Search Publications

An Extremely Massive White Dwarf Escaped from the Hyades Star Cluster
DOI: 10.3847/2041-8213/acffc4 Bibcode: 2023ApJ...956L..41M

El-Badry, Kareem; Rodriguez, Antonio C.; van Roestel, Jan +5 more

We searched the Gaia DR3 database for ultramassive white dwarfs with kinematics consistent with having escaped the nearby Hyades open cluster, identifying three such candidates. Two of these candidates have masses estimated from Gaia photometry of approximately 1.1 solar masses; their status as products of single-stellar evolution that have escape…

2023 The Astrophysical Journal
Gaia 5
The Differential Assembly History of the Centers and Outskirts of Main-sequence Galaxies at z 2.3
DOI: 10.3847/1538-4357/acb5e9 Bibcode: 2023ApJ...945...97C

Giavalisco, Mauro; Ji, Zhiyuan; Cutler, Sam E. +1 more

We present a study of spatially resolved star formation histories (SFHs) for 60 z ~ 2.3 main-sequence, star-forming galaxies selected from the MOSDEF spectroscopic survey in the GOODS-N field, with median stellar mass $\mathrm{log}({M}_{\star }/{M}_{\odot })$ = 9.75 and spanning the range $8.6\lt \mathrm{log}({M}_{\star }/{M}_{\odot })\lt 11.5$ . …

2023 The Astrophysical Journal
eHST 5
Fast Reconstruction of 3D Density Distribution around the Sun Based on the MAS by Deep Learning
DOI: 10.3847/1538-4357/acbd3c Bibcode: 2023ApJ...948...21R

Moon, Yong-Jae; Rahman, Sumiaya; Park, Eunsu +5 more

This study is the first attempt to generate a three-dimensional (3D) coronal electron density distribution based on the pix2pixHD model, whose computing time is much shorter than that of the magnetohydrodynamic (MHD) simulation. For this, we consider photospheric solar magnetic fields as input, and electron density distribution simulated with the …

2023 The Astrophysical Journal
SOHO 5
Electrostatic Solitary Waves in the Venusian Ionosphere Pervaded by the Solar Wind: A Theoretical Perspective
DOI: 10.3847/1538-4357/acd2d7 Bibcode: 2023ApJ...950..111R

Lakhina, G. S.; Kamalam, T.; Singh, S. V. +3 more

Electrostatic solitary waves (ESWs) in the Venusian ionosphere that are impinged by the solar wind are investigated using a homogeneous, collisionless, and magnetized multicomponent plasma consisting of Venusian H+ and O+ ions, Maxwellian Venusian electrons and streaming solar wind protons, and suprathermal electrons followin…

2023 The Astrophysical Journal
SolarOrbiter 5
Halfway to the Peak: Spatially Resolved Star Formation and Kinematics in a z = 0.54 Dusty Galaxy with JWST/MIRI
DOI: 10.3847/2041-8213/ad07e1 Bibcode: 2023ApJ...958L...5Y

Veilleux, Sylvain; Ogle, Patrick; Alberts, Stacey +16 more

We present JWST Mid-InfraRed Instrument/Medium-Resolution Spectrometer (MIRI/MRS) observations of an infrared luminous disk galaxy, FLS1, at z ~ 0.54. With a lookback time of 5 Gyr, FLS1 is chronologically at the midpoint between the peak epoch of star formation and the present day. The MRS data provide maps of the atomic fine structure lines [Ar …

2023 The Astrophysical Journal
ISO eHST JWST 5
Separated Twins or Just Siblings? A Multiplanet System around an M Dwarf Including a Cool Sub-Neptune
DOI: 10.3847/2041-8213/ad037d Bibcode: 2023ApJ...959L...1H

Quinn, Samuel N.; Stassun, Keivan G.; Zhou, George +27 more

We report the discovery of two TESS sub-Neptunes orbiting the early M dwarf TOI-904 (TIC 261257684). Both exoplanets, TOI-904 b and c, were initially observed in TESS Sector 12 with twin sizes of ${2.426}_{-0.157}^{+0.163}$ and ${2.167}_{-0.118}^{+0.130}$ R , respectively. Through observations in five additional sectors in the TESS pri…

2023 The Astrophysical Journal
Gaia 5
Cosmic-CoNN: A Cosmic-Ray Detection Deep-learning Framework, Data Set, and Toolkit
DOI: 10.3847/1538-4357/ac9d91 Bibcode: 2023ApJ...942...73X

Howell, D. Andrew; McCully, Curtis; Xu, Chengyuan +2 more

Rejecting cosmic rays (CRs) is essential for the scientific interpretation of CCD-captured data, but detecting CRs in single-exposure images has remained challenging. Conventional CR detectors require experimental parameter tuning for different instruments, and recent deep-learning methods only produce instrument-specific models that suffer from p…

2023 The Astrophysical Journal
eHST 5
Stellar-reddening-based Extinction Maps for Cosmological Applications
DOI: 10.3847/1538-4357/acc32c Bibcode: 2023ApJ...949...47M

Finkbeiner, Douglas P.; Mudur, Nayantara; Park, Core Francisco

Cosmological surveys must correct their observations for the reddening of extragalactic objects by Galactic dust. Existing dust maps, however, have been found to have spatial correlations with the large-scale structure of the Universe. Errors in extinction maps can propagate systematic biases into samples of dereddened extragalactic objects and in…

2023 The Astrophysical Journal
Gaia 5
The Large Deficit of HMXB Emission from Luminous Infrared Galaxies: The Case of the Circumnuclear Starburst Ring in NGC 7552
DOI: 10.3847/1538-4357/acd9aa Bibcode: 2023ApJ...952...22W

Zezas, Andreas; Roberts, Timothy P.; West, Lacey +5 more

Luminous infrared galaxies (LIRGs), the most extreme star-forming galaxies in the nearby (D < 30 Mpc) universe, show a notable X-ray emission deficiency (up to a factor of ~10) compared with predictions from scaling relations of galaxy-wide high-mass X-ray binary (HMXB) luminosity with star formation rate. In the nearby (≈20 Mpc) LIRG NGC 7552,…

2023 The Astrophysical Journal
eHST 5
Intriguing Plasma Composition Pattern in a Solar Active Region: A Result of Nonresonant Alfvén Waves?
DOI: 10.3847/1538-4357/ad05bf Bibcode: 2023ApJ...959...72M

Stangalini, Marco; Long, David M.; Brooks, David H. +6 more

The plasma composition of the solar corona is different from that of the solar photosphere. Elements that have a low first ionization potential (FIP) are preferentially transported to the corona and therefore show enhanced abundances in the corona compared to the photosphere. The level of enhancement is measured using the FIP bias parameter. In th…

2023 The Astrophysical Journal
Hinode 5