Search Publications

TOI-1994b: A Low-mass Eccentric Brown Dwarf Transiting A Subgiant Star
DOI: 10.3847/1538-3881/ad1a18 Bibcode: 2024AJ....167..109P

Barclay, Thomas; Quinn, Samuel N.; Kane, Stephen R. +23 more

We present the discovery of TOI-1994b, a low-mass brown dwarf transiting a hot subgiant star on a moderately eccentric orbit. TOI-1994 has an effective temperature of ${7700}_{-410}^{+720}$ K, V magnitude of 10.51 mag and log(g) of ${3.982}_{-0.065}^{+0.067}$ . The brown dwarf has a mass of ${22.1}_{-2.5}^{+2.6}$ M J, a period of 4.034 …

2024 The Astronomical Journal
Gaia 5
A Strongly Lensed Dusty Starburst of an Intrinsic Disk Morphology at a Photometric Redshift of z ph > 7
DOI: 10.3847/2041-8213/ad59a3 Bibcode: 2024ApJ...969L..28L

Yan, Haojing; Cheng, Cheng; Ling, Chenxiaoji +3 more

We present COSBO-7, a strong millimeter source known for more than 16 yr that just revealed its near-to-mid-IR counterpart with the James Webb Space Telescope (JWST). The precise pinpointing by the Atacama Large Millimeter/submillimeter Array on the exquisite NIRCam and MIRI images show that it is a background source gravitationally lensed by a si…

2024 The Astrophysical Journal
JWST 5
The Near-infrared Ca II Triplet as a Stellar Activity Indicator: A Library and Comparative Study
DOI: 10.3847/1538-4365/ad33bc Bibcode: 2024ApJS..272....6H

Zhang, Yong; Huang, Xin; Zhang, Haotong +11 more

We have established and released a new stellar index library of the Ca II triplet, which serves as an indicator for characterizing the chromospheric activity of stars. The library is based on data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Low-Resolution Spectroscopic Survey (LRS) Data Release 9. To better reflect …

2024 The Astrophysical Journal Supplement Series
Gaia 5
Signatures of gas flows - I. Connecting the kinematics of the H I circumgalactic medium to galaxy rotation
DOI: 10.1093/mnras/stae1843 Bibcode: 2024MNRAS.533.1321N

Charlton, Jane C.; Kacprzak, Glenn G.; Churchill, Christopher W. +5 more

The circumgalactic medium (CGM) hosts many physical processes with different kinematic signatures that affect galaxy evolution. We address the CGM-galaxy kinematic connection by quantifying the fraction of H I that is aligned with galaxy rotation with the equivalent width co-rotation fraction, $f_{\rm EWcorot}$. Using 70 quasar sightlines having H…

2024 Monthly Notices of the Royal Astronomical Society
eHST 5
Constraints on Neutron Star Structure from the Clocked X-Ray Burster 1RXS J180408.9-342058
DOI: 10.3847/1538-4357/ad0a67 Bibcode: 2024ApJ...960...14D

Nagataki, S.; Hashimoto, M.; Dohi, A. +3 more

Type I X-ray bursts are rapid-brightening transient phenomena on the surfaces of accreting neutron stars (NSs). Some X-ray bursts, called clocked bursters, exhibit regular behavior with similar light-curve profiles in their burst sequences. The periodic nature of clocked bursters has the advantage of constraining X-ray binary parameters and physic…

2024 The Astrophysical Journal
INTEGRAL 5
An overlooked source of uncertainty in the mass of the Milky Way
DOI: 10.1093/mnrasl/slae042 Bibcode: 2024MNRAS.532L..48O

Riley, Alexander H.; Oman, Kyle A.

In the conventional approach to decomposing a rotation curve into a set of contributions from mass model components, the measurements of the rotation curve at different radii are taken to be independent. It is clear, however, that radial correlations are present in such data, for instance (but not only) because the orbital speed depends on the mas…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 5
Spectroscopic Observations of the Solar Corona during the 2017 August 21 Total Solar Eclipse: Comparison of Spectral Line Widths and Doppler Shifts between Open and Closed Magnetic Structures
DOI: 10.3847/1538-4357/ad3424 Bibcode: 2024ApJ...966..122Z

Landi, Enrico; Habbal, Shadia R.; Ding, Adalbert +5 more

The spectroscopic observations presented here were acquired during the 2017 August 21 total solar eclipse (TSE) with a three-channel partially multiplexed imaging spectrometer operating at extremely high orders (>50). The 4 R extent of the slit in the north–south direction scanned the corona starting from the central meridian out t…

2024 The Astrophysical Journal
Hinode 5
Identification of Carbon Stars from LAMOST DR7
DOI: 10.3847/1538-4365/ad1881 Bibcode: 2024ApJS..271...12L

Shi, Jianrong; Cui, Wenyuan; Li, Linlin +6 more

Carbon stars are excellent kinematic tracers of galaxies and play important roles in understanding the evolution of the Galaxy. Therefore, it is worthwhile to search for them in a large number of spectra. In this work, we build a new carbon star catalog based on the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) DR7 spectra. The…

2024 The Astrophysical Journal Supplement Series
Gaia 5
The Galaxy–Galaxy Strong Lensing Cross Section and the Internal Distribution of Matter in ΛCDM Substructure
DOI: 10.3847/1538-4357/ad51fd Bibcode: 2024ApJ...970..143T

Mahler, Guillaume; Meneghetti, Massimo; Jauzac, Mathilde +3 more

Strong gravitational lensing offers a powerful probe of the detailed distribution of matter in lenses, while magnifying and bringing faint background sources into view. Observed strong lensing by massive galaxy clusters, which are often in complex dynamical states, has also been used to map their dark matter (DM) substructures on smaller scales. D…

2024 The Astrophysical Journal
eHST 5
Realistic Uncertainties for Fundamental Properties of Asteroseismic Red Giants and the Interplay between Mixing Length, Metallicity, and νmax
DOI: 10.3847/1538-4357/ad6c3e Bibcode: 2024ApJ...974...77L

Li, Yaguang; van Saders, Jennifer; Huber, Daniel +8 more

Asteroseismic modeling is a powerful way to derive stellar properties. However, the derived quantities are limited by built-in assumptions used in stellar models. This work presents a detailed characterization of stellar model uncertainties in asteroseismic red giants, focusing on the mixing-length parameter α MLT, the initial helium fr…

2024 The Astrophysical Journal
Gaia 5