Search Publications

Patches of Magnetic Switchbacks and Their Origins
DOI: 10.3847/1538-4357/ac7c11 Bibcode: 2022ApJ...934..152S

de Wit, Thierry Dudok; Velli, Marco; Bale, Stuart D. +18 more

Parker Solar Probe (PSP) has shown that the solar wind in the inner heliosphere is characterized by the quasi omnipresence of magnetic switchbacks ("switchback" hereinafter), local backward bends of magnetic field lines. Switchbacks also tend to come in patches, with a large-scale modulation that appears to have a spatial scale size comparable to …

2022 The Astrophysical Journal
Hinode 24
Confirmation of Water Absorption in the Thermal Emission Spectrum of the Hot Jupiter WASP-77Ab with HST/WFC3
DOI: 10.3847/1538-3881/ac658f Bibcode: 2022AJ....163..261M

Fortney, Jonathan J.; Stevenson, Kevin B.; Désert, Jean-Michel +11 more

Secondary eclipse observations of hot Jupiters can reveal both their compositions and thermal structures. Previous observations have shown a diversity of hot Jupiter eclipse spectra, including absorption features, emission features, and featureless blackbody-like spectra. We present a secondary eclipse spectrum of the hot Jupiter WASP-77Ab observe…

2022 The Astronomical Journal
eHST 24
Luminosity functions of globular clusters in five nearby spiral galaxies using HST/ACS images
DOI: 10.1093/mnras/stab2890 Bibcode: 2022MNRAS.509..180L

Mayya, Y. D.; Rosa-González, D.; Rodríguez-Merino, L. H. +2 more

We here present the luminosity function (LF) of globular clusters (GCs) in five nearby spiral galaxies using the samples of GC candidates selected in Hubble Space Telescope mosaic images in F435W, F555W, and F814W filters. Our search, which surpasses the fractional area covered by all previous searches in these galaxies, has resulted in the detect…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 24
High-precision chemical abundances of Galactic building blocks. II. Revisiting the chemical distinctness of the Helmi streams
DOI: 10.1051/0004-6361/202243609 Bibcode: 2022A&A...665A..46M

Hattori, Kohei; Helmi, Amina; Ishigaki, Miho N. +6 more

Context. The Helmi streams are a kinematic substructure whose progenitor is likely a dwarf galaxy. Although 20 years have passed since their discovery, it is still unclear whether their members are chemically distinguishable from other halo stars in the Milky Way.
Aims: We aim to precisely characterize the chemical properties of the Helmi str…

2022 Astronomy and Astrophysics
Gaia 24
Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies
DOI: 10.1051/0004-6361/202243866 Bibcode: 2022A&A...667A..35R

Morisset, C.; Schaerer, D.; Ramambason, L. +8 more

Local metal-poor galaxies stand as ideal laboratories for probing the properties of the interstellar medium (ISM) in chemically unevolved conditions. Detailed studies of this primitive ISM can help gain insights into the physics of the first primordial galaxies that may be responsible for the reionization. Quantifying the ISM porosity to ionizing …

2022 Astronomy and Astrophysics
Herschel 24
Performance of near-infrared high-contrast imaging methods with JWST from commissioning
DOI: 10.1117/12.2628865 Bibcode: 2022SPIE12180E..3NK

Carter, Aarynn L.; Perrin, Marshall D.; Pueyo, Laurent +12 more

The James Webb Space Telescope (JWST) will revolutionize the field of high-contrast imaging and enable both the direct detection of Saturn-mass planets and the characterization of substellar companions in the mid-infrared. While JWST will feature unprecedented sensitivity, angular resolution will be the key factor when competing with ground-based …

2022 Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave
JWST 24
Superresolution trends in the ALMA Taurus survey: structured inner discs and compact discs
DOI: 10.1093/mnras/stac1770 Bibcode: 2022MNRAS.514.6053J

Tazzari, Marco; Rosotti, Giovanni P.; Clarke, Cathie J. +2 more

The 1.33-mm survey of protoplanetary discs in the Taurus molecular cloud found annular gaps and rings to be common in extended sources (≳ 55AU), when their 1D visibility distributions were fit parametrically. We first demonstrate the advantages and limitations of non-parametric visibility fits for data at the survey's 0.12-arcsec resolution. Then …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 24
First light for GRAVITY Wide. Large separation fringe tracking for the Very Large Telescope Interferometer
DOI: 10.1051/0004-6361/202243941 Bibcode: 2022A&A...665A..75G

Lutz, D.; Förster Schreiber, N. M.; Genzel, R. +114 more

GRAVITY+ is the upgrade for GRAVITY and the Very Large Telescope Interferometer (VLTI) with wide-separation fringe tracking, new adaptive optics, and laser guide stars on all four 8 m Unit Telescopes (UTs) to enable ever-fainter, all-sky, high-contrast, milliarcsecond interferometry. Here we present the design and first results of the first phase …

2022 Astronomy and Astrophysics
Gaia 24
A Maximum Likelihood Calibration of the Tip of the Red Giant Branch Luminosity from High Latitude Field Giants Using Gaia Early Data Release 3 Parallaxes
DOI: 10.3847/1538-4357/ac7559 Bibcode: 2022ApJ...939...96L

Casertano, Stefano; Li, Siyang; Riess, Adam G.

The calibration of the tip of the red giant branch (TRGB) in the I band has a direct role in determinations of the Hubble constant, a subject of recent interest due to the discrepancy between direct and indirect estimates of its value. We present a maximum likelihood method designed to obtain an independent calibration of the brightness of TRGB us…

2022 The Astrophysical Journal
Gaia 24
Orbital and dynamical analysis of the system around HR 8799. New astrometric epochs from VLT/SPHERE and LBT/LUCI
DOI: 10.1051/0004-6361/202243862 Bibcode: 2022A&A...666A.133Z

Avenhaus, H.; Marzari, F.; Henning, Th. +45 more

Context. HR 8799 is a young planetary system composed of four planets and a double debris belt. Being the first multi-planetary system discovered with the direct imaging technique, it has been observed extensively since 1998. This wide baseline of astrometric measurements, counting over 50 observations in 20 years, permits a detailed orbital and d…

2022 Astronomy and Astrophysics
Gaia eHST 24