Search Publications

Completeness of the Gaia-verse III: using hidden states to infer gaps, detection efficiencies, and the scanning law from the DR2 light curves
DOI: 10.1093/mnras/staa3791 Bibcode: 2021MNRAS.501.2954B

Everall, Andrew; Boubert, Douglas; Fraser, Jack +2 more

The completeness of the Gaia catalogues heavily depends on the status of that space telescope through time. Stars are only published with each of the astrometric, photometric, and spectroscopic data products if they are detected a minimum number of times. If there is a gap in scientific operations, a drop in the detection efficiency or Gaia deviat…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 15
The Gaia-ESO Survey: Oxygen Abundance in the Galactic Thin and Thick Disks
DOI: 10.3847/1538-3881/abc69b Bibcode: 2021AJ....161....9F

Kordopatis, Georges; Bragaglia, Angela; Adibekyan, Vardan +18 more

We analyze the oxygen abundances of a stellar sample representative of the two major Galactic populations: the thin and thick disks. The aim is to investigate the differences between members of the Galactic disks and contribute to the understanding of the origin of oxygen chemical enrichment in the Galaxy. The analysis is based on the [O I] = 6300…

2021 The Astronomical Journal
Gaia 15
A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113
DOI: 10.1093/mnras/stab182 Bibcode: 2021MNRAS.502.4842O

Bouchy, F.; Deleuil, M.; Helled, R. +53 more

We report the discovery of HD 110113 b (TESS object of interest-755.01), a transiting mini-Neptune exoplanet on a 2.5-d orbit around the solar-analogue HD 110113 (Teff = 5730 K). Using TESS photometry and High Accuracy Radial velocity Planet Searcher (HARPS) radial velocities gathered by the NCORES program, we find that HD 110113 b has …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 15
Investigation of Orbital Decay and Global Modeling of the Planet WASP-43 b
DOI: 10.3847/1538-3881/ac1baf Bibcode: 2021AJ....162..210D

Davoudi, Fatemeh; Safari, Hossein; Baştürk, Özgür +2 more

WASP-43 b is one of the most important candidates for detecting an orbital decay. We investigate pieces of evidence for this expectation as variations in its transit timings, based on the ground and space observations. The data set includes the transit observations at the TÜBİTAK National Observatory of Turkey and Transiting Exoplanet Survey Satel…

2021 The Astronomical Journal
Gaia eHST 15
Searching For Transiting Planets Around Halo Stars. II. Constraining the Occurrence Rate of Hot Jupiters
DOI: 10.3847/1538-3881/ac0e2d Bibcode: 2021AJ....162...85B

Li, Ting S.; Collins, Karen A.; Collins, Kevin I. +4 more

Jovian planet formation has been shown to be strongly correlated with host-star metallicity, which is thought to be a proxy for disk solids. Observationally, previous works have indicated that Jovian planets preferentially form around stars with solar and supersolar metallicities. Given these findings, it is challenging to form planets within meta…

2021 The Astronomical Journal
Gaia 15
OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf
DOI: 10.3847/1538-3881/ac00ba Bibcode: 2021AJ....162...77K

Kim, S. -L.; Lee, C. -U.; Bryden, G. +96 more

We report an analysis of the planetary microlensing event OGLE-2018-BLG-1185, which was observed by a large number of ground-based telescopes and by the Spitzer Space Telescope. The ground-based light curve indicates a low planet-host star mass ratio of q = (6.9 ± 0.2) × 10-5, which is near the peak of the wide-orbit exoplanet mass-rati…

2021 The Astronomical Journal
Gaia eHST 15
An Asymmetric Dust Ring around a Very Low Mass Star ZZ Tau IRS
DOI: 10.3847/1538-3881/abf431 Bibcode: 2021AJ....161..264H

Dong, Ruobing; Hashimoto, Jun; Muto, Takayuki

We present Atacama Large Millimeter/submillimeter Array (ALMA) gas and dust observations at band 7 (339 GHz: 0.89 mm) of the protoplanetary disk around a very low mass star ZZ Tau IRS with a spatial resolution of 0"25. The 12CO J = 3 → 2 position-velocity diagram suggests a dynamical mass of ZZ Tau IRS of ∼0.1-0.3 M. The dis…

2021 The Astronomical Journal
Gaia 15
Massive young stellar objects in the Local Group irregular galaxy NGC 6822 identified using machine learning
DOI: 10.1093/mnras/stab2386 Bibcode: 2021MNRAS.507.5106K

van Loon, Jacco Th; Oliveira, Joana M.; Kinson, David A.

We present a supervised machine learning methodology to classify stellar populations in the Local Group dwarf-irregular galaxy NGC 6822. Near-IR colours (J - H, H - K, and J - K), K-band magnitudes and far-IR surface brightness (at 70 and 160 $\mu$m) measured from Spitzer and Herschel images are the features used to train a Probabilistic Random Fo…

2021 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 15
The dependence of the hierarchical distribution of star clusters on galactic environment
DOI: 10.1093/mnras/stab2413 Bibcode: 2021MNRAS.507.5542M

Grebel, Eva K.; Smith, Linda J.; Calzetti, Daniela +15 more

We use the angular two-point correlation function (TPCF) to investigate the hierarchical distribution of young star clusters in 12 local (3-18 Mpc) star-forming galaxies using star cluster catalogs obtained with the Hubble Space Telescope (HST) as part of the Treasury Program Legacy ExtraGalactic UV Survey. The sample spans a range of different mo…

2021 Monthly Notices of the Royal Astronomical Society
eHST 15
Physical characterization of recently discovered globular clusters in the Sagittarius dwarf spheroidal galaxy. I. Metallicities, ages, and luminosities
DOI: 10.1051/0004-6361/202141067 Bibcode: 2021A&A...654A..23G

Minniti, D.; Alonso-García, J.; Gómez, M. +1 more

Context. Globular clusters (GCs) are important tools for rebuilding the accretion history of a galaxy. In particular, newly discovered GCs in the Sagittarius (Sgr) dwarf galaxy can be used as probes of the accretion event onto the Milky Way (MW).
Aims: Our main aim is to characterize the GC system of the Sgr dwarf galaxy by measuring its main…

2021 Astronomy and Astrophysics
Gaia 15