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PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-domain Field II
DOI: 10.3847/1538-4357/ad2b61 Bibcode: 2024ApJ...965..188Z

Koekemoer, Anton M.; Yan, Haojing; Willmer, Christopher N. A. +30 more

We present the second NuSTAR and XMM-Newton extragalactic survey of the JWST north ecliptic pole (NEP) time-domain field (TDF). The first NuSTAR NEP-TDF survey had 681 ks total exposure time executed in NuSTAR cycle 5 in 2019 and 2020. This second survey, acquired from 2020 to 2022 in cycle 6, adds 880 ks of NuSTAR exposure time. The overall NuSTA…

2024 The Astrophysical Journal
Gaia XMM-Newton eHST JWST 8
Limits on Planetary-mass Primordial Black Holes from the OGLE High-cadence Survey of the Magellanic Clouds
DOI: 10.3847/2041-8213/ad8e68 Bibcode: 2024ApJ...976L..19M

Udalski, Andrzej; Mróz, Przemek; Szymański, Michał K. +11 more

Observations of the Galactic bulge revealed an excess of short-timescale gravitational microlensing events that are generally attributed to a large population of free-floating or wide-orbit exoplanets. However, in recent years, some authors suggested that planetary-mass primordial black holes (PBHs) comprising a substantial fraction (1%–10%) of th…

2024 The Astrophysical Journal
Gaia 8
ALMA-IMF. XII. Point-process mapping of 15 massive protoclusters
DOI: 10.1051/0004-6361/202348984 Bibcode: 2024A&A...687A.217D

Galván-Madrid, R.; Cunningham, N.; Csengeri, T. +29 more

Context. A crucial aspect in addressing the challenge of measuring the core mass function (CMF), that is pivotal for comprehending the origin of the initial mass function (IMF), lies in constraining the temperatures of the cores.
Aims: We aim to measure the luminosity, mass, column density and dust temperature of star-forming regions imaged b…

2024 Astronomy and Astrophysics
Herschel 8
Rotation plays a role in the generation of magnetic fields in single white dwarfs
DOI: 10.1093/mnras/stae307 Bibcode: 2024MNRAS.528.6056H

Bell, Keaton J.; Parsons, Steven G.; Landstreet, John D. +5 more

Recent surveys of close white dwarf binaries as well as single white dwarfs have provided evidence for the late appearance of magnetic fields in white dwarfs, and a possible generation mechanism, a crystallization and rotation-driven dynamo has been suggested. A key prediction of this dynamo is that magnetic white dwarfs rotate, at least on averag…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 8
The PIPER survey. II. The globular cluster systems of low surface brightness galaxies in the Perseus cluster
DOI: 10.1093/mnras/stae2137 Bibcode: 2024MNRAS.534..783J

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P. +7 more

We present Hubble Space Telescope ACS/WFC and WFC3/UVIS imaging for a sample of 50 low-surface brightness (LSB) galaxies in the $\sim 10^{15}$ M$_{\odot }$ Perseus cluster, which were…

2024 Monthly Notices of the Royal Astronomical Society
eHST 8
DAVOS: Dwarf Active Galactic Nuclei from Variability for the Origins of Seeds: Properties of Variability-selected Active Galactic Nuclei in the COSMOS Field and Expectations for the Rubin Observatory
DOI: 10.3847/1538-4357/ad54ca Bibcode: 2024ApJ...971..140B

Greene, Jenny E.; Natarajan, Priyamvada; Liu, Xin +3 more

We study the black hole mass–host galaxy stellar mass relation, M BH–M *, of a sample of z < 4 optically variable active galactic nuclei (AGNs) in the COSMOS field. The parent sample of 491 COSMOS AGNs were identified by optical variability from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) program. Using public…

2024 The Astrophysical Journal
eHST JWST 8
Re-energization of AGN head-tail radio galaxies in the galaxy cluster ZwCl 0634.1+47474
DOI: 10.1093/mnras/stad3962 Bibcode: 2024MNRAS.528..141L

Di Gennaro, G.; Brunetti, G.; Shimwell, T. W. +10 more

Low-frequency radio observations show an increasing number of radio galaxies located in galaxy clusters that display peculiar morphologies and spectral profiles. This is the result of the dynamical interaction of the galaxy with the surrounding medium. Studying this phenomenon is key to understanding the evolution of low-energy relativistic partic…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 8
Observation of Alfvén Wave Reflection in the Solar Chromosphere: Ponderomotive Force and First Ionization Potential Effect
DOI: 10.1103/PhysRevLett.132.215201 Bibcode: 2024PhRvL.132u5201M

Stangalini, Marco; Long, David M.; Brooks, David H. +7 more

We investigate the propagation of Alfvén waves in the solar chromosphere, distinguishing between upward and downward propagating waves. We find clear evidence for the reflection of waves in the chromosphere and differences in propagation between cases with waves interpreted to be resonant or nonresonant with the overlying coronal structures. This …

2024 Physical Review Letters
Hinode 8
The accretion burst of the massive young stellar object G323.46−0.08
DOI: 10.1051/0004-6361/202449891 Bibcode: 2024A&A...688A...8W

Matter, A.; Eislöffel, J.; Stecklum, B. +10 more

Context. Accretion bursts from low-mass young stellar objects (YSOs) have been known for many decades. In recent years, the first accretion bursts of massive YSOs (MYSOs) have been observed. These phases of intense protostellar growth are of particular importance for studying massive star formation. Bursts of MYSOs are accompanied by flares of Cla…

2024 Astronomy and Astrophysics
AKARI Gaia 8
Astrometric search for ultralight dark matter
DOI: 10.1103/PhysRevD.110.083031 Bibcode: 2024PhRvD.110h3031K

Kim, Hyungjin

Precision astrometry offers a way to probe new physics. By measuring the angular position of light sources at unprecedented precision, astrometry could probe minuscule fluctuations of underlying spacetime. This work explores the possibility of probing ultralight dark matter candidates using precision astrometry. Through the coherent and stochastic…

2024 Physical Review D
Gaia 8