Results 61 to 70 of about 252,176 (198)
A New Constraint on the Ly$\alpha$ Fraction of UV Very Bright Galaxies
at Redshift 7
, 2016 We study the extent to which very bright (-23.0 < MUV < -21.75) Lyman-break
selected galaxies at redshifts z~7 display detectable Lya emission. To explore
this issue, we have obtained follow-up optical spectroscopy of 9 z~7 galaxies
from a parent sample ...Dunlop, James S., Fevre, Olivier Le, Furusawa, Hisanori, Furusawa, Junko, Fynbo, Johan P. U., Kajisawa, Masaru, Kashikawa, Nobunari, Kobayashi, Masakazu A. R., Naito, Yoshiaki, Nakata, Fumiaki, Okura, Yuki, Ouchi, Masami, Sekiguchi, Kazuhiro, Shimasaku, Kazuhiro, Takata, Tadafumi, Taniguchi, Yoshiaki, Yamada, Toru, Yasuda, Naoki +17 morecore +4 more sourcesThe Magellan M2FS Spectroscopic Survey of High-redshift Galaxies: A Sample of 260 Lyα Emitters at Redshift z ≈ 5.7 [PDF]
Astrophysical Journal, 2020 We present a spectroscopic survey of Lyα emitters (LAEs) at z ≈ 5.7 using the multiobject spectrograph M2FS on the Magellan Clay telescope. This is part of a high-redshift galaxy survey carried out in several well-studied deep fields.Y. Ning, Linhua Jiang, Zhen-ya Zheng, Jin Wu, F. Bian, E. Egami, Xiaohui Fan, L. Ho, Yue Shen, Ran Wang, Xue-bing Wu +10 moresemanticscholar +1 more sourceProperties of Ly-alpha emitters around the radio galaxy MRC 0316-257
, 2005 Observations of the radio galaxy MRC 0316-257 at z=3.13 and the surrounding
field are presented. Using narrow- and broad-band imaging obtained with the
VLT, 77 candidate Ly-alpha emitters with a rest-frame equivalent width of > 15
A were selected in a ~7'Adelberger, Aguirre, Ajiki, Appenzeller, Archibald, Athreya, B. P. Venemans, Baldwin, Baugh, Beers, Bennert, Bertin, Bessell, Best, Best, Blakeslee, Blakeslee, Brocklehurst, Bunker, C. De Breuck, C. L. Carilli, Carilli, Chambers, Ciardullo, Cowie, Dawson, De Breuck, De Breuck, De Breuck, De Breuck, De Breuck, Della Ceca, Deutsch, Dey, Ferguson, Fouqué, Friaça, Fruchter, Fynbo, Fynbo, G. K. Miley, Giavalisco, Giavalisco, H. Ford, H. J. A. Röttgering, Hashimoto, Heckman, Hill, Hu, Hu, Hunt, J. D. Kurk, Jarvis, Keel, Keel, Kudritzki, Kurk, L. Pentericci, Lahav, Landolt, Large, Le Fèvre, Leitherer, Lia, Madau, Madau, Maier, Malhotra, Maughan, Maughan, McCarthy, Monet, Moorwood, Mushotzky, Oke, P. McCarthy, Papadopoulos, Pascarelle, Pentericci, Pentericci, Pentericci, Pentericci, Pettini, Press, R. A. Overzier, Reuland, Rhoads, Rosati, Rosati, Röttgering, Schlegel, Shapley, Shapley, Shimasaku, Spergel, Stanford, Steidel, Steidel, Steidel, Steidel, Steidel, Stevens, Stone, T. Heckman, Tapken, Thommes, Toft, Tozzi, Venemans, Venemans, Venemans, Vernet, W. J. M. van Breugel, White, Willott, Zirm +115 morecore +1 more sourceA search for clusters at high redshift - III. Candidate H-alpha emitters
and EROs in the PKS 1138-262 proto-cluster at z=2.16 [PDF]
, 2004 In this paper we present deep VLT multi wavelength imaging observations of
the field around the radio galaxy PKS 1138-262 aimed at detecting and studying
a (potential) proto-cluster centered at this radio source.Abell, Bahcall, Bahcall, Beers, Bertin, Best, Bower, Bruzual, Buat, Bunker, Butcher, Carilli, Carilli, Cowie, Cowie, Daddi, Daddi, De Breuck, De Breuck, De Propris, Dey, Donahue, Dressler, Eggen, Eke, Elston, Elston, Feigelson, Fynbo, Fynbo, Fynbo, Gladders, Glazebrook, Hamuy, Hamuy, Hill, Hoeg, Hu, Iglesias-Páramo, Infante, Ivison, Jarvis, Kauffmann, Kauffmann, Kennicutt, Kennicutt, Kennicutt, Kron, Kurk, Kurk, Lacy, Lacy, Leitherer, Madau, McLure, Moorwood, Møller, Nakata, Oke, Ouchi, Pentericci, Pentericci, Pentericci, Pentericci, Pentericci, Pozzetti, Prentice, Refregier, Rhoads, Rhoads, Rosati, Rosati, Röttgering, Salpeter, Schlegel, Scodeggio, Small, Stanford, Stanford, Stanford, Steidel, Steidel, Stiavelli, Taylor, van Breugel, van der Werf, van Dokkum, van Dokkum, van Dokkum, Venemans, Yates +90 morecore +4 more sourcesPhysical 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 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 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 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 source