Zobrazeno 1 - 10
of 91
pro vyhledávání: '"G. B. Caminha"'
Autor:
J. D. R. Pierel, A. B. Newman, S. Dhawan, M. Gu, B. A. Joshi, T. Li, S. Schuldt, L. G. Strolger, S. H. Suyu, G. B. Caminha, S. H. Cohen, J. M. Diego, J. C. J. DŚilva, S. Ertl, B. L. Frye, G. Granata, C. Grillo, A. M. Koekemoer, J. Li, A. Robotham, J. Summers, T. Treu, R. A. Windhorst, A. Zitrin, S. Agarwal, A. Agrawal, N. Arendse, S. Belli, C. Burns, R. Cañameras, S. Chakrabarti, W. Chen, T. E. Collett, D. A. Coulter, R. S. Ellis, M. Engesser, N. Foo, O. D. Fox, C. Gall, N. Garuda, S. Gezari, S. Gomez, K. Glazebrook, J. Hjorth, X. Huang, S. W. Jha, P. S. Kamieneski, P. Kelly, C. Larison, L. A. Moustakas, M. Pascale, I. Pérez-Fournon, T. Petrushevska, F. Poidevin, A. Rest, M. Shahbandeh, A. J. Shajib, M. Siebert, C. Storfer, M. Talbot, Q. Wang, T. Wevers, Y. Zenati
Publikováno v:
The Astrophysical Journal Letters, Vol 967, Iss 2, p L37 (2024)
A bright ( m _F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detected in
Externí odkaz:
https://doaj.org/article/2158c50abcc04d72963ef0b011df2e1a
Autor:
J. D. R. Pierel, B. L. Frye, M. Pascale, G. B. Caminha, W. Chen, S. Dhawan, D. Gilman, M. Grayling, S. Huber, P. Kelly, S. Thorp, N. Arendse, S. Birrer, M. Bronikowski, R. Cañameras, D. Coe, S. H. Cohen, C. J. Conselice, S. P. Driver, J. C. J. DŚilva, M. Engesser, N. Foo, C. Gall, N. Garuda, C. Grillo, N. A. Grogin, J. Henderson, J. Hjorth, R. A. Jansen, J. Johansson, P. S. Kamieneski, A. M. Koekemoer, C. Larison, M. A. Marshall, L. A. Moustakas, M. Nonino, R. Ortiz III, T. Petrushevska, N. Pirzkal, A. Robotham, R. E. Ryan Jr., S. Schuldt, L. G. Strolger, J. Summers, S. H. Suyu, T. Treu, C. N. A. Willmer, R. A. Windhorst, H. Yan, A. Zitrin, A. Acebron, S. Chakrabarti, D. A. Coulter, O. D. Fox, X. Huang, S. W. Jha, G. Li, P. A. Mazzali, A. K. Meena, I. Pérez-Fournon, F. Poidevin, A. Rest, A. G. Riess
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 1, p 50 (2024)
Supernova (SN) SN H0pe is a gravitationally lensed, triply imaged, Type Ia SN (SN Ia) discovered in James Webb Space Telescope imaging of the PLCK G165.7+67.0 cluster of galaxies. Well-observed multiply imaged SNe provide a rare opportunity to constr
Externí odkaz:
https://doaj.org/article/5060013de8ee41a58fc63301fe908ece
Autor:
U Meštrić, E Vanzella, A Zanella, M Castellano, F Calura, P Rosati, P Bergamini, A Mercurio, M Meneghetti, C Grillo, G B Caminha, M Nonino, E Merlin, G Cupani, E Sani
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:3532-3555
We study the physical properties (size, stellar mass, luminosity, star formation rate) and scaling relations for a sample of 166 star-forming clumps with redshift $z \sim 2-6.2$. They are magnified by the Hubble Frontier Field galaxy cluster MACS~J04
Autor:
L. Tortorelli, A. Mercurio, G. Granata, P. Rosati, C. Grillo, M. Nonino, A. Acebron, G. Angora, P. Bergamini, G. B. Caminha, U. Meštrić, E. Vanzella
The wavelength dependence of the Kormendy relation (KR) is well characterised at low redshift but poorly studied at intermediate redshifts. The KR provides information on the evolution of the population of early-type galaxies (ETGs). Therefore, by st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::078e22c01371116bb62a10c2ad7993b6
http://arxiv.org/abs/2302.07896
http://arxiv.org/abs/2302.07896
Autor:
