output
20032026
most citedGaia Data Release 3: Summary of the content and survey properties

4.2k citations

Showing astro-ph.GAShow all

15 papers · 1 filter

astro-ph.GA2025★ 12 cited

SIEGE IV: compact star clusters in cosmological simulations with high star formation efficiency and sub-parsec resolution

R. Pascale, F. Calura, E. Vesperini +10

The formation of compact high-redshift star-forming clumps, the physical processes driving their evolution and their potential connection to present-day Globular Clusters are key o…

astro-ph.GA2024★ 1 cited

A Glimpse of the New Redshift Frontier Through Abell S1063

Vasily Kokorev, Hakim Atek, John Chisholm +31

We report the discovery of two galaxy candidates at redshifts between in JWST observations from the GLIMPSE survey. These robust sources were identified using a combi…

astro-ph.GA2024★ 29 cited

Evidence for Very Massive Stars in extremely UV-bright star-forming galaxies at

A. Upadhyaya, R. Marques-Chaves, D. Schaerer +4

We present a comprehensive analysis of the presence of very massive stars (VMS > ) in the integrated spectra of 13 UV-bright star-forming galaxies at $2.2 \lesssim z…

astro-ph.GA2023★ 9 cited

Five methods for determining pattern speeds in galaxies

Daniel Pfenniger, Kanak Saha, Yu-Ting Wu

Aims. New or refined methods for determining instantaneous scalar and vector pattern speeds from a restricted domain are developed, for applications in N-body simulations or in gal…

astro-ph.GA2022★ 4.2k cited

Gaia Data Release 3: Summary of the content and survey properties

Gaia Collaboration, A. Vallenari, A. G. A. Brown +453

We present the third data release of the European Space Agency's Gaia mission, GDR3. The GDR3 catalogue is the outcome of the processing of raw data collected with the Gaia instrum…

astro-ph.GA2022★ 14 cited

Multi-wavelength properties of 850-m selected sources from the North Ecliptic Pole SCUBA-2 survey

H. Shim, D. Lee, Y. Kim +25

We present the multi-wavelength counterparts of 850-m selected submillimetre sources over a 2-deg field centred on the North Ecliptic Pole. In order to overcome the large be…