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  1. Home
  2. Browse by Author

Browsing by Author "Bina, D."

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    Faint end of the z ∼ 3-7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE
    (2019) de La Vieuville, G.; Bina, D.; Pello, R.; Mahler, G.; Richard, J.; Drake, A. B.; Herenz, E. C.; Bauer, F. E.; Clement, B.; Lagattuta, D.; Laporte, N.; Martinez, J.; Patricio, V.; Wisotzki, L.; Zabl, J.; Bouwens, R. J.; Contini, T.; Garel, T.; Guiderdoni, B.; Marino, R. A.; Maseda, M. V.; Matthee, J.; Schaye, J.; Soucail, G.
    Contact. This paper presents the results obtained with the Multi-Unit Spectroscopic Explorer (MUSE) at the ESOVery Large Telescope on the faint end of the Lyman-alpha luminosity function (LF) based on deep observations of four lensing clusters. The goal of our project is to set strong constraints on the relative contribution of the Lyman-alpha emitter (LAE) population to cosmic reionization.
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    Frontier Fields: Combining HST, VLT, and Spitzer data to explore the z ∼ 8 Universe behind the lensing cluster MACSJ0416.1-2403
    (2015) Laporte, N.; Streblyanska, A.; Kim, S.; Pello, R.; Bauer, F. E.; Bina, D.; Brammer, G.; De Leo, M. A.; Infante, L.; Perez-Fournon, I.
    Context. The Hubble Space Telescope (HST) Frontier Fields (HFFs) project started at the end of 2013 with the aim of providing extremely deep images of six massive galaxy clusters. One of the main goals of this program is to push several telescopes to their limits to provide the best current view of the earliest stages of the Universe. The analysis of the initial data has already demonstrated the huge capabilities of the program.
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    YOUNG GALAXY CANDIDATES IN THE HUBBLE FRONTIER FIELDS. III. MACS J0717.5+3745
    (2016) Laporte, Nicolás; Infante Lira, Leopoldo; Troncoso Iribarren, P.; Zheng, W.; Molino, A.; Bauer, Franz Erik; Bina, D.; Broadhurst, Tom; Chilingarian, I.; Huang, X.; García, S.; Kim, S.; Marques Chaves, R.; Moustakas, J.; Pelló, R.; Pérez Fournon, I.; Shu, X.; Streblyanska, A.; Zitrin, A.

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