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JWST COMPASS: The 3–5 µm Transmission Spectrum of the Super-Earth L 98-59 c
DOI: 10.3847/1538-3881/ad73cf Bibcode: 2024AJ....168..276S

Batalha, Natalie M.; Moran, Sarah E.; Kirk, James +14 more

We present a JWST Near-InfraRed Spectrograph (NIRSpec) transmission spectrum of the super-Earth exoplanet L 98-59 c. This small (R p = 1.385 ± 0.085R , M p = 2.22 ± 0.26 R ), warm (T eq = 553 K) planet resides in a multiplanet system around a nearby, bright (J = 7.933) M3V star. We find …

2024 The Astronomical Journal
JWST 7
Determining stellar accretion rates from Paα and Brβ emission lines with JWST NIRSpec. Accretion of pre-main-sequence stars in NGC 3603
DOI: 10.1051/0004-6361/202449282 Bibcode: 2024A&A...684L...8R

de Marchi, Guido; Brandl, Bernhard; Rogers, Ciarán

In this Letter, we present the first systematic spectroscopic measurements of the near-infrared (NIR) hydrogen recombination lines Paschen alpha (Paαλ = 1.875 µm) and Brackett beta (Brβλ = 2.626 µm), produced by pre-main-sequence (PMS) stars. Such stars include T Tauri and Herbig AeBe stars, located in the massive…

2024 Astronomy and Astrophysics
JWST 7
Clues to growth and disruption of two neighbouring spiral arms of the Milky Way
DOI: 10.1093/mnras/stae2041 Bibcode: 2024MNRAS.533.4324F

Matsunaga, Noriyuki; Kawata, Daisuke; Taniguchi, Daisuke +3 more

Studying the nature of spiral arms is essential for understanding the formation of the intricate disc structure of the Milky Way. The European Space Agency's Gaia mission has provided revolutionary observational data that have uncovered detailed kinematical features of stars in the Milky Way. However, so far the nature of spiral arms continues to …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
DOI: 10.3847/1538-4357/ad234a Bibcode: 2024ApJ...964...94C

Cleri, Nikko J.; Giavalisco, Mauro; Ji, Zhiyuan +3 more

We explore the relationships between the [O/H] gas-phase metallicity radial gradients and multiple galaxy properties for 238 star-forming galaxies at 0.6 < z < 2.6 selected from the CANDELS Lyα Emission at Reionization survey with stellar mass $8.5\lt \mathrm{log}\,{M}_{* }/{M}_{\odot }\lt 10.5$ . The gradients cover the range from ‑0.11 to …

2024 The Astrophysical Journal
eHST 7
CHEX-MATE: A LOFAR pilot X-ray - radio study on five radio halo clusters
DOI: 10.1051/0004-6361/202347965 Bibcode: 2024A&A...686A...5B

Brunetti, G.; Pointecouteau, E.; Pratt, G. W. +24 more

The connection between the thermal and non-thermal properties in galaxy clusters hosting radio halos seems fairly well established. However, a comprehensive analysis of such a connection has only been done for integrated quantities (e.g. LX − Pradio relation). In recent years, new-generation radio telescopes have enabled the …

2024 Astronomy and Astrophysics
XMM-Newton 7
VaTEST III: Validation of eight potential super-earths from TESS data
DOI: 10.1017/pasa.2024.29 Bibcode: 2024PASA...41...30M

Barclay, Thomas; Tan, Thiam-Guan; Schlieder, Joshua E. +39 more

NASA's all-sky survey mission, the Transiting Exoplanet Survey Satellite (TESS), is specifically engineered to detect exoplanets that transit bright stars. Thus far, TESS has successfully identified approximately 400 transiting exoplanets, in addition to roughly 6 000 candidate exoplanets pending confirmation. In this study, we present the results…

2024 Publications of the Astronomical Society of Australia
Gaia JWST 7
The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release
DOI: 10.3847/1538-4357/ad3c44 Bibcode: 2024ApJ...967..123T

Connor, Thomas; Gonzalez, Anthony H.; Stanford, S. A. +7 more

The Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2) is a new survey designed as the successor of the original MaDCoWS survey. MaDCoWS2 improves upon its predecessor by using deeper optical and infrared data and a more powerful detection algorithm (PZWav). As input to the search, we use grz photometry from the DECam Legacy Survey (DECaLS) …

2024 The Astrophysical Journal
Gaia 7
Localizing Quasiperiodic Pulsations in Hard X-Ray, Microwave, and Lyα Emissions of an X6.4 Flare
DOI: 10.3847/1538-4357/ad566c Bibcode: 2024ApJ...970...77L

Su, Yang; Li, Dong; Hong, Zhenxiang +1 more

We report the simultaneous observations of quasiperiodic pulsations (QPPs) in wavelengths of hard X-ray (HXR), microwave, Lyα, and ultraviolet (UV) emissions during the impulsive phase of an X6.4 flare on 2024 February 22 (SOL2024-02-22T22:08). The X6.4 flare shows three repetitive and successive pulsations in HXR and microwave wavebands, and they…

2024 The Astrophysical Journal
SolarOrbiter 7
Imprints of the Local Bubble and Dust Complexity on Polarized Dust Emission
DOI: 10.3847/1538-4357/ad61e0 Bibcode: 2024ApJ...973...54H

Tahani, Mehrnoosh; Clark, S. E.; Halal, George

Using 3D dust maps and Planck polarized dust emission data, we investigate the influence of the 3D geometry of the nearby interstellar medium (ISM) on the statistics of the dust polarization on large ( 80' ) scales. We test rece…

2024 The Astrophysical Journal
Gaia 7
Measuring Tracers of Planet Formation in the Atmosphere of WASP-77A b: Substellar O/H and C/H Ratios, with a Stellar C/O Ratio and a Potentially Superstellar Ti/H Ratio
DOI: 10.3847/2041-8213/ad2000 Bibcode: 2024ApJ...962L..30E

Changeat, Quentin; Edwards, Billy

We present a comprehensive atmospheric retrieval study of the hot Jupiter WASP-77A b using eclipse observations from the Hubble Space Telescope (HST) and JWST. Using atmospheric retrievals, the spectral features of H2O, CO, and TiO are identified, with volume mixing ratios estimated at log10(VMR) = ‑4.40 ${}_{-0.11}^{+0.14}$ …

2024 The Astrophysical Journal
eHST JWST 7