E. Vanzella, M. Castellano, P. Bergamini, T. Treu, A. Mercurio, C. Scarlata, P. Rosati, C. Grillo, A. Acebron, G. B. Caminha, M. Nonino, T. Nanayakkara, G. Roberts-Borsani, M. Bradac, X. Wang, G. Brammer, V. Strait, B. Vulcani, U. Meštrić, M. Meneghetti, F. Calura, Alaina Henry, A. Zanella, M. Trenti, K. Boyett, T. Morishita, A. Calabrò, K. Glazebrook, D. Marchesini, S. Birrer, L. Yang, T. Jones
Publikováno v:
Vanzella, E, Castellano, M, Bergamini, P, Treu, T, Mercurio, A, Scarlata, C, Rosati, P, Grillo, C, Acebron, A, Caminha, G B, Nonino, M, Nanayakkara, T, Roberts-Borsani, G, Bradac, M, Wang, X, Brammer, G, Strait, J B, Vulcani, B, Mestric, U, Meneghetti, M, Calura, F, Henry, A, Zanella, A, Trenti, M, Boyett, K, Morishita, T, Calabro, A, Glazebrook, K, Marchesini, D, Birrer, S, Yang, L & Jones, T 2022, ' Early Results from GLASS-JWST. VII. Evidence for Lensed, Gravitationally Bound Protoglobular Clusters at z=4 in the Hubble Frontier Field A2744* ', Astrophysical Journal Letters, vol. 940, no. 2, 53 . https://doi.org/10.3847/2041-8213/ac8c2d
We investigate the blue and optical rest-frame sizes (lambda~2300A-4000A) of three compact star-forming regions in a galaxy at z=4 strongly lensed (x30, x45, x100) by the Hubble Frontier Field galaxy cluster A2744 using GLASS-ERS JWST/NIRISS imaging
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07f4e20f7eb688426776194296bf9db2
https://hdl.handle.net/2434/949518
https://hdl.handle.net/2434/949518
Autor:
Franz E. Bauer, Kotaro Kohno, G. B. Caminha, Seiji Fujimoto, Daniel Espada, Jorge González-López, Nicolas Laporte, Johan Richard, Karina Caputi, Richard S. Ellis, Bunyo Hatsukade, Adi Zitrin, Masami Ouchi, G. B. Brammer, Francesco Valentino, Georgios E. Magdis, Minju Lee, Yiping Ao, Masamune Oguri, Eiichi Egami, Kirsten Kraiberg Knudsen, Yuki Yoshimura, Tao Wang
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 505 (4), pp.4838-4846. ⟨10.1093/mnras/stab191⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (4), pp.4838-4846. ⟨10.1093/mnras/stab191⟩
Monthly Notices of the Royal Astronomical Society, 505(4), 4838-4846. Oxford University Press
Laporte, N, Zitrin, A, Ellis, R S, Fujimoto, S, Brammer, G, Richard, J, Oguri, M, Caminha, G B, Kohno, K, Yoshimura, Y, Ao, Y, Bauer, F E, Caputi, K, Egami, E, Espada, D, López-Gonzáles, P J, Hatsukade, B, Kundsen, K K, Lee, M M Y, Magdis, G, Ouchi, M, Valentino, F M & Wang, T 2021, ' ALMA Lensing Cluster Survey : a strongly lensed multiply imaged dusty system at z ≥6 ', Monthly Notices of the Royal Astronomical Society, vol. 505, no. 4, pp. 4838-4846 . https://doi.org/10.1093/mnras/stab191
Monthly Notices of the Royal Astronomical Society, 2021, 505 (4), pp.4838-4846. ⟨10.1093/mnras/stab191⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 505 (4), pp.4838-4846. ⟨10.1093/mnras/stab191⟩
Monthly Notices of the Royal Astronomical Society, 505(4), 4838-4846. Oxford University Press
Laporte, N, Zitrin, A, Ellis, R S, Fujimoto, S, Brammer, G, Richard, J, Oguri, M, Caminha, G B, Kohno, K, Yoshimura, Y, Ao, Y, Bauer, F E, Caputi, K, Egami, E, Espada, D, López-Gonzáles, P J, Hatsukade, B, Kundsen, K K, Lee, M M Y, Magdis, G, Ouchi, M, Valentino, F M & Wang, T 2021, ' ALMA Lensing Cluster Survey : a strongly lensed multiply imaged dusty system at z ≥6 ', Monthly Notices of the Royal Astronomical Society, vol. 505, no. 4, pp. 4838-4846 . https://doi.org/10.1093/mnras/stab191
