Search Publications

Radio-loud Quasars above Redshift 4: Very Long Baseline Interferometry (VLBI) Imaging of an Extended Sample
DOI: 10.3847/1538-4365/ac63b8 Bibcode: 2022ApJS..260...49K

Paragi, Zsolt; Krezinger, Máté; Frey, Sándor +7 more

High-redshift radio sources provide plentiful opportunities for studying the formation and evolution of early galaxies and supermassive black holes. However, the number of known radio-loud active galactic nuclei (AGN) above redshift 4 is rather limited. At high redshifts, it appears that blazars, with relativistically beamed jets pointing toward t…

2022 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 18
First Census of Gas-phase Metallicity Gradients of Star-forming Galaxies in Overdense Environments at Cosmic Noon
DOI: 10.3847/2041-8213/ac626f Bibcode: 2022ApJ...929L...8L

Teplitz, Harry I.; Fan, Xiaohui; Cai, Zheng +8 more

We report the first spatially resolved measurements of gas-phase metallicity radial gradients in star-forming galaxies in overdense environments at z ≳ 2. The spectroscopic data are acquired by the MAMMOTH-Grism survey, a Hubble Space Telescope (HST) cycle 28 medium program. This program is obtaining 45 orbits of WFC3/IR grism spectroscopy in the …

2022 The Astrophysical Journal
eHST 18
Detection of Intracluster Globular Clusters in the First JWST Images of the Gravitational Lens Cluster SMACS J0723.3-7327 at z = 0.39
DOI: 10.3847/2041-8213/ac990b Bibcode: 2022ApJ...940L..19L

Lee, Myung Gyoon; Jang, In Sung; Bae, Jang Ho

We present a survey of globular clusters (GCs) in the massive gravitational lens cluster SMACS J0723.3-7327 at z = 0.39 based on the early released JWST/NIRCam images. In the color-magnitude diagrams of the point sources, we clearly find a rich population of intracluster GCs that are spread over a wide area of the cluster. Their ages, considering …

2022 The Astrophysical Journal
JWST 18
Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
DOI: 10.1051/0004-6361/202243683 Bibcode: 2022A&A...667A..77R

Massa, D.; Hamann, W. -R.; Postnov, K. A. +10 more

M33 X-7 is the only known eclipsing black hole high mass X-ray binary. The system is reported to contain a very massive O supergiant donor and a massive black hole in a short orbit. The high X-ray luminosity and its location in the metal-poor galaxy M33 make it a unique laboratory for studying the winds of metal-poor donor stars with black hole co…

2022 Astronomy and Astrophysics
XMM-Newton eHST 18
Weak evidence for variable occultation depth of 55 Cnc e with TESS
DOI: 10.1051/0004-6361/202243768 Bibcode: 2022A&A...663A..95M

Demory, B. -O.; Morris, B. M.; Schanche, N. +2 more

Context. 55 Cnc e is in a 0.73 day orbit transiting a Sun-like star. It has been observed that the occultation depth of this super-Earth, with a mass of 8 M and radius of 2 R, changes significantly over time at mid-infrared wavelengths. Observations with Spitzer measured a change in its day-side brightness temperature of 12…

2022 Astronomy and Astrophysics
Gaia 18
Updated Photometry of the Yellow Supergiant Progenitor and Late-time Observations of the Type IIb Supernova SN 2016gkg
DOI: 10.3847/1538-4357/ac8a4c Bibcode: 2022ApJ...936..111K

Kilpatrick, Charles D.; Coulter, David A.; Foley, Ryan J. +4 more

We present Hubble Space Telescope (HST) observations of the Type IIb supernova (SN) SN 2016gkg at 652, 1698, and 1795 days from explosion with the Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Comparing to pre-explosion imaging from 2001 obtained with the Wide Field Planetary Camera 2, we demonstrate that SN 2016gkg is now fain…

2022 The Astrophysical Journal
eHST 18
Probing the Galactic halo with RR lyrae stars - III. The chemical and kinematic properties of the stellar halo
DOI: 10.1093/mnras/stac2666 Bibcode: 2022MNRAS.517.2787L

Tian, Haijun; Liu, Gaochao; Huang, Yang +3 more

Based on a large spectroscopic sample of ~4300 RR Lyrae stars with metallicity, systemic radial velocity, and distance measurements, we present a detailed analysis of the chemical and kinematic properties of the Galactic halo. Using this sample, the metallicity distribution function (MDF) as a function of r and the velocity anisotropy parameter β …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18
The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18
DOI: 10.1093/mnras/stab2669 Bibcode: 2022MNRAS.509.1075C

Bonavera, L.; González-Nuevo, J.; Korth, J. +28 more

We present the first results of K2-OjOS, a collaborative project between professional and amateur astronomers primarily aimed to detect, characterize, and validate new extrasolar planets. For this work, 10 amateur astronomers looked for planetary signals by visually inspecting the 20 427 light curves of K2 campaign 18 (C18). They found 42 planet c…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18
Solar Energetic Particles Produced during Two Fast Coronal Mass Ejections
DOI: 10.3847/2041-8213/ac5b72 Bibcode: 2022ApJ...928L...6L

Wang, Yuming; Guo, Jingnan; Li, Xiaolei +1 more

Two recent extremely fast coronal mass ejections (CMEs) are of particular interest. The first one originated from the southern hemisphere on 2021 October 28 and caused strong solar energetic particle (SEP) events over a wide longitude range from Earth, STEREO-A, to Mars. However, the other one, originating from the center of the Earth-viewed solar…

2022 The Astrophysical Journal
SOHO 18
Data Fusion of Total Solar Irradiance Composite Time Series Using 41 Years of Satellite Measurements
DOI: 10.1029/2021JD036146 Bibcode: 2022JGRD..12736146M

Schmutz, W.; Haberreiter, M.; Dudok de Wit, T. +4 more

Since the late 1970s, successive satellite missions have been monitoring the sun's activity and recording the total solar irradiance (TSI). Some of these measurements have lasted for more than a decade. In order to obtain a seamless record whose duration exceeds that of the individual instruments, the time series have to be merged. Climate models …

2022 Journal of Geophysical Research (Atmospheres)
SOHO 18