Search Publications

Imaging detection of the inner dust belt and the four exoplanets in the HR 8799 system with JWST's MIRI coronagraph
DOI: 10.1051/0004-6361/202347912 Bibcode: 2024A&A...686A..33B

Henning, Thomas; Güdel, Manuel; Colina, Luis +35 more

Context. The MIRI instrument on board JWST is now offering high-contrast imaging capacity at mid-IR wavelengths, thereby opening a completely new field of investigation for characterizing young exoplanetary systems.
Aims: The multiplanet system HR 8799 is the first target observed with MIRI's coronagraph as part of the MIRI-EC Guaranteed Time…

2024 Astronomy and Astrophysics
AKARI Gaia JWST 17
The cosmic dipole in the Quaia sample of quasars: a Bayesian analysis
DOI: 10.1093/mnras/stad3706 Bibcode: 2024MNRAS.527.8497M

Lewis, Geraint F.; Mittal, Vasudev; Oayda, Oliver T.

We present a Bayesian analysis of the Quaia sample of 1.3 million quasars as a test of the cosmological principle. This principle postulates that the Universe is homogeneous and isotropic on sufficiently large scales, forming the basis of prevailing cosmological models. However, recent analyses of quasar samples have found a matter dipole inconsis…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 17
Ticking away: The long-term X-ray timing and spectral evolution of eRO-QPE2
DOI: 10.1051/0004-6361/202451218 Bibcode: 2024A&A...690A..80A

Merloni, A.; Ponti, G.; Miniutti, G. +11 more

Quasi-periodic eruptions (QPEs) are repeated X-ray flares from galactic nuclei that recur every few hours to days, depending on the source. Despite some diversity in the recurrence and amplitude of eruptions, their striking regularity has motivated theorists to associate QPEs with orbital systems. Among the known QPE sources, eRO-QPE2 has shown th…

2024 Astronomy and Astrophysics
XMM-Newton 17
Dynamical Stellar Mass-to-light Ratio Gradients: Evidence for Very Centrally Concentrated IMF Variations in ETGs?
DOI: 10.3847/1538-4357/acfe09 Bibcode: 2024ApJ...961..127M

Bender, Ralf; Thomas, Jens; Erwin, Peter +4 more

Evidence from different probes of the stellar initial mass function (IMF) of massive early-type galaxies (ETGs) has repeatedly converged on IMFs more bottom heavy than in the Milky Way (MW). This consensus has come under scrutiny due to often contradictory results from different methods on the level of individual galaxies. In particular, a number …

2024 The Astrophysical Journal
eHST 16
The Merian survey: design, construction, and characterization of a filter set optimized to find dwarf galaxies and measure their dark matter halo properties with weak lensing
DOI: 10.1093/mnras/stae925 Bibcode: 2024MNRAS.530.4988L

Johnson, Sean D.; Cai, Zheng; Lin, Xiaojing +28 more

The Merian survey is mapping ~ 850 deg2 of the Hyper Suprime-Cam Strategic Survey Program (HSC-SSP) wide layer with two medium-band filters on the 4-m Victor M. Blanco telescope at the Cerro Tololo Inter-American Observatory, with the goal of carrying the first high signal-to-noise (S/N) measurements of weak gravitational lensing around…

2024 Monthly Notices of the Royal Astronomical Society
eHST 16
Chemical Cartography of the Sagittarius Stream with Gaia
DOI: 10.3847/1538-4357/ad187b Bibcode: 2024ApJ...963...95C

Price-Whelan, Adrian M.; Ness, Melissa K.; Johnston, Kathryn V. +5 more

The stellar stream connected to the Sagittarius (Sgr) dwarf galaxy is the most massive tidal stream that has been mapped in the Galaxy, and is the dominant contributor to the outer stellar halo of the Milky Way (MW). We present metallicity maps of the Sgr stream, using 34,240 red giant branch stars with inferred metallicities from Gaia BP/RP spect…

2024 The Astrophysical Journal
Gaia 16
DESI Early Data Release Milky Way Survey value-added catalogue
DOI: 10.1093/mnras/stae1842 Bibcode: 2024MNRAS.533.1012K

Moustakas, J.; Brooks, D.; Li, T. S. +40 more

We present the stellar value-added catalogue based on the Dark Energy Spectroscopic Instrument (DESI) Early Data Release. The catalogue contains radial velocity and stellar parameter measurements for $\simeq$ 400 000 unique stars observed during commissioning and survey validation by DESI. These observations were made under conditions similar to t…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 16
The Mass of the Large Magellanic Cloud from the Three-dimensional Kinematics of Its Globular Clusters
DOI: 10.3847/1538-4357/ad1f58 Bibcode: 2024ApJ...963...84W

van der Marel, Roeland P.; Watkins, Laura L.; Bennet, Paul

We estimate the mass of the Large Magellanic Cloud (LMC) using the kinematics of 30 LMC globular clusters (GCs). We combine proper motions measured with the Hubble Space Telescope, Gaia, or a combination of the two, from a recent study by Bennet et al. with literature line-of-sight velocities (LOSVs) to give three components of motion. With these,…

2024 The Astrophysical Journal
eHST 16
Ground-based and JWST Observations of SN 2022pul. II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type Ia Supernova
DOI: 10.3847/1538-4357/ad2c0d Bibcode: 2024ApJ...966..135K

Temim, Tea; Filippenko, Alexei V.; Coulter, David A. +78 more

We present an analysis of ground-based and JWST observations of SN 2022pul, a peculiar "03fg-like" (or "super-Chandrasekhar") Type Ia supernova (SN Ia), in the nebular phase at 338 days postexplosion. Our combined spectrum continuously covers 0.4–14 µm and includes the first mid-infrared spectrum of a 03fg-like SN Ia. Compared to normal SN I…

2024 The Astrophysical Journal
JWST 16
Statistical investigation of decayless oscillations in small-scale coronal loops observed by Solar Orbiter/EUI
DOI: 10.1051/0004-6361/202346670 Bibcode: 2024A&A...685A..36S

Van Doorsselaere, Tom; Lim, Daye; Berghmans, David +6 more

Decayless kink oscillations are omnipresent in the solar atmosphere, and they are a viable candidate for coronal heating. Although there have been extensive studies of decayless oscillations in coronal loops with lengths of a few hundred megameters, the properties of these oscillations in small-scale (∼10 mm) loops are yet to be explored. In this …

2024 Astronomy and Astrophysics
SolarOrbiter 16