We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift $z=$6.07 viewed through the cluster MACSJ0600.1-2008 ($z$=0.46). A $\simeq4\sigma$ dust detection is seen at 1.2mm as part of the ALMA Lensing
Autor:
P. Bergamini, C. Grillo, P. Rosati, E. Vanzella, U. Mestric, A. Mercurio, A. Acebron, G. B. Caminha, G. Granata, M. Meneghetti, G. Angora, M. Nonino
The combination of multi-band imaging from HST with MUSE integral field spectroscopy, obtained at the VLT, has recently driven remarkable progress in strong lensing (SL) modeling of galaxy clusters. From a few tens of multiple images with photometric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64d0ddc01f2b37b47c971e7480316a03
http://arxiv.org/abs/2208.14020
http://arxiv.org/abs/2208.14020
Autor:
G. Granata, A. Mercurio, C. Grillo, L. Tortorelli, P. Bergamini, M. Meneghetti, P. Rosati, G. B. Caminha, M. Nonino
Publikováno v:
Granata, G, Mercurio, A, Grillo, C, Tortorelli, L, Bergamini, P, Meneghetti, M, Rosati, P, Caminha, G B & Nonino, M 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 & Astrophysics, vol. 659, A24 . https://doi.org/10.1051/0004-6361/202141817
From Hubble Frontier Fields photometry, and data from the Multi Unit Spectroscopic Explorer on the Very Large Telescope, we build the Fundamental Plane (FP) relation for the early-type galaxies of the cluster Abell S1063. We use this relation to deve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::15c9a605c63ac808cda512c50dd67eea
https://curis.ku.dk/ws/files/302553567/aa41817_21.pdf
https://curis.ku.dk/ws/files/302553567/aa41817_21.pdf
Autor:
E. Sani, Paolo Tozzi, Mario Nonino, Eros Vanzella, Laura Pentericci, M. Mignoli, Amata Mercurio, Adriano Fontana, Tommaso Treu, G. B. Caminha, Roberto Gilli, Francesco Calura, Andrea Grazian, Massimo Meneghetti, Max Gronke, Piero Rosati, Claudio Grillo, Mark Dijkstra, Karina Caputi, Italo Balestra, G. Cupani, Marco Castellano, Stefano Cristiani
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters, 494(1), L81-L85
We discovered a strongly lensed (\mu >40) Lya emission at z=6.629 (S/N~18) in the MUSE Deep Lensed Field (MDLF) targeting the Hubble Frontier Field galaxy cluster MACS~J0416. Dedicated lensing simulations imply that the Lya emitting region necessaril
Autor:
E. Vanzella, M. Castellano, P. Bergamini, M. Meneghetti, A. Zanella, F. Calura, G. B. Caminha, P. Rosati, G. Cupani, U. Meštrić, G. Brammer, P. Tozzi, A. Mercurio, C. Grillo, E. Sani, S. Cristiani, M. Nonino, E. Merlin, G. V. Pignataro
Publikováno v:
Vanzella, E, Castellano, M, Bergamini, P, Meneghetti, M, Zanella, A, Calura, F, Caminha, G B, Rosati, P, Cupani, G, Mestric, U, Brammer, G, Tozzi, P, Mercurio, A, Grillo, C, Sani, E, Cristiani, S, Nonino, M, Merlin, E & Pignataro, G 2022, ' High star cluster formation efficiency in the strongly lensed Sunburst Lyman-continuum galaxy at z=2.37 ', Astronomy & Astrophysics, vol. 659, A2 . https://doi.org/10.1051/0004-6361/202141590
We investigate the strongly lensed (\mu x10-100) Lyman continuum (LyC) galaxy, dubbed Sunburst, at z=2.37, taking advantage of a new accurate model of the lens. A characterization of the intrinsic (delensed) properties of the galaxy yields a size of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c5451078d85e5c7f7fa3f89e632c68c
https://hdl.handle.net/11386/4807896
https://hdl.handle.net/11386/4807896