Search Results - "Dreizler, Stefan"
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The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood
Published in The Astrophysical journal (20-09-2018)“…The compositions of stars are a critical diagnostic tool for many topics in astronomy such as the evolution of our Galaxy, the formation of planets, and the…”
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2
A detached stellar-mass black hole candidate in the globular cluster NGC 3201
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2018)“…Abstract As part of our massive spectroscopic survey of 25 Galactic globular clusters with MUSE, we performed multiple epoch observations of NGC 3201 with the…”
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3
Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69b
Published in Science (American Association for the Advancement of Science) (21-12-2018)“…Hot gas giant exoplanets can lose part of their atmosphere due to strong stellar irradiation, affecting their physical and chemical evolution. Studies of…”
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Ultradeep ATCA Imaging of 47 Tucanae Reveals a Central Compact Radio Source
Published in The Astrophysical journal (01-01-2024)“…Abstract We present the results of an ultradeep radio continuum survey, containing ∼480 hr of observations, of the Galactic globular cluster 47 Tucanae with…”
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5
Validating AU Microscopii d with Transit Timing Variations
Published in The Astronomical journal (01-12-2023)“…Abstract AU Mic is a young (22 Myr), nearby exoplanetary system that exhibits excess transit timing variations (TTVs) that cannot be accounted for by the two…”
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6
The Transit Ingress and the Tilted Orbit of the Extraordinarily Eccentric Exoplanet HD 80606b
Published in The Astrophysical journal (01-10-2009)“…We present the results of a transcontinental campaign to observe the 2009 June 5 transit of the exoplanet HD 80606b. We report the first detection of the…”
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7
The temporal evolution of neutron-capture elements in the Galactic discs
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract Important insights into the formation and evolution of the Galactic disc(s) are contained in the chemical compositions of stars. We analysed…”
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ω Centauri: a MUSE discovery of a counter-rotating core
Published in Monthly notices of the Royal Astronomical Society (01-03-2024)“…ABSTRACT ω Centauri is considered the most massive globular cluster of the Milky Way and likely the former nuclear star cluster of a Galaxy accreted by the…”
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A terrestrial planet candidate in a temperate orbit around Proxima Centauri
Published in Nature (London) (25-08-2016)“…A small planet of at least 1.3 Earth masses is orbiting Proxima Centauri with a period of about 11.2 days, with the potential for liquid water on its surface…”
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10
Ultra-deep ATCA imaging of 47 Tucanae reveals a central compact radio source
Published in The Astrophysical journal (15-01-2024)“…We present the results of an ultradeep radio continuum survey, containing ∼480 hr of observations, of the Galactic globular cluster 47 Tucanae with the…”
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The CRIRES Search for Planets Around the Lowest-mass Stars. I. High-precision Near-infrared Radial Velocities with an Ammonia Gas Cell
Published in The Astrophysical journal (10-04-2010)“…Radial velocities measured from near-infrared (NIR) spectra are a potentially powerful tool to search for planets around cool stars and sub-stellar objects…”
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12
Central kinematics of the Galactic globular cluster M80
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT We use spectra observed with the integral-field spectrograph Multi Unit Spectroscopic Explorer (MUSE) to reveal the central kinematics of the Galactic…”
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13
Spectroscopic binaries in the Solar Twin Planet Search program: from substellar–mass to M dwarf companions
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…Abstract Previous studies on the rotation of Sun-like stars revealed that the rotational rates of young stars converge towards a well-defined evolution that…”
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TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations Revealed by TESS
Published in The Astronomical journal (01-04-2023)“…Abstract The K-type star TOI-2525 has an estimated mass of M = 0.849 − 0.033 + 0.024 M ⊙ and radius of R = 0.785 − 0.007 + 0.007 R ⊙ observed by the TESS…”
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A Transiting, Temperate Mini-Neptune Orbiting the M Dwarf TOI-1759 Unveiled by TESS
Published in The Astronomical journal (01-03-2022)“…Abstract We report the discovery and characterization of TOI-1759 b, a temperate (400 K) sub-Neptune-sized exoplanet orbiting the M dwarf TOI-1759 (TIC…”
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The MAVERIC Survey: The first radio and X-ray limits on the detached black holes in NGC 3201
Published in Monthly notices of the Royal Astronomical Society (01-03-2022)“…ABSTRACT The Galactic globular cluster (GC) NGC 3201 is the first Galactic GC observed to host dynamically confirmed stellar-mass black holes (BHs), containing…”
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Proxima Centauri b is not a transiting exoplanet
Published in Monthly notices of the Royal Astronomical Society (21-07-2019)“…Abstract We report Spitzer Space Telescope observations during predicted transits of the exoplanet Proxima Centauri b. As the nearest terrestrial…”
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Transit Timing Variations for AU Microscopii b and c
Published in The Astronomical journal (01-07-2022)“…We explore the transit timing variations (TTVs) of the young (22 Myr) nearby AU Mic planetary system. For AU Mic b, we introduce three Spitzer (4.5 μm)…”
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TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations Revealed by TESS ∗ Based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere under MPG program 0104.A-9007. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile
Published in The Astronomical journal (28-03-2023)Get full text
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Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy
Published in Astrophysical journal. Letters (01-06-2024)“…Abstract Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via…”
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