NAME SXDF-S , the SIMBAD biblio

NAME SXDF-S , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:34:16


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Title First 3 Authors
2006ApJ...648...54S 44 57 Systematic survey of extended Lyα sources over z ∼ 3-5. SAITO T., SHIMASAKU K., OKAMURA S., et al.
2007MNRAS.376L..20F 54           X         1 1 52 Number counts and clustering properties of bright distant red galaxies in the UKIDSS Ultra Deep Survey Early Data Release. FOUCAUD S., ALMAINI O., SMAIL I., et al.
2008ApJ...675.1076S 37           X         1 24 31 Deep spectroscopy of systematically surveyed extended Lyα sources at z ∼ 3-5. SAITO T., SHIMASAKU K., OKAMURA S., et al.
2008ApJ...676..121M 39           X         1 3 15 The Subaru/XMM-Newton Deep Survey (SXDS). VI. Properties of active galactic nuclei selected by optical variability. MOROKUMA T., DOI M., YASUDA N., et al.
2008ApJ...676..163M 223           X C       5 14 20 The Subaru/XMM-Newton Deep Survey (SXDS). V. Optically faint variable object survey. MOROKUMA T., DOI M., YASUDA N., et al.
2008ApJS..176..301O viz 2 96 529 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. OUCHI M., SHIMASAKU K., AKIYAMA M., et al.
2010PASJ...62...91R viz 354       D     X   F     9 72 0 Proper motions with Subaru II. A sample in the Subaru/XMM-Newton Deep Survey Field. RICHMOND M.W., MOROKUMA T., DOI M., et al.
2012AJ....143...79Y 133       D     X         4 8 63 Panoramic survey of Lyα emitters at z = 3.1. YAMADA T., NAKAMURA Y., MATSUDA Y., et al.
2012ApJ...752..114S 81             C       2 13 132 The first systematic survey for Lyα emitters at z = 7.3 with red-sensitive Subaru/Suprime-Cam. SHIBUYA T., KASHIKAWA N., OTA K., et al.
2014PASJ...66...49O 712       D     X C       18 63 7 The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey. OKUMURA J.E., IHARA Y., DOI M., et al.
2016ApJ...823...20K 373       D     X C       9 12 92 Bright and faint ends of Lyα luminosity functions at z = 2 determined by the Subaru survey: implications for AGNs, magnification bias, and ISM H I evolution. KONNO A., OUCHI M., NAKAJIMA K., et al.
2017MNRAS.467.3951M 238           X C F     4 8 10 Imaging of diffuse H I absorption structure in the SSA22 protocluster region at z = 3.1. MAWATARI K., INOUE A.K., YAMADA T., et al.
2019PASJ...71...55K 285           X C       6 4 4 The dominant origin of diffuse Lyα halos around Lyα emitters explored by spectral energy distribution fitting and clustering analysis. KUSAKABE H., SHIMASAKU K., MOMOSE R., et al.
2021ApJ...919..120M 130           X         3 7 37 The evolution of the Lyman-alpha luminosity function during reionization. MORALES A.M., MASON C.A., BRUTON S., et al.
2023ApJ...958..187L 87           X         2 7 ~ A Spectroscopic Survey of Lyα Emitters and Lyα Luminosity Function at Redshifts 3.7 and 4.8. LIU W. and JIANG L.

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