Search Publications

The Ancient Star Formation History of the Extremely Low-mass Galaxy Leo P: An Emerging Trend of a Post-reionization Pause in Star Formation
DOI: 10.3847/1538-4357/ad8158 Bibcode: 2024ApJ...976...60M

McQuinn, Kristen B. W.; Cannon, John M.; Dolphin, Andrew E. +12 more

Isolated, low-mass galaxies provide the opportunity to assess the impact of reionization on their star formation histories (SFHs) without the ambiguity of environmental processes associated with massive host galaxies. There are very few isolated, low-mass galaxies that are close enough to determine their SFHs from resolved star photometry reaching…

2024 The Astrophysical Journal
JWST 4
Limitations and rotation of the two-armed phase spiral in the Milky Way stellar disc
DOI: 10.1051/0004-6361/202451387 Bibcode: 2024A&A...690A..15A

McMillan, P. J.; Bensby, T.; Alinder, S.

Context. The Milky Way's history of recent disturbances is vividly demonstrated by a structure in the vertical phase-space distribution known as the Gaia phase spiral. A one-armed phase spiral has been seen widely across the Milky Way disc, while a two-armed one has only been observed in the solar neighbourhood. Aims. This study aims to determine …

2024 Astronomy and Astrophysics
Gaia 4
Revealing the burning and soft heart of the bright bare active galactic nucleus ESO 141-G55: X-ray broadband and SED analysis
DOI: 10.1051/0004-6361/202449708 Bibcode: 2024A&A...689A.336P

Grosso, N.; Porquet, D.; Reeves, J. N. +4 more

Context. ESO 141-G55 is a nearby X-ray bright broad-line Seyfert 1 (BLS1) that has been classified as a bare active galactic nucleus (AGN) due to a lack of warm absorption along its line of sight, providing an unhampered view into its disc-corona system. Aims. We aim to probe its disc-corona system thanks to the first simultaneous XMM-Newton and N…

2024 Astronomy and Astrophysics
XMM-Newton 4
UVIT Study of the MAgellanic Clouds (U-SMAC). II. A Far-UV Catalog of the Small Magellanic Cloud: Morphology and Kinematics of Young Stellar Population
DOI: 10.3847/1538-3881/ad7de2 Bibcode: 2024AJ....168..255H

Subramaniam, Annapurni; Subramanian, Smitha; Nayak, Prasanta K. +1 more

The Small Magellanic Cloud (SMC) is an irregular dwarf galaxy that has recently undergone an interaction with the Large Magellanic Cloud. The young massive stars in the SMC formed in the disturbed low-metallicity environment are important targets in astrophysics. We present a catalog of ∼76,800 far-ultraviolet (FUV) sources toward the SMC detected…

2024 The Astronomical Journal
Gaia 4
The White-light Superflares from Cool Stars in GWAC Triggers
DOI: 10.3847/1538-4357/ad55e8 Bibcode: 2024ApJ...971..114L

Wang, Jing; Wang, Liang; Liang, En-Wei +16 more

M-type stars are the ones that flare most frequently, but how big their maximum flare energy can reach is still unknown. We present 163 flares from 162 individual M2 through L1-type stars that triggered the GWAC, with flare energies ranging from 1032.2 to 1036.4 erg. The flare amplitudes range from △G = 0.84 to ∼10 mag. Flare…

2024 The Astrophysical Journal
Gaia 4
PYSSED: an automated method of collating and fitting stellar spectral energy distributions
DOI: 10.1093/rasti/rzae005 Bibcode: 2024RASTI...3...89M

McDonald, Iain; Zijlstra, Albert A.; Cox, Nick L. J. +4 more

Stellar atmosphere modelling predicts the luminosity and temperature of a star, together with parameters such as the effective gravity and the metallicity, by reproducing the observed spectral energy distribution. Most observational data come from photometric surveys, using a variety of passbands. We herein present the Python Stellar Spectral Ener…

2024 RAS Techniques and Instruments
Gaia 4
Investigating X-ray emission in the GeV-emitting compact symmetric objects PKS 1718-649 and TXS 1146+596
DOI: 10.1051/0004-6361/202348208 Bibcode: 2024A&A...684A..65B

Vignali, C.; Giroletti, M.; Stawarz, Ł. +8 more


Aims: Compact symmetric objects (CSOs) are thought to represent the first step in the evolutionary path of radio galaxies. In the present study, we investigated the X-ray emission of two CSOs confirmed to emit at GeV energies: PKS 1718-649 and TXS 1146+596. Unveiling the origin of their observed high-energy emission is crucial to establishing…

2024 Astronomy and Astrophysics
XMM-Newton 4
The population of young low-mass stars in Trumpler 14
DOI: 10.1051/0004-6361/202347380 Bibcode: 2024A&A...685A.100I

Testi, Leonardo; Reiter, Megan; Hennebelle, Patrick +8 more

Massive star-forming regions are thought to be the most common birth environments in the Galaxy and the only birth places of very massive stars. Their presence in the stellar cluster alters the conditions within the cluster, impacting at the same time the evolution of other cluster members. In principle, copious amounts of ultraviolet radiation pr…

2024 Astronomy and Astrophysics
Gaia 4
Nano-Newton electrostatic force actuators for femto-Newton-sensitive measurements: System performance test in the LISA Pathfinder mission
DOI: 10.1103/PhysRevD.109.102009 Bibcode: 2024PhRvD.109j2009A

Mendes, L.; Russano, G.; Nofrarias, M. +89 more

Electrostatic force actuation is a key component of the system of geodesic reference test masses (TM) for the LISA orbiting gravitational wave observatory and in particular for performance at low frequencies, below 1 mHz, where the observatory sensitivity is limited by stray force noise. The system needs to apply forces of order 10-9 N …

2024 Physical Review D
LISAPathfinder 4
A complex node of the cosmic web associated with the massive galaxy cluster MACS J0600.1-2008
DOI: 10.1093/mnras/stae1943 Bibcode: 2024MNRAS.533.2242F

Koekemoer, Anton M.; Mahler, Guillaume; Richard, Johan +18 more

MACS J0600.1-2008 (MACS0600) is an X-ray-luminous, massive galaxy cluster at $z_{\mathrm{d}}=0.43$, studied previously by the REionization LensIng Cluster Survey and ALMA Lensing Cluster Survey projects which revealed a complex, bimodal mass distribution and an intriguing high-redshift object behind it. Here, we report on the results of a combined…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST JWST 4