NAOS-CONICA first on sky results in a variety of observing modes

By R. Lenzen, M. Hartung, W. Brandner, G. Finger, N. Hubin, F. Lacombe, Anne-Marie Lagrange, M. Lehnert, A. Moorwood, David Mouillet. SPIE Astronomical Telescopes + Instrumentation, 2003

261 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Atomic and Molecular Physics, and Optics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/6c41c08ac861fd7a4ac6c06c201273a312edd4de

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The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. R. Genzel
2. R. Somerville
3. Roger Davies
4. M. Bessell

In Atomic and Molecular Physics, and Optics

1. M. Meyer
2. B. Macintosh
3. Inseok Song
4. C. Marois
5. S. Desidera
6. Roger Davies
7. R. Doyon
8. R. Genzel

In Instrumentation

1. P. Hopkins
2. R. Somerville
3. L. Hernquist
4. Hans-Walter Rix
5. Christopher J. Conselice
6. Thomas J. Cox
7. S. Jogee
8. A. Dekel

Citations in the corpus

• A Close Look at Star Formation around Active Galactic Nuclei (2007, methodology): “Data for IRAS 05189 2524 and NGC 1068 were taken in 2002 December at the VLT with NACO, an AO near-infrared camera and long-slit spectrograph (Lenzen et al. 2003; Rousset c References to detailed studies of individual objects: Mrk 231 (Davies et al. 2004b), NGC7469 (Davies et al. 2004a), Circinus…”
• DISCOVERY OF A PROBABLE 4–5 JUPITER-MASS EXOPLANET TO HD 95086 BY DIRECT IMAGING (2013, methodology): “HD95086 was observed with VLT/NaCo (Lenzen et al. 2003, Rousset et al. 2003) in thermal infrared with angular differential imaging (ADI Marois et al. 2006) mode as part of our direct-imaging survey of young, dusty, and early-type stars (Rameau et al. 2013).”
• A YOUNG PROTOPLANET CANDIDATE EMBEDDED IN THE CIRCUMSTELLAR DISK OF HD 100546 (2013, methodology): “The VLT/NACO PDI data presented in Quanz et al. (2011b) have sufficient spatial resolution and inner working angle to probe the disk surface on scales relevant for the APP dataset.”
• A probable giant planet imaged in the beta Pictoris disk. VLT/NaCo deep L'-band imaging (2008, methodology): “…image quality provided by the Nasmyth Adaptive Optics System (NAOS; Rousset et al. 2003) at infrared wavelengths and the good dy- namics offered by the Near-Infrared Imager and Spectrograph (CONICA; Lenzen et al. 2003) detector, in order to study the immediate circumstellar environement ofβ Pic.”
• The VAST Survey - III. The multiplicity of A-type stars within 75 pc (2013, methodology): “In addition to the new observations presented within this study, VLT/NaCo (Lenzen et al. 2003; Rousset et al. 2003) and CFHT/KIR data taken in similar AO snapshot modes were obtained from the ESO and CFHT science archives.”
• GEMS: Galaxy Evolution from Morphologies and SEDs (2004, background): “To date HST is still far more efficient to deliver this over wide fields over wide fields than AO on large ground-based telescopes, such as afforded by CONICA on the VLT (Lenzen et al. 2003).”