Search Publications

VLT/MUSE Observations of SDSS J1029+2623: Toward a High-precision Strong Lensing Model
DOI: 10.3847/1538-4357/ac3d35 Bibcode: 2022ApJ...926...86A

Brammer, Gabriel B.; Acebron, Ana; Nonino, Mario +9 more

We present a strong lensing analysis of the galaxy cluster SDSS J1029+2623 at z = 0.588, one of the few currently known lens clusters with multiple images of a background (z = 2.1992) quasar with a measured time delay. We use archival Hubble Space Telescope multiband imaging and new Multi Unit Spectroscopic Explorer follow-up spectroscopy to build…

2022 The Astrophysical Journal
Gaia eHST 23
The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
DOI: 10.1051/0004-6361/202243834 Bibcode: 2022A&A...664A.199L

Amado, P. J.; Caballero, J. A.; Pallé, E. +64 more

We report the discovery of a multiplanetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655 b, with a period of 2.77 d, a radius of Rb = 1.240 ± 0.023 R, a mass of Mb = 2.14 ± 0.34 M, and a bulk density of ρb

2022 Astronomy and Astrophysics
Gaia 23
J-PLUS: Spectral evolution of white dwarfs by PDF analysis
DOI: 10.1051/0004-6361/202141746 Bibcode: 2022A&A...658A..79L

Hernández-Monteagudo, C.; Gänsicke, B. T.; Carrasco, J. M. +17 more


Aims: We estimated the spectral evolution of white dwarfs with effective temperature using the Javalambre Photometric Local Universe Survey (J-PLUS) second data release (DR2), which provides 12 photometric optical passbands over 2176 deg2.
Methods: We analyzed 5926 white dwarfs with r ≤ 19.5 mag in common between a white dwarf…

2022 Astronomy and Astrophysics
Gaia 23
New Photometric Calibration of the Wide Field Camera 3 Detectors
DOI: 10.3847/1538-3881/ac73f0 Bibcode: 2022AJ....164...32C

Mack, Jennifer; Calamida, Annalisa; Medina, Jennifer +6 more

We present a new photometric calibration of the WFC3-UVIS and WFC3-IR detectors based on observations collected from 2009 to 2020 for four white dwarfs-namely, GRW +70 5824, GD 153 , GD 71 , G191B2B-and a G-type star, P330E. These calibrations include recent updates to the Hubble Space Telescope primary standard white dwarf models and a new refere…

2022 The Astronomical Journal
eHST 23
Stellar Loci. V. Photometric Metallicities of 27 Million FGK Stars Based on Gaia Early Data Release 3
DOI: 10.3847/1538-4365/ac3df6 Bibcode: 2022ApJS..258...44X

Huang, Yang; Niu, Zexi; Beers, Timothy C. +3 more

We combine LAMOST DR7 spectroscopic data and Gaia EDR3 photometric data to construct high-quality giant (0.7 < (BP - RP) < 1.4) and dwarf (0.5 < (BP - RP) < 1.5) samples in the high Galactic latitude region, with precise corrections for magnitude-dependent systematic errors in the Gaia photometry and careful reddening corrections using…

2022 The Astrophysical Journal Supplement Series
Gaia 23
Limits on the mass and initial entropy of 51 Eri b from Gaia EDR3 astrometry
DOI: 10.1093/mnras/stab3148 Bibcode: 2022MNRAS.509.4411D

Dupuy, Trent J.; Brandt, Timothy D.; Brandt, G. Mirek

51 Eri b is one of the only young planets consistent with a wide range of possible initial entropy states, including the cold-start scenario associated with some models of planet formation by core accretion. The most direct way to constrain the initial entropy of a planet is by measuring its luminosity and mass at a sufficiently young age that the…

2022 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 23
Bright, relatively isolated star clusters in PHANGS-HST galaxies: Aperture corrections, quantitative morphologies, and comparison with synthetic stellar population models
DOI: 10.1093/mnras/stab3213 Bibcode: 2022MNRAS.510...32D

Kruijssen, J. M. Diederik; Rosolowsky, Erik; Glover, Simon C. O. +14 more

Using PHANGS-HST NUV-U-B-V-I imaging of 17 nearby spiral galaxies, we study samples of star clusters and stellar associations, visually selected to be bright and relatively isolated, for three purposes: to compute aperture corrections for star cluster photometry, to explore the utility of quantitative morphologies in the analysis of clusters and a…

2022 Monthly Notices of the Royal Astronomical Society
eHST 23
The Structure of the Global Heliosphere as Seen by In-Situ Ions from the Voyagers and Remotely Sensed ENAs from Cassini
DOI: 10.1007/s11214-022-00889-0 Bibcode: 2022SSRv..218...21D

Krimigis, Stamatios M.; Mitchell, Donald G.; Hilchenbach, Martin +5 more

The exploration of interplanetary space and our solar bubble, the heliosphere, has made a big leap over the past two decades, due to the path-breaking observations of the two Voyager spacecraft, launched more than 44 years ago. Their in-situ particle and fields measurements were complemented by remote observations of 5.2 to 55 keV Energetic Neutra…

2022 Space Science Reviews
Cassini SOHO 23
Turbulence in Milky Way Star-forming Regions Traced by Young Stars and Gas
DOI: 10.3847/1538-4357/ac76bf Bibcode: 2022ApJ...934....7H

Kounkel, Marina; Li, Hui; Zheng, Yong +3 more

The interstellar medium (ISM) is turbulent over vast scales and in various phases. In this paper, we study turbulence with different tracers in four nearby star-forming regions: Orion, Ophiuchus, Perseus, and Taurus. We combine the APOGEE-2 and Gaia surveys to obtain the full six-dimensional measurements of positions and velocities of young stars …

2022 The Astrophysical Journal
Gaia 23
The evolution of ultra-massive carbon-oxygen white dwarfs
DOI: 10.1093/mnras/stac348 Bibcode: 2022MNRAS.511.5198C

Córsico, Alejandro H.; Althaus, Leandro G.; Torres, Santiago +3 more

Ultra-massive white dwarfs ($\rm \mathit{M}_{WD} \gtrsim 1.05\, {\rm M}_{\odot }$) are considered powerful tools to study Type Ia supernovae explosions, merger events, the occurrence of physical processes in the superasymptotic giant branch phase, and the existence of high magnetic fields. Traditionally, ultra-massive white dwarfs are expected to …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 23