Results 31 to 40 of about 14,388 (158)
ZEN2: A narrow J-band search for z~9 Lya emitting galaxies directed
towards three lensing clusters [PDF]
, 2007 We present the results of a continuing survey to detect Lya emitting galaxies
at redshifts z~9: the ZEN ("z equals nine'') survey. We have obtained deep
VLT/ISAAC observations in the narrow J-band filter NB119 directed towards three
massive lensing ...Barton, Bertin, Bouwens, Broadhurst, Bunker, Campusano, Casali, Cuby, D. Minniti, Dickinson, Eyles, F. Courbin, Fan, Gunn, Haiman, Hempel, Horton, Hu, Hu, Iye, J. P. Willis, J.-P. Kneib, Kashikawa, Kneib, Le Delliou, Limousin, Page, Puget, Rhoads, Santos, Santos, Smith, Stanway, Stark, Taniguchi, Willis, Yan +36 morecore +2 more sourcesResolving dust and Lyman α emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS
Astronomy & AstrophysicsContext. Lyman α (Lyα) emission is highly sensitive to dust and neutral hydrogen and is believed to be suppressed in dusty or hydrogen-rich galaxies – especially during the epoch of reionization (EoR).Markov V., Bradač M., Estrada-Carpenter V., Desprez G., Rihtaršič G., Judež J., Tripodi R., Sawicki M., Noirot G., Martis N., Willott C., Abraham R., Asada Y., Brammer G., Matharu J., Muzzin A., Sarrouh G. T. E., Withers S., Ferrara A., Fujimoto S., Gallerani S., Goovaerts I., Harshan A. +22 moredoaj +1 more sourceThe Kinematics of Multiple-Peaked Lyα Emission in Star-Forming Galaxies at z ~ 2-3 [PDF]
, 2012 We present new results on the Lyα emission-line kinematics of 18 z ~ 2-3 star-forming galaxies with multiple-peaked Lyα profiles. With our large spectroscopic database of UV-selected star-forming galaxies at these redshifts, we have determined that ~30 ...Hainline, Kevin N., Kollmeier, Juna A., Kulas, Kristin R., Shapley, Alice E., Steidel, Charles C., Zheng, Zheng +5 morecore A Systematic Survey of Protoclusters at $z\sim3\mathrm{-}6$ in the
CFHTLS Deep Fields [PDF]
, 2016 We present the discovery of three protoclusters at $z\sim3\mathrm{-}4$ with
spectroscopic confirmation in the Canada-France-Hawaii Telescope (CFHT) Legacy
Survey Deep Fields.Furusawa, Hisanori, Ishikawa, Shogo, Kashikawa, Nobunari, Malkan, Matthew A., Niino, Yuu, Onoue, Masafusa, Ota, Kazuaki, Overzier, Roderik, Tanaka, Masayuki, Toshikawa, Jun, Uchiyama, Hisakazu +10 morecore +2 more sourcesUsing Lyα Absorption to Measure the Intensity and Variability of z ∼ 2.4 Ultraviolet Background Light
The Astrophysical JournalWe present measurements of z ∼ 2.4 ultraviolet (UV) background light using Ly α absorption from galaxies at z ∼ 2–3 in the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) database.Laurel H. Weiss, Karl Gebhardt, Dustin Davis, Erin Mentuch Cooper, Maja Lujan Niemeyer, Mahdi Qezlou, Mahan Mirza Khanlari, Robin Ciardullo, Daniel Farrow, Eric Gawiser, Simon Gazagnes, Caryl Gronwall, Gary J. Hill, Donald P. Schneider +13 moredoaj +1 more sourcePhysical properties of z~4 LBGs: differences between galaxies with and
without Ly-alpha emission
, 2007 We have analysed the physical properties of z~4 Lyman Break Galaxies observed
in the GOODS-S survey, in order to investigate the possible differences between
galaxies where the Ly-alpha is present in emission, and those where the line is
