Search Publications

A Census of the Stellar Populations in the Sco-Cen Complex
DOI: 10.3847/1538-3881/ac35e2 Bibcode: 2022AJ....163...24L

Luhman, K. L.

I have used high-precision photometry and astrometry from the early installment of the third data release of Gaia (EDR3) to perform a survey for members of the stellar populations within the Sco-Cen complex, which consist of Upper Sco, UCL/LCC, the V1062 Sco group, Ophiuchus, and Lupus. Among Gaia sources with σ π < 1 mas, I have i…

2022 The Astronomical Journal
Gaia 41
ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets
DOI: 10.3847/1538-4357/ac4399 Bibcode: 2022ApJ...926..120V

Jenkins, Jon M.; Caldwell, Douglas A.; Twicken, Joseph D. +10 more

The Kepler and Transiting Exoplanet Survey Satellite (TESS) missions have generated over 100,000 potential transit signals that must be processed in order to create a catalog of planet candidates. During the past few years, there has been a growing interest in using machine learning to analyze these data in search of new exoplanets. Different from…

2022 The Astrophysical Journal
Gaia 41
Constraining the original composition of the gas forming first-generation stars in globular clusters
DOI: 10.1093/mnras/stac734 Bibcode: 2022MNRAS.513..735L

Milone, A. P.; Cordoni, G.; Marino, A. F. +13 more

Disentangling distinct stellar populations along the red-giant branches (RGBs) of globular clusters (GCs) is possible by using the pseudo-two-colour diagram dubbed chromosome map (ChM). One of the most intriguing findings is that the so-called first-generation (1G) stars, characterized by the same chemical composition of their natal cloud, exhibit…

2022 Monthly Notices of the Royal Astronomical Society
eHST 41
Milky Way Star Clusters and Gaia: A Review of the Ongoing Revolution
DOI: 10.3390/universe8020111 Bibcode: 2022Univ....8..111C

Cantat-Gaudin, Tristan

The unprecedented quality of the astrometric measurements obtained with the ESA Gaia spacecraft have initiated a revolution in Milky Way astronomy. Studies of star clusters in particular have been transformed by the precise proper motions and parallaxes measured by Gaia over the entire sky as well as Gaia's deep all-sky photometry. This paper pres…

2022 Universe
Gaia 41
X-ray detection of a nova in the fireball phase
DOI: 10.1038/s41586-022-04635-y Bibcode: 2022Natur.605..248K

Wilms, Jörn; Haberl, Frank; Rauch, Thomas +17 more

Novae are caused by runaway thermonuclear burning in the hydrogen-rich envelopes of accreting white dwarfs, which leads to a rapid expansion of the envelope and the ejection of most of its mass1,2. Theory has predicted the existence of a `fireball' phase following directly on from the runaway fusion, which should be observable as a shor…

2022 Nature
Gaia 40
Spi-OPS: Spitzer and CHEOPS confirm the near-polar orbit of MASCARA-1 b and reveal a hint of dayside reflection
DOI: 10.1051/0004-6361/202141645 Bibcode: 2022A&A...658A..75H

Alonso, R.; Deleuil, M.; Erikson, A. +82 more

Context. The light curves of tidally locked hot Jupiters transiting fast-rotating, early-type stars are a rich source of information about both the planet and star, with full-phase coverage enabling a detailed atmospheric characterisation of the planet. Although it is possible to determine the true spin-orbit angle Ψ - a notoriously difficult para…

2022 Astronomy and Astrophysics
CHEOPS Gaia 40
Characterizing Extreme Emission Line Galaxies. II. A Self-consistent Model of Their Ionizing Spectrum
DOI: 10.3847/1538-4357/ac8f2c Bibcode: 2022ApJ...938...16O

Skillman, Evan D.; Chisholm, John; Erb, Dawn K. +3 more

Observations of high-redshift galaxies (z > 5) have shown that these galaxies have extreme emission lines with equivalent widths much larger than their local star-forming counterparts. Extreme emission line galaxies (EELGs) in the nearby universe are likely analogs to galaxies during the Epoch of Reionization and provide nearby laboratories to …

2022 The Astrophysical Journal
eHST 40
The GALAH survey: chemical clocks
DOI: 10.1093/mnras/stac2787 Bibcode: 2022MNRAS.517.5325H

Lewis, Geraint F.; Casey, Andrew R.; Buder, Sven +29 more

We present the first large-scale study that demonstrates how ages can be determined for large samples of stars through Galactic chemical evolution. Previous studies found that the elemental abundances of a star correlate directly with its age and metallicity. Using this knowledge, we derive ages for 214 577 stars in GALAH DR3 using only overall me…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 40
A3COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time
DOI: 10.1051/0004-6361/202142299 Bibcode: 2022A&A...660A.142W

Schinnerer, Eva; Liu, Daizhong; Kokorev, Vasily +6 more


Aims: We aim to constrain for the first time the mean mass and extent of the molecular gas of a mass-complete sample of normal > 1010 M star-forming galaxies at 0.4 < z < 3.6.
Methods: We apply an innovative uv-based stacking analysis to a large set of archival Atacama Large Millimeter/submillimeter Array …

2022 Astronomy and Astrophysics
Herschel 40
Cosmic evolution of low-excitation radio galaxies in the LOFAR two-metre sky survey deep fields
DOI: 10.1093/mnras/stac1128 Bibcode: 2022MNRAS.513.3742K

Calistro Rivera, Gabriela; Małek, Katarzyna; Wang, Lingyu +16 more

Feedback from low-excitation radio galaxies (LERGs) plays a key role in the lifecycle of massive galaxies in the local Universe; their evolution, and the impact of these active galactic nuclei on early galaxy evolution, however, remain poorly understood. We use a sample of 10 481 LERGs from the first data release of the LOFAR two-metre Sky Survey …

2022 Monthly Notices of the Royal Astronomical Society
Herschel 40