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Identification of the brightest Ly\alpha\ emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era

J. Matthee, D. Sobral, S. Santos, H. Röttgering, B. Darvish, und B. Mobasher. (2015)cite arxiv:1502.07355Comment: 20 pages, main results shown in Fig. 6 and Fig. 7, submitted to MNRAS.

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Mona Mobasher

Amin Mobasher

Bahram Bastani

Bahram Bahrami

Bahram Kakavand

Weitere Publikationen von Autoren mit dem selben Namen

On the nature of the luminous Lya emitter CR7 and its UV components: physical conditions and JWST predictionsD. Sobral, J. Matthee, G. Brammer, A. Ferrara, L. Alegre, H. Rottgering, D. Schaerer, B. Mobasher, und B. Darvish. (2017)cite arxiv:1710.08422Comment: Submitted to MNRAS, comments welcomed. 19 pages, 11 figures.Searching for z > 6.5 Analogs Near the Peak of Cosmic Star FormationX. Du, A. Shapley, M. Tang, D. Stark, C. Martin, B. Mobasher, M. Topping, und J. Chevallard. (2019)cite arxiv:1910.11877Comment: 21 pages, 9 figures, submitted to ApJ.The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z~1.4-2.6N. Reddy, M. Kriek, A. Shapley, W. Freeman, B. Siana, A. Coil, B. Mobasher, S. Price, R. Sanders, und I. Shivaei. (2015)cite arxiv:1504.02782Comment: 24 pages, 2 tables, 24 figures, accepted to the Astrophysical Journal.New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark EnergyA. Riess, L. Strolger, S. Casertano, H. Ferguson, B. Mobasher, B. Gold, P. Challis, A. Filippenko, S. Jha, W. Li und 11 andere Autor(en). (2006)The clustering of H$\beta$+OIII and OII emitters since $z 5$: dependencies with line luminosity and stellar massA. Khostovan, D. Sobral, B. Mobasher, P. Best, I. Smail, J. Matthee, B. Darvish, H. Nayyeri, S. Hemmati, und J. Stott. (2017)cite arxiv:1705.01101Comment: 19 pages, 11 figures, 4 tables, submitted to MNRAS.Evolution of the H$\beta$+OIII and OII luminosity functions and the OII star-formation history of the Universe up to $z$ ~ 5 from HiZELSA. Khostovan, D. Sobral, B. Mobasher, P. Best, I. Smail, J. Stott, S. Hemmati, und H. Nayyeri. (2015)cite arxiv:1503.00004Comment: 23 pages, 14 figures, 7 Tables, submitted to MNRAS.The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion YearsS. Finkelstein, R. Ryan Jr., C. Papovich, M. Dickinson, M. Song, R. Somerville, H. Ferguson, B. Salmon, M. Giavalisco, A. Koekemoer und 19 andere Autor(en). (2014)cite arxiv:1410.5439Comment: Submitted to the Astrophysical Journal. 33 pages, 20 figures, 7 tables.Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy EvolutionA. Riess, L. Strolger, J. Tonry, S. Casertano, H. Ferguson, B. Mobasher, P. Challis, A. Filippenko, S. Jha, W. Li und 9 andere Autor(en). (2004)cite arxiv:astro-ph/0402512 Comment: Accepted Astrophysical Journal, to Appear June 2004 72 pages, 17 Figures.The MOSDEF Survey: Detection of OIII$łambda$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08R. Sanders, A. Shapley, M. Kriek, N. Reddy, W. Freeman, A. Coil, B. Siana, B. Mobasher, I. Shivaei, S. Price und 1 andere Autor(en). (2016)cite arxiv:1606.04107Comment: 7 pages, 3 figures, 1 table, submitted to ApJ Letters.Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844 - 7.213: Lyman Alpha Demography of z ~ 7 GalaxiesY. Ono, M. Ouchi, B. Mobasher, M. Dickinson, K. Penner, K. Shimasaku, B. Weiner, J. Kartaltepe, K. Nakajima, H. Nayyeri und 3 andere Autor(en). (2011)cite arxiv:1107.3159Comment: 14 pages, 8 figures, submitted to ApJ.

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