Search Publications

GECAM Localization of High-energy Transients and the Systematic Error
DOI: 10.3847/1538-4365/acafeb Bibcode: 2023ApJS..265...17Z

Gao, Min; Gong, Ke; Qiao, Rui +63 more

The Gravitational Wave High-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a pair of microsatellites (i.e., GECAM-A and GECAM-B) dedicated to monitoring gamma-ray transients including the high-energy electromagnetic counterparts of gravitational waves, such as gamma-ray bursts, soft gamma-ray repeaters, solar flares, and terrestrial…

2023 The Astrophysical Journal Supplement Series
INTEGRAL 10
Chemistry of multiple stellar populations in the mono-metallic, in situ, bulge globular cluster NGC 6388
DOI: 10.1051/0004-6361/202346174 Bibcode: 2023A&A...677A..73C

Bragaglia, Angela; Carretta, Eugenio

We present the homogeneous abundance analysis for a combined sample of 185 giants in the bulge globular cluster (GC) NGC 6388. Our results are used to describe the multiple stellar populations and differences or analogies with bulge field stars. Proton-capture elements indicate that a single class of first-generation polluters is sufficient to rep…

2023 Astronomy and Astrophysics
eHST 10
No Surviving SN Ia Companion in SNR 0509-67.5: Stellar Population Characterization and Comparison to Models
DOI: 10.3847/2041-8213/acd6a0 Bibcode: 2023ApJ...950L..10S

Hughes, John P.; Shields, Joshua V.; Kerzendorf, Wolfgang +4 more

The community agrees that Type Ia supernovae arise from carbon/oxygen white dwarfs undergoing thermonuclear runaway. However, the full progenitor system and the process that prompts the white dwarf to explode remain unknown. Most current models suggest that the white dwarf explodes because of interaction with a binary companion that may survive th…

2023 The Astrophysical Journal
eHST 10
An X-Ray Census of Fast Radio Burst Host Galaxies: Constraints on Active Galactic Nuclei and X-Ray Counterparts
DOI: 10.3847/1538-4357/acf843 Bibcode: 2023ApJ...958...66E

Tejos, N.; Dong, Y.; Fong, W. +16 more

We present the first X-ray census of fast radio burst (FRB) host galaxies to conduct the deepest search for active galactic nuclei (AGN) and X-ray counterparts to date. Our sample includes seven well-localized FRBs with unambiguous host associations and existing deep Chandra observations, including two events for which we present new observations.…

2023 The Astrophysical Journal
eHST 10
Multiple flares in the changing-look AGN NGC 5273
DOI: 10.1093/mnras/stad725 Bibcode: 2023MNRAS.521.3810N

Kochanek, C. S.; Huber, M. E.; Stanek, K. Z. +15 more

NGC 5273 is a known optical and X-ray variable AGN. We analyse new and archival IR, optical, UV, and X-ray data in order to characterize its long-term variability from 2000-2022. At least one optical changing-look event occurred between 2011 and 2014 when the AGN changed from a Type 1.8/1.9 Seyfert to a Type 1. It then faded considerably at all wa…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 10
A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
DOI: 10.1051/0004-6361/202346055 Bibcode: 2023A&A...674A..56R

Pauli, D.; Rickard, M. J.

Context. Most massive stars are believed to be born in close binary systems where they can exchange mass, which impacts the evolution of both binary components. Their evolution is of great interest in the search for the progenitors of gravitational waves. However, there are unknowns in the physics of mass transfer as observational examples are rar…

2023 Astronomy and Astrophysics
Gaia eHST 9
Vortex fiber nulling for exoplanet observations: implementation and first light
DOI: 10.1117/1.JATIS.9.3.035002 Bibcode: 2023JATIS...9c5002E

Fitzgerald, Michael P.; Ren, Bin B.; Jovanovic, Nemanja +31 more

Vortex fiber nulling (VFN) is a single-aperture interferometric technique for detecting and characterizing exoplanets separated from their host star by less than a diffracted beam width. VFN uses a vortex mask and single-mode fiber to selectively reject starlight while coupling off-axis planet light with a simple optical design that can be readily…

2023 Journal of Astronomical Telescopes, Instruments, and Systems
Gaia 9
Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-infrared Spectroscopy
DOI: 10.3847/1538-3881/accc25 Bibcode: 2023AJ....166....5O

Zuckerman, B.; Manjavacas, Elena; Dufour, Patrick +7 more

Excess infrared flux from white dwarf stars is likely to arise from a dusty debris disk or a cool companion. In this work, we present near-infrared spectroscopic observations with Keck/MOSFIRE, Gemini/GNIRS, and Gemini/Flamingos-2 of seven white dwarfs with infrared excesses identified in previous studies. We confirmed the presence of dust disks a…

2023 The Astronomical Journal
Gaia 9
Revisiting the Transit Timing and Atmosphere Characterization of the Neptune-mass Planet HAT-P-26 b
DOI: 10.3847/1538-3881/acfeea Bibcode: 2023AJ....166..223A

McDonald, Iain; Dhillon, Vik S.; A-thano, Napaporn +11 more

We present a transit-timing variation (TTV) and planetary atmosphere analysis of the Neptune-mass planet HAT-P-26 b. We present a new set of 13 transit light curves from optical ground-based observations and combine them with light curves from the Wide Field Camera 3 on the Hubble Space Telescope, the Transiting Exoplanet Survey Satellite, and pre…

2023 The Astronomical Journal
Gaia eHST 9
Weighing the Darkness. II. Astrometric Measurement of Partial Orbits with Gaia
DOI: 10.3847/1538-4357/acbb5f Bibcode: 2023ApJ...946..111A

Breivik, Katelyn; Andrews, Jeff J.; Chawla, Chirag +2 more

Over the course of several years, stars trace helical trajectories as they traverse across the sky due to the combined effects of proper motion and parallax. It is well known that the gravitational pull of an unseen companion can cause deviations to these tracks. Several studies have pointed out that the astrometric mission Gaia will be able to id…

2023 The Astrophysical Journal
Gaia 9