Search Publications

Discovery of a variable energy-dependent X-ray polarization in the accreting neutron star GX 5−1
DOI: 10.1051/0004-6361/202347374 Bibcode: 2024A&A...684A.137F

Kaaret, Philip; Wu, Kinwah; Steiner, James F. +116 more

We report on the coordinated observations of the neutron star low-mass X-ray binary (NS-LMXB) GX 5−1 in X-rays (IXPE, NICER, NuSTAR, and INTEGRAL), optical (REM and LCO), near-infrared (REM), mid-infrared (VLT VISIR), and radio (ATCA). This Z-source was observed by IXPE twice in March-April 2023 (Obs. 1 and 2). In the radio band the source was det…

2024 Astronomy and Astrophysics
INTEGRAL 31
UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at z spec = 3.97
DOI: 10.3847/1538-4357/ad6a18 Bibcode: 2024ApJ...974..145S

Glazebrook, Karl; Nanayakkara, Themiya; van Dokkum, Pieter +28 more

We report the spectroscopic confirmation of a massive ( log(M/M

2024 The Astrophysical Journal
JWST 31
Ionized Gas Kinematics with FRESCO: An Extended, Massive, Rapidly Rotating Galaxy at z = 5.4
DOI: 10.3847/2041-8213/ad7b17 Bibcode: 2024ApJ...976L..27N

Maseda, Michael V.; Übler, Hannah; Bunker, Andrew J. +43 more

With the remarkable sensitivity and resolution of JWST in the infrared, measuring rest-optical kinematics of galaxies at z > 5 has become possible for the first time. This study pilots a new method for measuring galaxy dynamics for highly multiplexed, unbiased samples by combining FRESCO NIRCam grism spectroscopy and JADES medium-band imaging. …

2024 The Astrophysical Journal
JWST 31
Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWST
DOI: 10.3847/1538-4357/ad5290 Bibcode: 2024ApJ...971...43M

Stiavelli, Massimo; Treu, Tommaso; Trenti, Michele +10 more

We present deep JWST NIRSpec observations in the sight line of MACS J1149.5+2223, a massive cluster of galaxies at z = 0.54. We report the spectroscopic redshift of 28 sources at 3 < z < 9.1, including nine sources with the detection of the

2024 The Astrophysical Journal
eHST JWST 31
Stellar flares
DOI: 10.1007/s41116-024-00039-4 Bibcode: 2024LRSP...21....1K

Kowalski, Adam F.

Magnetic storms on stars manifest as remarkable, randomly occurring changes of the luminosity over durations that are tiny in comparison to the normal evolution of stars. These stellar flares are bursts of electromagnetic radiation from X-ray to radio wavelengths, and they occur on most stars with outer convection zones. They are analogous to the …

2024 Living Reviews in Solar Physics
Gaia 31
Testing EMRI Models for Quasi-periodic Eruptions with 3.5 yr of Monitoring eRO-QPE1
DOI: 10.3847/1538-4357/ad2941 Bibcode: 2024ApJ...965...12C

Remillard, Ronald A.; Maccarone, Thomas J.; Burdge, Kevin B. +13 more

Quasi-periodic eruptions (QPEs) are luminous X-ray outbursts recurring on hour timescales, observed from the nuclei of a growing handful of nearby low-mass galaxies. Their physical origin is still debated, and usually modeled as (a) accretion disk instabilities or (b) interaction of a supermassive black hole (SMBH) with a lower mass companion in a…

2024 The Astrophysical Journal
XMM-Newton 30
Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13
DOI: 10.3847/1538-4357/ad7d03 Bibcode: 2024ApJ...975..178K

Finkelstein, Steven L.; Casey, Caitlin M.; Larson, Rebecca L. +8 more

The James Webb Space Telescope (JWST) has uncovered a ubiquitous population of dust-obscured compact sources at z ≳ 4. Many of these objects exhibit signs of active galactic nucleus (AGN) activity, making their study crucial for understanding the formation of supermassive black holes (SMBHs) and their growth with host galaxies. In this work, we ex…

2024 The Astrophysical Journal
JWST 30
A double take on early and interacting dark energy from JWST
DOI: 10.1088/1475-7516/2024/05/097 Bibcode: 2024JCAP...05..097F

Melchiorri, Alessandro; Mena, Olga; Nunes, Rafael C. +4 more

The very first light captured by the James Webb Space Telescope (JWST) revealed a population of galaxies at very high redshifts more massive than expected in the canonical ΛCDM model of structure formation. Barring, among others, a systematic origin of the issue, in this paper, we test alternative cosmological perturbation histories. We argue that…

2024 Journal of Cosmology and Astroparticle Physics
JWST 30
Beyond Gaia DR3: Tracing the [α/M] - [M/H] bimodality from the inner to the outer Milky Way disc with Gaia-RVS and convolutional neural networks
DOI: 10.1051/0004-6361/202347122 Bibcode: 2024A&A...682A...9G

Guiglion, G.; Fabbro, S.; Valentini, M. +17 more

Context. In June 2022, Gaia DR3 provided the astronomy community with about one million spectra from the Radial Velocity Spectrometer (RVS) covering the CaII triplet region. In the next Gaia data releases, we anticipate the number of RVS spectra to successively increase from several 10 million spectra to eventually more than 200 million spectra. T…

2024 Astronomy and Astrophysics
Gaia 30
A mature quasar at cosmic dawn revealed by JWST rest-frame infrared spectroscopy
DOI: 10.1038/s41550-024-02273-0 Bibcode: 2024NatAs...8.1054B

Henning, Thomas; Costantin, Luca; Langeroodi, Danial +29 more

The rapid assembly of the first supermassive black holes is an enduring mystery. Until now, it was not known whether quasar `feeding' structures (the `hot torus') could assemble as fast as the smaller-scale quasar structures. We present JWST/MRS (rest-frame infrared) spectroscopic observations of the quasar J1120+0641 at z = 7.0848 (well within th…

2024 Nature Astronomy
JWST 30