Search Publications

TEMPLATES: Characterization of a Merger in the Dusty Lensing SPT0418–47 System
DOI: 10.3847/1538-4357/ad33c9 Bibcode: 2024ApJ...967...11C

Hutchison, Taylor A.; Mahler, Guillaume; Rigby, Jane R. +24 more

We present JWST and Atacama Large Millimeter/submillimeter Array (ALMA) imaging for the lensing system SPT0418‑47, which includes a strongly lensed, dusty, star-forming galaxy at redshift z = 4.225 and an associated multiply imaged companion. The JWST NIRCam and MIRI imaging observations presented in this paper were acquired as part of the Early R…

2024 The Astrophysical Journal
JWST 8
X-ray view of dissipative warm corona in active galactic nuclei
DOI: 10.1051/0004-6361/202450111 Bibcode: 2024A&A...690A.308P

Bianchi, S.; Petrucci, P. O.; Belmont, R. +8 more

Context. Detections of the X-ray spectra of active galactic nuclei (AGNs) typically reveal a noticeable excess of soft X-rays beyond the extrapolation of the power-law trend observed between 2 and 10 keV. However, the cause of this surplus remains unclear. In the scenario of soft Comptonization, observations suggest a warm corona temperature, rang…

2024 Astronomy and Astrophysics
XMM-Newton 8
E-XQR-30: The evolution of Mg II, C II, and O I across 2 < z < 6
DOI: 10.1093/mnras/stae789 Bibcode: 2024MNRAS.530.1829S

Lai, Samuel; Bosman, Sarah E. I.; Meyer, Romain A. +12 more

Intervening metal absorbers in quasar spectra at z > 6 can be used as probes to study the chemical enrichment of the Universe during the Epoch of Reionization. This work presents the comoving line densities (dn/dX) of low-ionization absorbers, namely, Mg II (2796 Å), C II (1334 Å), and O I (1302 Å) across 2 < z < 6 using the E-XQR-30 meta…

2024 Monthly Notices of the Royal Astronomical Society
JWST 8
Hunting down white dwarf-main sequence binaries using multiwavelength observations
DOI: 10.1093/mnras/stad3580 Bibcode: 2024MNRAS.527.6100N

Chatterjee, Sourav; Nayak, Prasanta K.; Ganguly, Anindya

Identification of white dwarfs (WD) with main-sequence (MS) companions and characterization of their properties can put important constraints on our understanding of binary stellar evolution and guide the theoretical predictions for a wide range of interesting transient events relevant for, e.g. Rubin Observatory (LSST), ZTF, and LISA. In this stu…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 8
Mid-infrared Spectrum of the Disk around the Forming Companion GQ Lup B Revealed by JWST/MIRI
DOI: 10.3847/2041-8213/ad3cbc Bibcode: 2024ApJ...966L..21C

Banzatti, Andrea; MacDonald, Ryan J.; Stolker, Tomas +5 more

GQ Lup B is a forming brown dwarf companion (M ∼ 10–30 M J) showing evidence for an infrared excess associated with a disk surrounding the companion itself. Here we present mid-infrared (MIR) observations of GQ Lup B with the Medium Resolution Spectrometer (MRS) on JWST, spanning 4.8–11.7 µm. We remove the stellar contamination us…

2024 The Astrophysical Journal
JWST 8
A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Impact of Galaxies on the Circumgalactic Medium Metal Enrichment at z > 6 Using the JWST and VLT
DOI: 10.3847/2041-8213/ad23e7 Bibcode: 2024ApJ...963L..28Z

Chevallard, Jacopo; Hennawi, Joseph F.; Fan, Xiaohui +27 more

We characterize the multiphase circumgalactic medium (CGM) and galaxy properties at z = 6.0–6.5 in four quasar fields from the James Webb Space Telescope A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE) program. We use the Very Large Telescope/X-shooter spectra of quasar J0305–3150 to identify one new metal absorber at z = 6…

2024 The Astrophysical Journal
eHST JWST 8
Examining the nature of the ultraluminous X-ray source Holmberg II X-1
DOI: 10.1051/0004-6361/202348471 Bibcode: 2024A&A...682A..94B

Pinto, C.; Di Salvo, T.; Roberts, T. P. +4 more

We present a comprehensive spectral analysis of the ultraluminous X-ray source Holmberg II X-1 using broadband and high-resolution X-ray spectra taken with the XMM-Newton satellite over a period of 19 yr, taking advantage of data from a recent campaign. We tested several models for the broadband spectra, including a double thermal component provid…

2024 Astronomy and Astrophysics
XMM-Newton 8
Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection
DOI: 10.1051/0004-6361/202347873 Bibcode: 2024A&A...683A..31M

Jebaraj, I. C.; Vainio, R.; Kilpua, E. K. J. +7 more

Context. One of the most prominent sources for energetic particles in our Solar System are huge eruptions of magnetised plasma from the Sun, known as coronal mass ejections (CMEs), which usually drive shocks that accelerate charged particles up to relativistic energies. In particular, energetic electron beams can generate radio bursts through the …

2024 Astronomy and Astrophysics
SOHO SolarOrbiter 8
Secular change in the spin states of asteroids due to radiation and gravitation torques. New detections and updates of the YORP effect
DOI: 10.1051/0004-6361/202348350 Bibcode: 2024A&A...682A..93D

Snodgrass, C.; Ehgamberdiev, Sh. A.; Kučáková, H. +21 more

Context. The rotation state of small asteroids is affected in the long term by perturbing torques of gravitational and radiative origin (the YORP effect). The former can be detected by a change in the spin-axis orientation in the inertial space; the latter manifests itself by a quadratic increase in the rotation phase.
Aims: Direct observatio…

2024 Astronomy and Astrophysics
Gaia 8
No Longer Impossible: The Self-lensing Binary KIC 8145411 is a Triple
DOI: 10.1088/1538-3873/ad5ebd Bibcode: 2024PASP..136g4201Y

Bieryla, Allyson; Latham, David W.; El-Badry, Kareem +5 more

Five self-lensing binaries (SLBs) have been discovered with data from the Kepler mission. One of these systems is KIC 8145411, which was reported to host an extremely low mass (ELM; 0.2 M ) white dwarf (WD) in a 456 days orbit with a solar-type companion. The system has been dubbed "impossible," because evolutionary models predict that…

2024 Publications of the Astronomical Society of the Pacific
Gaia 8