Search Publications

An Edge-on Regular Disk Galaxy at z = 5.289
DOI: 10.3847/1538-4357/ad7de9 Bibcode: 2024ApJ...975...44Y

Yan, Haojing; Ling, Chenxiaoji; Sun, Bangzheng

While rotation-supported gas disks are known to exist as early as at z ≈ 7, it is still a general belief that stellar disks form late in the Universe. This picture is now being challenged by the observations from the James Webb Space Telescope (JWST), which have revealed a large number of disk-like galaxies that could be at z > 3, with some bei…

2024 The Astrophysical Journal
eHST JWST 3
The Timescales of Star Cluster Emergence: The Case of NGC 4449
DOI: 10.3847/1538-4357/ad3e64 Bibcode: 2024ApJ...967..102M

Smith, Linda J.; Calzetti, Daniela; Johnson, Kelsey E. +7 more

We survey the young star cluster population in the dwarf galaxy NGC 4449 with the goal of investigating how stellar feedback may depend on the clusters' properties. Using ultraviolet (UV)–optical–near-infrared photometry obtained with the Hubble Space Telescope, we have recovered 99 compact sources exhibiting emission in the Paβ hydrogen recombina…

2024 The Astrophysical Journal
eHST JWST 3
Pseudo-Drag-Free System Simulation for Bepicolombo Radio Science Using Accelerometer Data
DOI: 10.2514/1.G007916 Bibcode: 2024JGCD...47..685D

Cappuccio, Paolo; di Stefano, Ivan; Iess, Luciano +6 more

The Mercury Orbiter Radio Science Experiment onboard the European Space Agency/Japan Aerospace Exploration Agency (JAXA) BepiColombo mission aims at determining the gravity field and the rotational state of the planet to provide insight into its internal structure and at performing tests of general relativity. The experiment will rely on accurate …

2024 Journal of Guidance Control Dynamics
BepiColombo 3
A disc wind origin for the optical spectra of dwarf novae in outburst
DOI: 10.1093/mnras/stae1557 Bibcode: 2024MNRAS.532.1199T

Long, Knox S.; Tampo, Yusuke; Knigge, Christian +2 more

Many high-state cataclysmic variables (CVs) exhibit blue-shifted absorption features in their ultraviolet (UV) spectra - a smoking-gun signature of outflows. However, the impact of these outflows on optical spectra remains much more uncertain. During its recent outburst, the eclipsing dwarf nova V455 And displayed strong optical emission lines who…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 3
A newborn active galactic nucleus in a star-forming galaxy
DOI: 10.1051/0004-6361/202348900 Bibcode: 2024A&A...683L...8A

Salvato, M.; Merloni, A.; Arévalo, P. +8 more


Aims: We report on the finding of a newborn active galactic nucleus (AGN), based on the observation of current AGN activity in a galaxy previously classified as non-active. We subsequently characterize the AGN's evolution.
Methods: Black hole ignition event candidates were selected from a parent sample of spectrally classified non-active…

2024 Astronomy and Astrophysics
XMM-Newton 3
WFC3 Infrared Spectroscopic Parallel (WISP) survey: photometric and emission-line data release
DOI: 10.1093/mnras/stae911 Bibcode: 2024MNRAS.530..894B

Malkan, M. A.; Wang, X.; Shahinyan, K. +21 more

We present reduced images and catalogues of photometric and emission-line data (~230 000 and ~8000 sources, respectively) for the WFC3 (Wide Field Camera 3) Infrared Spectroscopic Parallel (WISP) survey. These data are made publicly available on the Mikulski Archive for Space Telescopes and include reduced images from various facilities: ground-ba…

2024 Monthly Notices of the Royal Astronomical Society
eHST 3
Assessing the capability of a model-based stellar XUV estimation
DOI: 10.1051/0004-6361/202450129 Bibcode: 2024A&A...691A.152S

Namekata, Kosuke; Takasao, Shinsuke; Shoda, Munehito

Stellar X-ray and extreme ultraviolet (XUV) emission drives the heating and chemical reactions in planetary atmospheres and proto-planetary disks, and therefore, a proper estimation of a stellar XUV spectrum is required for their studies. One proposed solution is to estimate stellar atmospheric heating using numerical models, although the validati…

2024 Astronomy and Astrophysics
eHST 3
TOI-2015 b: A Warm Neptune with Transit Timing Variations Orbiting an Active Mid-type M Dwarf
DOI: 10.3847/1538-3881/ad55ea Bibcode: 2024AJ....168...93J

Kobulnicky, Henry A.; Hawley, Suzanne L.; Cochran, William D. +29 more

We report the discovery of a close-in (P orb = 3.349 days) warm Neptune with clear transit timing variations (TTVs) orbiting the nearby (d = 47.3 pc) active M4 star, TOI-2015. We characterize the planet's properties using Transiting Exoplanet Survey Satellite (TESS) photometry, precise near-infrared radial velocities (RVs) with the Habi…

2024 The Astronomical Journal
Gaia 3
Hemispheric Distribution of Halo Coronal Mass Ejection Source Locations
DOI: 10.3847/1538-4357/ad18af Bibcode: 2024ApJ...962..172Z

Mei, Ying; Wang, Feng; Deng, Hui +2 more

The hemispheric asymmetry of solar activity is one of the essential physical consequences of the interior dynamo process. However, the hemispheric distribution of halo coronal mass ejection (HCME) source locations has not been investigated in detail. Based on the HCME catalog identified from the Large Angle and Spectrometric Coronagraph Experiment…

2024 The Astrophysical Journal
SOHO 3
JWST-TST High Contrast: Spectroscopic Characterization of the Benchmark Brown Dwarf HD 19467 B with the NIRSpec Integral Field Spectrograph
DOI: 10.3847/1538-3881/ad6cd3 Bibcode: 2024AJ....168..187H

van der Marel, Roeland P.; Perrin, Marshall D.; Pueyo, Laurent +14 more

We present the atmospheric characterization of the substellar companion HD 19467 B as part of the pioneering James Webb Space Telescope Guaranteed Time Observer program to obtain moderate resolution spectra (R ∼ 2700, 3–5 µm) of a high-contrast companion with the NIRSpec integral field unit (IFU). HD 19467 B is an old, ∼9 Gyr, companion to a…

2024 The Astronomical Journal
AKARI Gaia JWST 3