First light of SINFONI at the VLT

By H. Bonnet, R. Abuter, A. Baker, W. Bornemann, Anthony G. A. Brown, R. Castillo, R. Conzelmann, Romuald Damster, Roger Davies, B. Delabre and 44 more. 2004

197 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/eda8bb60a7e9753a1bf0e4790ef4a611f58e3cd5

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Citations in the corpus

• A method to remove residual OH emission from near-infrared spectra (2007, methodology): “For example, the largest field of view of SINFONI (Eisenhauer et al. 2003a,b; Bonnet et al. 2004) at the VLT is 8 × 8 arcsec2; and at the finest pixel scale used with adaptive optics it is less than 1 arcsec.”
• From Rings to Bulges: Evidence for Rapid Secular Galaxy Evolution at z ~ 2 from Integral Field Spectroscopy in the SINS Survey (2008, methodology): “In this paper we present and analyze high-quality SINFONI/ VLT integral field ( IFU) spectroscopy (Eisenhauer et al. 2003; Bonnet et al. 2004) of eight representative UV/optically selected (BX/s-BzK) z 2 star forming galaxies.”
• The Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics, and Formation (2006, unknown): “The new adaptive optics assisted, near-infrared integral field spectrometer on the ESO-VLT, SPIFFI/SINFONI (Eisenhauer et al. 2003b; Bonnet et al. 2004) represents a key new capability for addressing the issues discussed above.”
• CONSTRAINTS ON THE ASSEMBLY AND DYNAMICS OF GALAXIES. I. DETAILED REST-FRAME OPTICAL MORPHOLOGIES ON KILOPARSEC SCALE OF z ∼ 2 STAR-FORMING GALAXIES (2010, methodology): “They were drawn from the initial sample of 17 rest-UV selected objects atz∼ 2 from the SINS survey (Förster Schreiber et al. 2006b, 2009) carried out with SINFONI (Eisenhauer et al. 2003; Bonnet et al. 2004) at the ESO VLT.”
• SINFONI in the Galactic Center: Young Stars and Infrared Flares in the Central Light-Month (2005, methodology): “The data were taken in 2004 July and August during the commissioning and first guaranteed time observations of SINFONI (Bonnet et al. 2004) at the Cassegrain focus of Very Large Telescope (VLT) Unit Telescope 4 (Yepun).”
• Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole (2018, methodology): “…measurements of the Brackett-γ line velocity were taken with the AO-assisted integral field spectrometer SINFONI at the VLT (Eisenhauer et al. 2003a; Bonnet et al. 2004), with five additional 2000-2003 slit-spectra from the AO imagers and spectrometers NIRC2 at Keck (see Ghez et al. 2003; Chu et…”
• THE SINS SURVEY OF z ∼ 2 GALAXY KINEMATICS: PROPERTIES OF THE GIANT STAR-FORMING CLUMPS (2010, methodology): “In this paper we present and analyze new high-quality SINFONI/VLT integral field (IFU) spectroscopy (Eisenhauer et al. 2003; Bonnet et al. 2004) of five luminous, clumpy z ∼ 2 SFGs.”
• MONITORING STELLAR ORBITS AROUND THE MASSIVE BLACK HOLE IN THE GALACTIC CENTER (2008, methodology): “Since July 2004 we regularly monitored the GC with the AO assisted field spectrometer SINFONI (Eisenhauer et al. 2003; Bonnet et al. 2004).”
• Integral field spectroscopy with SINFONI of VVDS galaxies I. Galaxy dynamics and mass assembly at 1.2 < z < 1.6 (2009, background): “The latter are necessary to engage into log single objects integrations with SINFONI (Eisenhauer et al. 2003; Bonnet et al. 2004) being sure to observe the Hα line outside bright OH night-sky emission lines.”
• Stellar and wind properties of massive stars in the central parsec of the Galaxy (2006, methodology): “The observations analysed here were conducted with the integral field spectrograph SPIFFI/SINFONI on the ESO/VLT Yepun 8 m telescope (Eisenhauer et al. 2003a,b; Bonnet et al. 2004) as part of the MPE-Garching GTO program “Galactic Center”.”
• CONSTRAINTS ON THE ASSEMBLY AND DYNAMICS OF GALAXIES. II. PROPERTIES OF KILOPARSEC-SCALE CLUMPS IN REST-FRAME OPTICAL EMISSION OF z ∼ 2 STAR-FORMING GALAXIES (2011, methodology): “The targets were drawn from the initial sample of 17 rest-UV selected objects atz ∼ 2 from the SINS survey (Förster Schreiber et al. 2006, 2009) carried out with the near-IR integral field spectrometer SINFONI (Eisenhauer et al. 2003; Bonnet et al. 2004) at the ESO VLT.”
• The Star-forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC 3227 (2006, methodology): “The data presented here were obtained on 21 Dec 2004 using SINFONI (Eisenhauer et al. 2003a; Bonnet et al. 2004) on the VLT UT4.”
• SINFONI Integral Field Spectroscopy of z ~ 2 UV-selected Galaxies: Rotation Curves and Dynamical Evolution (2006, methodology): “We collected the data with SINFONI (Eisenhauer et al. 2003a; Bonnet et al. 2004; Gillessen et al. 2005), mounted at the Cassegrain focus of theVLTUT4 telescope during several observing campaigns between 2004 July and 2005 October, as part of commissioning and guaranteed time observations.”
• A Close Look at Star Formation around Active Galactic Nuclei (2007, methodology): “Data for NGC 7469, NGC 2992, NGC 1097, NGC 1068, and NGC 3783 were taken during 2004Y2005 at the VLT with SINFONI, an AO near-infrared integral field spectrograph (Eisenhauer et al. 2003; Bonnet et al. 2004).”
• LSD: Lyman-break galaxies Stellar populations and Dynamics – I. Mass, metallicity and gas at z∼ 3.1 (2009, methodology): “The targets were observed at ESO/VLT by using the SINFONI instrument (Eisenhauer et al. 2003; Bonnet et al. 2004), an IFU spectrograph fed by an adaptive optics module with a natural guide star (NGS).”
• Evidence for powerful AGN winds at high redshift: dynamics of galactic outflows in radio galaxies during the “Quasar Era” (2008, methodology): “Our SINFONI data illustrate that this is indeed the case.”
• OUTFLOWS FROM ACTIVE GALACTIC NUCLEI: KINEMATICS OF THE NARROW-LINE AND CORONAL-LINE REGIONS IN SEYFERT GALAXIES, (2011, background): “Details about the SINFONI instrument can be found in Eisenhauer et al. (2003) and Bonnet et al. (2004), and a more complete discussion on the integral-field spectrometer OSIRIS can be found in Larkin et al. (2006).”
• The most massive stars in the Arches cluster (2007, methodology): “The Arches cluster was observed in service mode between May 3rd and June 27th 2005 with SINFONI on the ESO/VLT (Eisenhauer et al. 2003; Bonnet et al. 2004).”