Search Publications

Global-scale magnetosphere convection driven by dayside magnetic reconnection
DOI: 10.1038/s41467-024-44992-y Bibcode: 2024NatCo..15..639D

Branduardi-Raymont, Graziella; Wang, Chi; Dai, Lei +8 more

Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part of the magnetosphere relies on magnetic reconnection in the nightside magnetospheric tail. Nevertheless, time-dependent models of the Dungey cycle suggest an alternative scenario whe…

2024 Nature Communications
Cluster 16
CHEOPS in-flight performance. A comprehensive look at the first 3.5 yr of operations
DOI: 10.1051/0004-6361/202348576 Bibcode: 2024A&A...687A.302F

Guterman, P.; Alonso, R.; Deleuil, M. +128 more

Context. Since the discovery of the first exoplanet almost three decades ago, the number of known exoplanets has increased dramatically. By beginning of the 2000s it was clear that dedicated facilities to advance our studies in this field were needed. The CHaracterising ExOPlanet Satellite (CHEOPS) is a space telescope specifically designed to mon…

2024 Astronomy and Astrophysics
CHEOPS Gaia 16
Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High-redshift Galaxies
DOI: 10.3847/1538-4357/ad58e2 Bibcode: 2024ApJ...971...47F

Morishita, Takahiro; Faisst, Andreas L.

The recent discovery of a galaxy at z = 7.3 with undetected optical emission lines and a blue UV-to-optical continuum ratio in JWST spectroscopy is surprising and needs to be explained physically. Here, we explore two possibilities that could cause such a seemingly quiescent ∼5 × 108 M galaxy in the early Universe: (i) stoc…

2024 The Astrophysical Journal
JWST 16
JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs
DOI: 10.1093/mnras/stad3670 Bibcode: 2024MNRAS.528.3392W

Matsuura, Mikako; Volk, Kevin; Cami, Jan +18 more

We present JWST images of the well-known planetary nebula NGC 6720 (the Ring Nebula), covering wavelengths from 1.6 to 25 $\, \mu$m. The bright shell is strongly fragmented with some 20 000 dense globules, bright in H2, with a characteristic diameter of 0.2 arcsec and density nH ~ 105-106 cm-3

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 16
JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b
DOI: 10.3847/2041-8213/ad72e9 Bibcode: 2024ApJ...973L...8X

Eastman, Jason D.; Bean, Jacob L.; Zhang, Michael +9 more

We present thermal emission measurements of GJ 1132b spanning 5–12 µm obtained with the Mid-Infrared Instrument Low-Resolution Spectrometer on the James Webb Space Telescope. GJ 1132b is an M dwarf rocky planet with T eq = 584 K and an orbital period of 1.6 days. We measure a white-light secondary eclipse depth of 140 ± 17 ppm, wh…

2024 The Astrophysical Journal
JWST 16
Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints
DOI: 10.3847/1538-4357/ad41e0 Bibcode: 2024ApJ...968...46D

De la Torre Luque, Pedro; Balaji, Shyam; Koechler, Jordan

We study sub-GeV dark matter (DM) particles that may annihilate or decay into Standard Model particles producing an exotic injection component in the Milky Way that leaves an imprint in both photon and cosmic-ray (CR) fluxes. Specifically, the DM particles may annihilate or decay into e + e , µ + µ

2024 The Astrophysical Journal
XMM-Newton 16
Data reconstruction of the dynamical connection function in f(Q) cosmology
DOI: 10.1093/mnras/stae1905 Bibcode: 2024MNRAS.533.2232Y

Ren, Xin; Wang, Bo; Cai, Yi-Fu +2 more

We employ Hubble data and Gaussian Processes in order to reconstruct the dynamical connection function in $f(Q)$ cosmology beyond the coincident gauge. In particular, there exist three branches of connections that satisfy the torsionless and curvatureless conditions, parametrized by a new dynamical function $\gamma$. We express the redshift depend…

2024 Monthly Notices of the Royal Astronomical Society
eHST 16
Freeze-in production of sterile neutrino dark matter in a gauged U(1)‧ model with inverse seesaw
DOI: 10.1016/j.nuclphysb.2024.116568 Bibcode: 2024NuPhB100416568D

Poddar, Tanmay Kumar; Das, Arindam; Goswami, Srubabati +1 more

We consider a general, anomaly free U(1)‧ extension of the Standard Model (SM) where the neutrino mass is generated at the tree level via the inverse seesaw mechanism. The model contains three right handed neutrinos, three additional singlet fermions, one extra complex scalar and a neutral gauge boson (Z‧). Instead of resorting to a specific U(1) …

2024 Nuclear Physics B
INTEGRAL 16
Proper Motions and Orbits of Distant Local Group Dwarf Galaxies from a Combination of Gaia and Hubble Data
DOI: 10.3847/1538-4357/ad5349 Bibcode: 2024ApJ...971...98B

van der Marel, Roeland P.; Watkins, Laura L.; Sacchi, Elena +12 more

We have determined the proper motions (PMs) of 12 dwarf galaxies in the Local Group (LG), ranging from the outer Milky Way (MW) halo to the edge of the LG. We used the Hubble Space Telescope (HST) as the first and Gaia as the second epoch using the GaiaHub software. For Leo A and Sag DIG, we also used multi-epoch HST measurements relative to backg…

2024 The Astrophysical Journal
Gaia eHST 16
A Rest-frame Near-IR Study of Clumps in Galaxies at 1 < z < 2 Using JWST/NIRCam: Connection to Galaxy Bulges
DOI: 10.3847/1538-4357/acfee4 Bibcode: 2024ApJ...960...25K

Ho, Luis C.; Daddi, Emanuele; Bottrell, Connor +4 more

A key question in galaxy evolution has been the importance of the apparent "clumpiness" of high-redshift galaxies. Until now, this property has been primarily investigated in rest-frame UV, limiting our understanding of their relevance. Are they short-lived or are they associated with more long-lived massive structures that are part of the underly…

2024 The Astrophysical Journal
JWST 16