Search Publications

Detecting Solar System Analogs through Joint Radial Velocity/Astrometric Surveys
DOI: 10.3847/1538-3881/ad05cc Bibcode: 2023AJ....166..258Y

Angus, Ruth; Foreman-Mackey, Daniel; Spergel, David N. +1 more

Earth-mass exoplanets on year-long orbits and cool gas giants (CGG) on decade-long orbits lie at the edge of current detection limits. The Terra Hunting Experiment (THE) will take nightly radial velocity (RV) observations on HARPS3 of at least 40 bright nearby G and K dwarfs for 10 yr, with a target 1σ measurement error of ~0.3 m s-1, i…

2023 The Astronomical Journal
Gaia 5
Small-scale EUV features as the drivers of coronal upflows in the quiet Sun
DOI: 10.1051/0004-6361/202346036 Bibcode: 2023A&A...674A.219S

Teriaca, Luca; Long, David M.; Schühle, Udo +18 more

Context. Coronal upflows in the quiet Sun are seen in a wide range of features, including jets and filament eruptions. The in situ measurements from Parker Solar Probe within ≈0.2 au have demonstrated that the solar wind is highly structured, showing abrupt and near-ubiquitous magnetic field reversals (i.e., switchbacks) on different timescales. T…

2023 Astronomy and Astrophysics
Hinode IRIS SolarOrbiter 5
Stellar-reddening-based Extinction Maps for Cosmological Applications
DOI: 10.3847/1538-4357/acc32c Bibcode: 2023ApJ...949...47M

Finkbeiner, Douglas P.; Mudur, Nayantara; Park, Core Francisco

Cosmological surveys must correct their observations for the reddening of extragalactic objects by Galactic dust. Existing dust maps, however, have been found to have spatial correlations with the large-scale structure of the Universe. Errors in extinction maps can propagate systematic biases into samples of dereddened extragalactic objects and in…

2023 The Astrophysical Journal
Gaia 5
To grow old and peculiar: Survey of anomalous variable stars in M80 with age determinations using K2 and Gaia
DOI: 10.1051/0004-6361/202346507 Bibcode: 2023A&A...678A.104M

Pál, András; Kinemuchi, Karen; Kollmeier, Juna A. +11 more

The globular cluster Messier 80 was monitored by the Kepler space telescope for 80 days during the K2 mission. Continuous, high-precision photometry of such an old, compact cluster allows us for studies of its variable star population in unprecedented detail. We used differential-image photometry to extract light curves for 27 variable stars A sea…

2023 Astronomy and Astrophysics
Gaia 5
The Large Deficit of HMXB Emission from Luminous Infrared Galaxies: The Case of the Circumnuclear Starburst Ring in NGC 7552
DOI: 10.3847/1538-4357/acd9aa Bibcode: 2023ApJ...952...22W

Zezas, Andreas; Roberts, Timothy P.; West, Lacey +5 more

Luminous infrared galaxies (LIRGs), the most extreme star-forming galaxies in the nearby (D < 30 Mpc) universe, show a notable X-ray emission deficiency (up to a factor of ~10) compared with predictions from scaling relations of galaxy-wide high-mass X-ray binary (HMXB) luminosity with star formation rate. In the nearby (≈20 Mpc) LIRG NGC 7552,…

2023 The Astrophysical Journal
eHST 5
NGTS clusters survey - V. Rotation in the Orion star-forming complex
DOI: 10.1093/mnras/stad1435 Bibcode: 2023MNRAS.523..169S

Ramsay, Gavin; Wheatley, Peter J.; Moyano, Maximiliano +16 more

We present a study of rotation across 30 square degrees of the Orion Star-forming Complex, following a ~200 d photometric monitoring campaign by the Next Generation Transit Survey (NGTS). From 5749 light curves of Orion members, we report periodic signatures for 2268 objects and analyse rotation period distributions as a function of colour for 178…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Asteroseismic modelling strategies in the PLATO era. I. Mean density inversions and direct treatment of the seismic information
DOI: 10.1051/0004-6361/202346258 Bibcode: 2023A&A...676A..10B

Bétrisey, J.; Buldgen, G.; Reese, D. R. +6 more

Context. Asteroseismology experienced a breakthrough in the last two decades thanks to the so-called photometry revolution with space-based missions such as CoRoT, Kepler, and TESS. Because asteroseismic modelling will be part of the pipeline of the future PLATO mission, it is relevant to compare some of the current modelling strategies and discus…

2023 Astronomy and Astrophysics
Gaia 5
Intriguing Plasma Composition Pattern in a Solar Active Region: A Result of Nonresonant Alfvén Waves?
DOI: 10.3847/1538-4357/ad05bf Bibcode: 2023ApJ...959...72M

Stangalini, Marco; Long, David M.; Brooks, David H. +6 more

The plasma composition of the solar corona is different from that of the solar photosphere. Elements that have a low first ionization potential (FIP) are preferentially transported to the corona and therefore show enhanced abundances in the corona compared to the photosphere. The level of enhancement is measured using the FIP bias parameter. In th…

2023 The Astrophysical Journal
Hinode 5
How Magnetic Reconnection May Affect the Coherence of Interplanetary Coronal Mass Ejections
DOI: 10.3847/1538-4357/acdcf7 Bibcode: 2023ApJ...953...15F

Farrugia, C. J.; Galvin, A. B.; Davies, E. E. +12 more

On 2020 April 19-20, a solar ejection was seen by spacecraft in a radial alignment that included Solar Orbiter and Wind. The ejection contained a magnetic flux rope where magnetic field and plasma parameters were well correlated between spacecraft. This structure is called an "unperturbed magnetic flux rope" (UMFR). Ahead of the UMFR is a portion …

2023 The Astrophysical Journal
SolarOrbiter 5
Internal Calibration of LAMOST and Gaia DR3 GSP-Spec Stellar Abundances
DOI: 10.3847/1538-4357/accf8b Bibcode: 2023ApJ...950..104N

Niu, Zexi; Liu, Jifeng; Yuan, Haibo

Stellar chemical abundances are crucial and fundamental in astrophysics. However, they could suffer from substantial systematic errors according to several investigations but still lack calibrations in bulk. By using Gaia wide binaries, we find the temperature-dependent bias between the two binary components for [Fe/H] and [α/Fe] measurements from…

2023 The Astrophysical Journal
Gaia 5