Commissioning and performances of the VLT-VIMOS

By O. Lefevre, M. Saisse, D. Mancini, S. Brau-Nogué, O. Caputi, L. Castinel, S. D’odorico, Bianca Garilli, M. Kissler-Patig, C. Lucuix and 6 more. SPIE Astronomical Telescopes + Instrumentation, 2003

255 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/47c21a60e7c8b7ad9e4d7cbd7389fee763995e92

How researchers see this paper

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In Astronomy and Astrophysics

1. M. Ouchi
2. K. Shimasaku
3. N. Kashikawa
4. S. Okamura
5. H. Furusawa
6. L. Hernquist
7. M. Iye
8. P. Hopkins

In Instrumentation

1. M. Ouchi
2. K. Shimasaku
3. N. Kashikawa
4. S. Okamura
5. H. Furusawa
6. M. Iye
7. M. Akiyama
8. S. Sánchez

Citations in the corpus

• 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, methodology): “Spectroscopic Data We carried out spectroscopic follow-up observations for our LAE candidates with Faint Object Camera and Spectrograph (FOCAS; Kashikawa et al. 2002) of Subaru and Visible MultiObject Spectrograph (VIMOS; LeFevre et al. 2003) of VLT.”
• PMAS: The Potsdam Multi‐Aperture Spectrophotometer. II. The Wide Integral Field Unit PPak (2005, background): “Additionally, a single PPak fiber with 5.7 arcsec2 on the sky, collects twice the amount of light at the 3.5m telescope, than a single spatial element of the VIMOS-IFU (LeFevre et al. 2003) at the 8.2m-VLT (see specific grasp in Table 1).”