absent or in ...A. Fontana, A. Grazian, Bouwens, Bruzual, C. De Santis, Cowie, Dickinson, Dickinson, Drory, E. Giallongo, Fontana, Fontana, Fontana, Fujita, Gawiser, Giavalisco, Grazian, Grazian, Hansen, Iwata, Iye, Kashikawa, Keel, L. Pentericci, Lai, Le Fevre, Leitherer, Madau, Malhotra, Mori, Ouchi, Ouchi, P. Santini, Papovich, Rhoads, S. Gallozzi, S. Salimbeni, Shapley, Shapley, Steidel, Steidel, Steidel, Tapken, Thommes, Vanzella, Vanzella, Venemans, Venemans +47 morecore +1 more sourceMAMMOTH-Subaru. IV. Large Scale Structure and Clustering Analysis of Lyα Emitters and Lyα Blobs at z = 2.2–2.3
The Astrophysical JournalWe report the large scale structure and clustering analysis of Ly α emitters (LAEs) and Ly α blobs (LABs) at z = 2.2–2.3. Using 3341 LAEs, 117 LABs, and 58 bright (Ly α luminosity L _Ly _α > 10 ^43.4 erg s ^−1 ) LABs at z = 2.2–2.3 selected with ...Haibin Zhang, Zheng Cai, Mingyu Li, Yongming Liang, Nobunari Kashikawa, Ke Ma, Yunjing Wu, Qiong Li, Sean D. Johnson, Satoshi Kikuta, Masami Ouchi, Xiaohui Fan, Yuanhang Ning +12 moredoaj +1 more sourceGas Accretion and Giant Lyman-alpha Nebulae
, 2016 Several decades of observations and discoveries have shown that high-redshift
AGN and massive galaxies are often surrounded by giant Lyman-alpha nebulae
extending in some cases up to 500 kpc in size.A. Basu-Zych, A. Bunker, A. Dekel, A. Dey, A. Humphrey, A. Humphrey, A. Humphrey, A. Humphrey, B. P. Venemans, C. C. Steidel, C. C. Steidel, C. C. Steidel, C. C. Steidel, C. Leitherer, C. Scarlata, C.-A. Faucher-Giguère, D. C. Martin, D. C. Martin, D. E. Osterbrock, D. J. B. Smith, D. P. Schneider, E. Borisova, E. C. Herenz, E. Lusso, E. M. Hu, E. M. Hu, F. Arrigoni Battaia, F. Arrigoni Battaia, F. Courbin, F. Valentino, H. J. A. Röttgering, J. A. Kollmeier, J. Bergeron, J. Bergeron, J. D. Kurk, J. E. Geach, J. E. Geach, J. F. Hennawi, J. F. Hennawi, J. G. Baker, J. Rosdahl, J. W. Fried, J. X. Prochaska, K. K. Nilsson, L. Christensen, L. Pentericci, L. Wisotzki, M. A. Fardal, M. Beck, M. Dijkstra, M. Dijkstra, M. Fumagalli, M. Hayes, M. K. M. Prescott, M. K. M. Prescott, M. K. M. Prescott, M. K. M. Prescott, M. Reuland, M. Trebitsch, M. Villar-Martín, M. Villar-Martín, M. Weidinger, M. Weidinger, N. K. Hine, N. P. H. Nesvadba, N. P. H. Nesvadba, N. Roche, P. D. Barthel, P. J. Francis, P. J. Francis, P. J. McCarthy, P. J. McCarthy, P. J. McCarthy, P. J. McCarthy, P. L. North, P. Møller, P. Palunas, R. A. Overzier, R. Antonucci, R. Antonucci, R. F. Trainor, R. Ojik van, R. Ojik van, S. A. Eales, S. C. Chapman, S. C. Chapman, S. Cantalupo, S. Cantalupo, S. Cantalupo, S. Cantalupo, S. Cantalupo, S. Djorgovski, S. F. Sánchez, S. J. Lilly, S. R. Furlanetto, S. Veilleux, T. Goerdt, T. M. Heckman, T. Saito, W. C. Keel, Y. Ao, Y. Matsuda, Y. Matsuda, Y. Shen, Y. Taniguchi, Y. Ueda, Y. Yang, Y. Yang, Z. Haiman +108 morecore +1 more sourceDetecting Early Galaxies Through Their 21-cm Signature [PDF]
, 2007 New observations over the next few years of the emission of distant objects
will help unfold the chapter in cosmic history around the era of the first
galaxies. These observations will use the neutral hydrogen emission or
absorption at a wavelength of 21-Barkana R., Hogan C. J., Kaiser N., Rennan Barkana, Smadar Naoz, Wouthuysen S. A. +5 morecore +2 more sources