Search Publications

Revisiting the 16 Cygni planet host at unprecedented precision and exploring automated tools for precise abundances
DOI: 10.1051/0004-6361/201935952 Bibcode: 2019A&A...628A.126M

Spina, L.; Jofré, P.; Meléndez, J. +2 more

The binary system 16 Cygni is key in studies of the planet-star chemical composition connection, as only one of the stars is known to host a planet. This allows us to better assess the possible influence of planet interactions on the chemical composition of stars that are born from the same cloud and thus should have a similar abundance pattern. I…

2019 Astronomy and Astrophysics
Gaia 43
Characterization of Ring Substructures in the Protoplanetary Disk of HD 169142 from Multiwavelength Atacama Large Millimeter/submillimeter Array Observations
DOI: 10.3847/1538-4357/ab31a2 Bibcode: 2019ApJ...881..159M

Flock, Mario; Henning, Thomas; Dent, William R. F. +10 more

We present a detailed multiwavelength characterization of the multi-ring disk of HD 169142. We report new Atacama Large Millimeter/submillimeter Array (ALMA) observations at 3 mm and analyze them together with archival 0.89 and 1.3 mm data. Our observations resolve three out of the four rings in the disk previously seen in high-resolution ALMA dat…

2019 The Astrophysical Journal
Gaia 43
Understanding the Limitations of Gyrochronology for Old Field Stars
DOI: 10.3847/1538-4357/aaf575 Bibcode: 2019ApJ...871...39M

Metcalfe, Travis S.; Egeland, Ricky

Nearly half a century has passed since the initial indications that stellar rotation slows while chromospheric activity weakens with a power-law dependence on age, the so-called Skumanich relations. Subsequent characterization of the mass-dependence of this behavior up to the age of the Sun led to the advent of gyrochronology, which uses the rotat…

2019 The Astrophysical Journal
Gaia 42
Effects of Ducting on Whistler Mode Chorus or Exohiss in the Outer Radiation Belt
DOI: 10.1029/2019GL083115 Bibcode: 2019GeoRL..46.5735H

Hanzelka, Miroslav; Santolík, Ondřej

Previously published statistics based on Cluster spacecraft measurements surprisingly show that in the outer radiation belt, lower band whistler mode waves predominantly propagate unattenuated parallel to the magnetic field lines up to midlatitudes, where ray tracing simulations indicated highly attenuated waves with oblique wave vectors. We expla…

2019 Geophysical Research Letters
Cluster 42
Masses and radii for the three super-Earths orbiting GJ 9827, and implications for the composition of small exoplanets
DOI: 10.1093/mnras/stz130 Bibcode: 2019MNRAS.484.3731R

Bouchy, F.; Vanderburg, A.; Poretti, E. +34 more

Super-Earths belong to a class of planet not found in the Solar system, but which appear common in the Galaxy. Given that some super-Earths are rocky, while others retain substantial atmospheres, their study can provide clues as to the formation of both rocky and gaseous planets, and - in particular - they can help to constrain the role of photoev…

2019 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 42
Detecting shocked intergalactic gas with X-ray and radio observations
DOI: 10.1051/0004-6361/201935439 Bibcode: 2019A&A...627A...5V

Ettori, S.; Roncarelli, M.; Vazza, F. +3 more

Detecting the thermal and non-thermal emission from the shocked cosmic gas surrounding large-scale structures represents a challenge for observations, as well as a unique window into the physics of the warm-hot intergalactic medium. In this work, we present synthetic radio and X-ray surveys of large cosmological simulations in order to assess the …

2019 Astronomy and Astrophysics
XMM-Newton 42
Cosmological test using the Hubble diagram of high-z quasars
DOI: 10.1093/mnras/stz2120 Bibcode: 2019MNRAS.489..517M

Melia, Fulvio

It has been known for over three decades that the monochromatic X-ray and UV luminosities in quasars are correlated, though non-linearly. This offers the possibility of using high-z quasars as standard candles for cosmological testing. In this paper, we use a recently assembled, high-quality catalogue of 1598 quasars extending all the way to redsh…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 42
KiDS-SQuaD. II. Machine learning selection of bright extragalactic objects to search for new gravitationally lensed quasars
DOI: 10.1051/0004-6361/201936006 Bibcode: 2019A&A...632A..56K

Agnello, Adriano; Kuijken, Konrad; Spiniello, Chiara +9 more

Context. The KiDS Strongly lensed QUAsar Detection project (KiDS-SQuaD) is aimed at finding as many previously undiscovered gravitational lensed quasars as possible in the Kilo Degree Survey. This is the second paper of this series where we present a new, automatic object-classification method based on the machine learning technique.
Aims: Th…

2019 Astronomy and Astrophysics
Gaia 42
Machine-learning approaches to exoplanet transit detection and candidate validation in wide-field ground-based surveys
DOI: 10.1093/mnras/sty3146 Bibcode: 2019MNRAS.483.5534S

Bouchy, F.; Queloz, D.; Boumis, P. +23 more

Since the start of the Wide-angle Search for Planets (WASP) program, more than 160 transiting exoplanets have been discovered in the WASP data. In the past, possible transit-like events identified by the WASP pipeline have been vetted by human inspection to eliminate false alarms and obvious false positives. The goal of this paper is to assess the…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 42
Multiple Temperature Components of the Hot Circumgalactic Medium of the Milky Way
DOI: 10.3847/1538-4357/ab5846 Bibcode: 2019ApJ...887..257D

Nicastro, Fabrizio; Mathur, Smita; Gupta, Anjali +2 more

We present a deep XMM-Newton observation of the Galactic halo emission in the direction of the blazar 1ES 1553+113. In order to extract the Galactic halo component from the diffuse soft X-ray emission spectrum, accurately modeling the foreground components is crucial. Here we present complex modeling of the foregrounds with unprecedented details. …

2019 The Astrophysical Journal
XMM-Newton 42