Search Publications

SKYSURF-3: Testing Crowded Object Catalogs in the Hubble eXtreme Deep Field Mosaics to Study Sample Incompleteness from an Extragalactic Background Light Perspective
DOI: 10.3847/2041-8213/ac9cca Bibcode: 2022ApJ...940L..15K

Pirzkal, Nor; Windhorst, Rogier A.; Koekemoer, Anton +6 more

Extragalactic background light (EBL) studies have revealed a significant discrepancy between direct measurements-via instruments measuring "bare" sky from which Zodiacal and Galactic light models are subtracted-and measurements of the integrated galaxy light (IGL). This discrepancy could lie in either method, whether it be an incomplete Zodiacal m…

2022 The Astrophysical Journal
eHST 9
A Star-sized Impact-produced Dust Clump in the Terrestrial Zone of the HD 166191 System
DOI: 10.3847/1538-4357/ac4bbb Bibcode: 2022ApJ...927..135S

Rieke, G. H.; Kennedy, Grant M.; Su, Kate Y. L. +2 more

We report on five years of 3-5 µm photometry measurements obtained by warm Spitzer to track the dust debris emission in the terrestrial zone of HD 166191 in combination with simultaneous optical data. We show that the debris production in this young (~10 Myr) system increased significantly in early 2018 and reached a record high level (almos…

2022 The Astrophysical Journal
Gaia 9
Radio Observations of Four Active Galactic Nuclei Hosting Intermediate-mass Black Hole Candidates: Studying the Outflow Activity and Evolution
DOI: 10.3847/1538-4357/ac9e9d Bibcode: 2022ApJ...941...43Y

Ho, Luis C.; Zhang, Shaohua; Yang, Jun +5 more

Observational searches for intermediate-mass black holes (IMBHs; 102-106 M ) include relatively isolated dwarf galaxies. For those that host active galactic nuclei (AGNs), the IMBH nature may be discerned through the accretion-jet activity. We present radio observations of four AGN-hosting dwarf galaxies, which po…

2022 The Astrophysical Journal
Gaia 9
Far-ultraviolet Flares on Accreting Protostars: Weak and Classical T Tauri Stellar Pair Analysis
DOI: 10.3847/1538-4357/ac8f26 Bibcode: 2022ApJ...939...82H

Kowalski, Adam F.; France, Kevin; Hinton, P. C. +5 more

The far-ultraviolet (FUV) emission of classical T Tauri stars (CTTSs) is known to play an important role in protoplanetary disk dispersal and giant planet formation, yet the role played by protostellar flares in these processes is largely unknown. We use nearby star-forming regions as laboratories to probe the FUV flare characteristics of CTTSs an…

2022 The Astrophysical Journal
eHST 9
First Report of a Solar Energetic Particle Event Observed by China's Tianwen-1 Mission in Transit to Mars
DOI: 10.3847/2041-8213/ac80f5 Bibcode: 2022ApJ...934L..15F

Zhao, Lingling; Sun, Zhiyu; Yu, Yuhong +15 more

Solar energetic particles (SEPs) associated with flares and/or coronal mass ejection (CME)-driven shocks can impose acute radiation hazards on space explorations. To measure energetic particles in near-Mars space, the Mars Energetic Particle Analyzer (MEPA) instrument on board China's Tianwen-1 (TW-1) mission was designed. Here, we report the firs…

2022 The Astrophysical Journal
SOHO 9
Relationship between Total Solar Irradiance and Magnetic Flux during Solar Minima
DOI: 10.3847/1538-4357/ac8a98 Bibcode: 2022ApJ...936..158M

Lean, Judith L.; Marchenko, Sergey V.; DeLand, Matthew T.

What drives the small total solar irradiance (TSI) changes of ~50-100 parts per million (compared with >1000 ppm solar-cycle amplitudes) during a deep solar minimum, i.e., in the practical absence of detectable sunspots and long-lasting active regions? We consider the epoch 2008 June-October and investigate multiple data sets (TSI; various Mg I…

2022 The Astrophysical Journal
SOHO 9
A Very Long Baseline Array Trigonometric Parallax for RR Aql and the Mira Period-Luminosity Relation
DOI: 10.3847/1538-4357/ac69e0 Bibcode: 2022ApJ...931...74S

Sun, Yan; Reid, Mark J.; Zhang, Bo +4 more

We report Very Long Baseline Array observations of 22 GHz H2O and 43 GHz SiO masers toward the Mira variable RR Aql. By fitting the SiO maser emission to a circular ring, we estimate the absolute stellar position of RR Aql and find agreement with Gaia astrometry to within the joint uncertainty of ≈1 mas. Using the maser astrometry we me…

2022 The Astrophysical Journal
Gaia 9
On the Evolution of Rotational Modulation Amplitude in Solar-mass Main-sequence Stars
DOI: 10.3847/1538-4357/ac7527 Bibcode: 2022ApJ...933..195M

Masuda, Kento

We investigate the relation between rotation periods P rot and photometric modulation amplitudes R per for ≈4000 Sun-like main-sequence stars observed by Kepler, using P rot and R per from McQuillan et al., effective temperature T eff from LAMOST DR6, and parallax data from Gaia EDR3. As has b…

2022 The Astrophysical Journal
Gaia 9
Radio Emission from Binary Ultracool Dwarf Systems
DOI: 10.3847/1538-4357/ac660b Bibcode: 2022ApJ...932...21K

Kao, Melodie M.; Pineda, J. Sebastian

Well-characterized binary systems will provide valuable opportunities to study the conditions that are necessary for the onset of both auroral and nonauroral magnetospheric radio emission in the ultracool dwarf regime. We present new detections of nonauroral "quiescent" radio emission at 4-8 GHz of the three ultracool dwarf binary systems GJ 564 B…

2022 The Astrophysical Journal
Gaia 9
Discovery of Nine Super Li-rich Unevolved Stars from the LAMOST Survey
DOI: 10.3847/2041-8213/ac63a5 Bibcode: 2022ApJ...929L..14Y

Wang, L.; Shi, J. -R.; Zhou, Y. -T. +7 more

Based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution spectroscopic survey (MRS), we report the discovery of nine super Li-rich unevolved stars with A(Li) > 3.8 dex. These objects show unusually high levels of lithium abundances, up to three times higher than the meteoritic value of 3.3 dex, which ind…

2022 The Astrophysical Journal
Gaia 9