
A search for Maunder-minimum candidate stars

March 27, 2025
PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). I. The Ubiquity of Fe I Emission and Inversions in Ultra Hot Jupiter Atmospheres

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Reference to PEPSI: Strassmeier et al. (2015AN....336..324S)

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