Large-Scale Structure of Emission-Line Galaxies at z = 3.1

By T. Hayashino, Y. Matsuda, H. Tamura, R. Yamauchi, Toru Yamada, M. Ajiki, S. Fujita, T. Murayama, Tohru Nagao, K. Ohta and 5 more. 2004

179 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/e6550ffe5e8e10cfb0fe062f0b42fb55a7aa8889

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In Astronomy and Astrophysics

1. P. Hopkins
2. L. Hernquist
3. M. Ouchi
4. A. Shapley
5. R. Dav'e
6. Naveen A. Reddy
7. P. V. van Dokkum
8. C. Steidel

In Instrumentation

1. A. Shapley
2. Naveen A. Reddy
3. C. Steidel
4. D. Erb
5. P. V. van Dokkum
6. M. Pettini
7. M. Franx
8. M. Ouchi

Citations in the corpus

• Lyα Emitting Galaxies as a Probe of Reionisation (2014, background): “…there is increasing observational support for the presence of spatially extended Lyα halos around star-forming galaxies (Fynbo, Møller, & Warren 1999; Hayashino et al. 2004; Hayes et al. 2005, 2007; Rauch et al. 2008; Östlin et al. 2009; Steidel et al. 2011; Matsuda et al. 2012; Hayes et al.…”
• The realm of the galaxy protoclusters (2016, background): “…is most likely due to scattered Lyα photons from central or extended star formation, AGN, and perhaps some amount of gravitational cooling radiation (e.g., Hayashino et al., 2004; Saito et al., 2006; Zheng et al., 2011; Steidel et al., 2011; Dijkstra & Kramer, 2012; Matsuda et al., 2012; Momose et…”
• Distant radio galaxies and their environments (2008, background): “…with several overdense regions found at large redshifts in the form of ”redshift spikes” or ”filaments” (e.g. Steidel et al 1998; Keel et al 1999; Steidel et al 2000; Möller and Fynbo 2001; Shimasaku et al 2003; Hayashino et al 2004; Matsuda et al 2005; Steidel et al 2005; Ouchi et al 2005).”
• DIFFUSE Lyα EMITTING HALOS: A GENERIC PROPERTY OF HIGH-REDSHIFT STAR-FORMING GALAXIES (2011, methodology): “Perhaps more directly analogous to the results of the present sample is the narrow-band Lyα survey of Hayashino et al. (2004).”
• Lyα Emission-Line Galaxies at z = 3.1 in the Extended Chandra Deep Field-South (2007, background): “…for Ly emission have been successfully conducted at a number of redshifts, including z 2:4 (Stiavelli et al. 2001), z 3:1 (Ciardullo et al. 2002; Hayashino et al. 2004; Venemans et al. 2005; Gawiser et al. 2006a), z 3:7 (Fujita et al. 2003), z 4:5 (Rhoads et al. 2000), z 4:9 (Ouchi et al.…”
• The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα Emitters from z = 3.1 to 5.7 in the 1 deg2 Field: Luminosity Functions and AGN (2007, background): “…2006; Kashikawa et al. 2006; Venemans et al. 2007), and the numbers are increasing from recent and ongoing wide-field projects such as the WFILAS (Westra et al. 2005, 2006), MUSYC (Gawiser et al. 2006; Gronwall et al. 2007), Hawaii (see Hu & Cowie 2006), and SSA22 surveys (Hayashino et al. 2004).”
• Spectroscopic Identification of a Protocluster at z = 2.300: Environmental Dependence of Galaxy Properties at High Redshift (2005, background): “Subsequent analysis of narrow-band Lyman α images over a much larger field by Hayashino et al. (2004) has shown that the initial SSA22 pointing was indeed the densest proto-cluster-sized sub-region within a largescale structure extending over a ∼ 60 Mpc co-moving scale.”
• Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program strategy and clustering properties of ∼2000 Lyα emitters at z = 6–7 over the 0.3–0.5 Gpc2 survey area (2017, background): “Outside the highly-ionized ISM, LAEs show diffuse extended Lyα halos in the circumgalactic medium (CGM) up to a few 10 kpc (Hayashino et al. 2004; Steidel et al. 2011).”
• SILVERRUSH. IV. Lyα luminosity functions at z = 5.7 and 6.6 studied with ∼1300 Lyα emitters on the 14–21 deg2 sky (2017, background): “…surveys (e.g., Cowie & Hu 1998; Hu et al. 1998; Rhoads et al. 2000; Steidel et al. 2000; Malhotra & Rhoads 2002; Ajiki et al. 2002; Ouchi et al. 2003; Hayashino et al. 2004; Matsuda et al. 2004; Taniguchi et al. 2005; Iye et al. 2006; Kashikawa et al. 2006; Shimasaku et al. 2006; Gronwall et al.…”
• The MUSE Hubble Ultra Deep Field Survey - VIII. Extended Lyman-α haloes around high-z star-forming galaxies (2017, background): “Later, Hayashino et al. (2004) observed 22 Lyman break galaxies (LBG) and detected extended Lyα emission by stacking the NB images.”
• Extended Lyman α haloes around individual high-redshift galaxies revealed by MUSE (2015, background): “Hayashino et al. (2004) discovered LAEs embedded in largescale extended Lyα emission and presented a first composite Lyα image providing clear evidence of excess flux beyond the PSF. Nilsson et al. (2009) compared the widths of a large sample of z ' 2.2 LAE candidates and noted that they were…”
• Protoclusters associated with z > 2 radio galaxies - I. Characteristics of high redshift protoclusters (2006, methodology): “More recently, Hayashino et al. (2004) measured the blank field space density of Lyα emitters atz ∼ 3.1 using the Suprime-Cam on the Subaru telescope.”
• THE STRUCTURE AND KINEMATICS OF THE CIRCUMGALACTIC MEDIUM FROM FAR-ULTRAVIOLET SPECTRA OF z ≃ 2–3 GALAXIES (2010, background): “…has already been observed in very deep Lyα images in the form of Lyα “Blobs” (Steidel et al. 2000; Matsuda et al. 2004)– the most extreme examples– or as diffuse emission evident only after stacking spatial regions surrounding normal LBGs (Hayashino et al. 2004, Steidel et al, in preparation).”