Extremely Large Telescope

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NIR Spectroscopy of Star-Forming Galaxies at z~1.4 with Subaru/FMOS: The Mass-Metallicity Relation

(2011)

Authors:

Kiyoto Yabe, Kouji Ohta, Fumihide Iwamuro, Suraphong Yuma, Masayuki Akiyama, Naoyuki Tamura, Masahiko Kimura, Naruhisa Takato, Yuuki Moritani, Masanao Sumiyoshi, Toshinori Maihara, John Silverman, Gavin Dalton, Ian Lewis, David Bonfield, Hanshin Lee, Emma Curtis Lake, Edward Macaulay, Fraser Clarke
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The Atlas3D Project -- XI. Dense molecular gas properties of CO-luminous early-type galaxies

(2011)

Authors:

Alison Crocker, Melanie Krips, Martin Bureau, Lisa M Young, Timothy A Davis, Estelle Bayet, Katherine Alatalo, Leo Blitz, Maxime Bois, Frédéric Bournaud, Michele Cappellari, Roger L Davies, PT de Zeeuw, Pierre-Alain Duc, Eric Emsellem, Sadegh Khochfar, Davor Krajnovic, Harald Kuntschner, Pierre-Yves Lablanche, Rchard M McDermid, Raffaella Morganti, Thorsten Naab, Tom Oosterloo, Marc Sarzi, Nicholas Scott, Paolo Serra, Anne-Marie Weijmans
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THE zCOSMOS–SINFONI PROJECT. I. SAMPLE SELECTION AND NATURAL-SEEING OBSERVATIONS**Based on observations obtained at the Very Large Telescope (VLT) of the European Southern Observatory, Paranal, Chile (ESO Program IDs 079.A-0341, 081.A-0672, and 183.A-0781). Also based on observations with the NASA/ESA Hubble Space Telescope (HST), obtained at the Space Telescope Science Institute, and with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology.

The Astrophysical Journal American Astronomical Society 743:1 (2011) 86

Authors:

C Mancini, NM Förster Schreiber, A Renzini, G Cresci, EKS Hicks, Y Peng, D Vergani, S Lilly, M Carollo, L Pozzetti, G Zamorani, E Daddi, R Genzel, C Maraston, HJ McCracken, L Tacconi, N Bouché, R Davies, P Oesch, K Shapiro, V Mainieri, D Lutz, M Mignoli, A Sternberg
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Astrophysics: Monster black holes.

Nature 480:7376 (2011) 187-188
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A project for an infrared synoptic survey from Antarctica with the Polar Large Telescope (PLT)

SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics (2011)

Authors:

N Epchtein, L Abe, W Ansorge, M Langlois, I Vauglin, S Argentini, I Esau, C David, I Bryson, GB Dalton, M Ashley, J Lawrence

Abstract:

The Polar Large Telescope (PLT) aims at performing a new generation of astronomical Infrared Synoptic Survey from Antarctica (ISSA). It would carry out for the first time large scale periodic imaging surveys at ˜ 0.3 arcsec angular resolution in the short thermal infrared (2-5 micron) range benefiting from the extremely dry, cold, and stable polar atmosphere. The PLT consists of a 2.5 m class telescope equipped with a 250-Mpixel infrared camera. The survey would produce diffraction limited images at 2 micron covering a total of ˜ 5000 square degrees, explore the time domain from seconds to years down to mab =25.5 in Kd, generate alerts of transients and react quickly to alerts from other ground based or space borne facilities.