Search Publications

WEAVE-StePS: A stellar population survey using WEAVE at WHT
DOI: 10.1051/0004-6361/202245361 Bibcode: 2023A&A...672A..87I

Bolzonella, M.; Gullieuszik, M.; Moretti, A. +45 more

Context. The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide valuable opportunities for forthcoming galaxy surveys through their huge multiplexing capabilities, excellent spectral resolution, and unprecedented wavelength coverage.
Aims: WEAVE is a new wide-field spectroscopic facility mounted on th…

2023 Astronomy and Astrophysics
Gaia 9
Observational Signatures of Electron-driven Chromospheric Evaporation in a White-light Flare
DOI: 10.3847/1538-4357/ace256 Bibcode: 2023ApJ...954....7L

Warmuth, Alexander; Li, Dong; Ning, Zongjun +7 more

We investigate observational signatures of explosive chromospheric evaporation during a white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis, bisector techniques, and the Gaussian fitting method, redshifted velocities of less than 20 km s‑1 are detected in low-temperature spectral lines of Hα, C I, and Si I…

2023 The Astrophysical Journal
IRIS SolarOrbiter 9
3D tomography of the giant Lyα nebulae of z ≈ 3-5 radio-loud AGN
DOI: 10.1051/0004-6361/202346415 Bibcode: 2023A&A...680A..70W

Noirot, Gaël; Lehnert, Matthew D.; De Breuck, Carlos +12 more

Lyα emission nebulae are ubiquitous around high-redshift galaxies and are tracers of the gaseous environment on scales out to ≳100 pkpc (proper kiloparsec). High-redshift radio galaxies (HzRGs, type-2 radio-loud quasars) host large-scale nebulae observed in the ionised gas differ from those seen in other types of high-redshift quasars. In this wor…

2023 Astronomy and Astrophysics
Gaia eHST 9
A catalogue of unusually long thermonuclear bursts on neutron stars
DOI: 10.1093/mnras/stad374 Bibcode: 2023MNRAS.521.3608A

Degenaar, N.; in't Zand, J. J. M.; Kuulkers, E. +10 more

Rare, energetic (long) thermonuclear (Type I) X-ray bursts are classified either as intermediate-duration or 'supern' bursts, based on their duration. Intermediate-duration bursts lasting a few to tens of minutes are thought to arise from the thermonuclear runaway of a relatively thick (≈1010 g cm-2) helium layer, while super…

2023 Monthly Notices of the Royal Astronomical Society
Exosat INTEGRAL 9
Chromospheric thermodynamic conditions from inversions of complex Mg II h & k profiles observed in flares
DOI: 10.3389/fspas.2023.1133429 Bibcode: 2023FrASS..1033429S

De Pontieu, Bart; Sainz Dalda, Alberto

The flare activity of the Sun has been studied for decades, using both space- and ground-based telescopes. The former have mainly focused on the corona, while the latter have mostly been used to investigate the conditions in the chromosphere and photosphere. The Interface Region Imaging Spectrograph (IRIS) instrument has served as a gateway betwee…

2023 Frontiers in Astronomy and Space Sciences
IRIS 9
Colour jumps across the spiral arms of Hubble Ultra Deep Field galaxies
DOI: 10.1093/mnras/stad1805 Bibcode: 2023MNRAS.524...18M

González-Lópezlira, Rosa A.; Martínez-García, Eric E.; Puerari, Ivânio

We have measured, at various wavelengths, the spiral arm pitch angles of a sample of distant spiral galaxies from the Hubble Space Telescope eXtreme Deep Field (XDF). According to density wave (DW) theory, we should detect colour jumps from red-to-blue across the spiral arms. Colour jumps are a consequence of large-scale shocks, which also generat…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
Dust-buried Compact Sources in the Dwarf Galaxy NGC 4449
DOI: 10.3847/1538-4357/acbeac Bibcode: 2023ApJ...946....1C

Ji, Zhiyuan; Smith, Linda J.; Calzetti, Daniela +10 more

Multiwavelength images from the Hubble Space Telescope covering the wavelength range 0.27-1.6 µm show that the central area of the nearby dwarf galaxy NGC 4449 contains several tens of compact sources that are emitting in the hydrogen recombination line Paβ (1.2818 µm) but are only marginally detected in Hα (0.6563 µm) and undete…

2023 The Astrophysical Journal
eHST 9
Probing the physics in the core boundary layers of the double-lined B-type binary KIC 4930889 from its gravito-inertial modes
DOI: 10.1051/0004-6361/202244192 Bibcode: 2023A&A...679A...6M

Aerts, C.; Tkachenko, A.; Van Reeth, T. +1 more

Context. Stellar evolution models of B-type stars are still uncertain in terms of internal mixing properties, notably in the area between the convective core and the radiative envelope. This impacts age determination of such stars in addition to the computation of chemical yields produced at the end of their life.
Aims: We investigated the th…

2023 Astronomy and Astrophysics
Gaia 9
KURVS: the outer rotation curve shapes and dark matter fractions of z 1.5 star-forming galaxies
DOI: 10.1093/mnras/stad1966 Bibcode: 2023MNRAS.524.2814P

Glazebrook, Karl; Obreschkow, Danail; Gillman, Steven +14 more

We present first results from the KMOS Ultra-deep Rotation Velocity Survey (KURVS), aimed at studying the outer rotation curves shape and dark matter content of 22 star-forming galaxies at z ~ 1.5. These galaxies represent 'typical' star-forming discs at z ~ 1.5, being located within the star-forming main sequence and stellar mass-size relation wi…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
The Dark Energy Survey Year 3 high-redshift sample: selection, characterization, and analysis of galaxy clustering
DOI: 10.1093/mnras/stad2402 Bibcode: 2023MNRAS.525.3896S

Bechtol, K.; Smith, M.; Abbott, T. M. C. +98 more

The fiducial cosmological analyses of imaging surveys like DES typically probe the Universe at redshifts z < 1. We present the selection and characterization of high-redshift galaxy samples using DES Year 3 data, and the analysis of their galaxy clustering measurements. In particular, we use galaxies that are fainter than those used in the prev…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9