Publikationen von G. B. Caminha
Alle Typen
Zeitschriftenartikel (32)
21.
Zeitschriftenartikel
935 (2), 110 (2022)
The GLASS-JWST early release science program. I. Survey design and release plans. The Astrophysical Journal 22.
Zeitschriftenartikel
516 (3), S. 3532 - 3555 (2022)
Exploring the physical properties of lensed star-forming clumps at 2 ≲ z ≲ 6. Monthly Notices of the Royal Astronomical Society 23.
Zeitschriftenartikel
930 (2), 128 (2022)
The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ≈ 3–6.5. The Astrophysical Journal 24.
Zeitschriftenartikel
659, A24 (2022)
Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063. Astronomy and Astrophysics 25.
Zeitschriftenartikel
659, A2 (2022)
High star cluster formation efficiency in the strongly lensed Sunburst Lyman-continuum galaxy at z = 2.37. Astronomy and Astrophysics 26.
Zeitschriftenartikel
926 (1), 86 (2022)
VLT/MUSE observations of SDSS J1029+2623: Toward a high-precision strong lensing model. The Astrophysical Journal 27.
Zeitschriftenartikel
657, A83 (2022)
Galaxy cluster strong lensing cosmography - Cosmological constraints from a sample of regular galaxy clusters. Astronomy and Astrophysics 28.
Zeitschriftenartikel
656, A147 (2021)
CLASH-VLT: Abell S1063 - Cluster assembly history and spectroscopic catalogue. Astronomy and Astrophysics 29.
Zeitschriftenartikel
655, A81 (2021)
A strong lensing model of the galaxy cluster PSZ1 G311.65-18.48. Astronomy and Astrophysics 30.
Zeitschriftenartikel
648, A123 (2021)
Cluster strong lensing with hierarchical inference - Formalism, functional tests, and public code release. Astronomy and Astrophysics 31.
Zeitschriftenartikel
648, A47 (2021)
Systematic search for lensed X-ray sources in the CLASH fields. Astronomy and Astrophysics 32.
Zeitschriftenartikel
645, A140 (2021)
A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403: Robust characterization of the cluster mass distribution from VLT/MUSE deep observations. Astronomy and Astrophysics