OSIRIS: a diffraction limited integral field spectrograph for Keck
By J. Larkin, M. Barczys, A. Krabbe, S. Adkins, T. Aliado, P. Amico, G. Brims, R. Campbell, John M. Canfield, T. Gasaway and 16 more. SPIE Astronomical Telescopes + Instrumentation, 2006
261 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/ee6eda95f94c469761edb3116393466b0a04a02e
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Citations in the corpus
- HIGH ANGULAR RESOLUTION INTEGRAL-FIELD SPECTROSCOPY OF THE GALAXY'S NUCLEAR CLUSTER: A MISSING STELLAR CUSP? (2009, methodology): “Near-IR spectra of the central 4′′ of the Galaxy were obtained between 2006 and 2008 using the OSIRIS integral field spectrograph (Larkin et al. 2006) in conjunction with the laser guide star adaptive optics (LGS AO) system on the Keck II telescope (Wizinowich et al. 2006; van Dam et al. 2006).”
- SIMULTANEOUS DETECTION OF WATER, METHANE, AND CARBON MONOXIDE IN THE ATMOSPHERE OF EXOPLANET HR 8799 b (2015, methodology): “HR8799 b was observed in 2013 on July 25, 26 and 27 (UT) with the OSIRIS instrument (Larkin et al. 2006) in the K band using an identical instrument configuration as previous work by this group (Barman et al. 2011a, hereafter B11) resulting in 5.2 hrs of on-target integration time under good…”
- AN IMPROVED DISTANCE AND MASS ESTIMATE FOR SGR A* FROM A MULTISTAR ORBIT ANALYSIS (2016, methodology): “New spectroscopic observations for S0-38 were obtained using the integral field spectrograph OSIRIS with the laser guide star AO system on the Keck 1 telescope (Larkin et al. 2006) on 2013 May 11-13.”
- 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).”
- CLOUDS AND CHEMISTRY IN THE ATMOSPHERE OF EXTRASOLAR PLANET HR8799b (2011, methodology): “Natural guide star adaptive optics and the OH-Suppressing Infra-Red Imaging Spectrograph (OSIRIS) instrument (Larkin et al. 2006) were used on the Keck II telescope.”
- DISCOVERY, PROGENITOR AND EARLY EVOLUTION OF A STRIPPED ENVELOPE SUPERNOVA iPTF13bvn (2013, methodology): “On Jun 20.276, we observed iPTF13bvn inH-band with OSIRIS (Larkin et al. 2006) and the Laser Guide Star Adaptive Optics (LGS-AO) system (Wizinowich et al. 2006) mounted on the 10m Keck I telescope.”
- Resolved spectroscopy of gravitationally lensed galaxies: recovering coherent velocity fields in subluminous z ~ 2-3 galaxies (2009, methodology): “Accordingly, we used the Keck II spectrograph, NIRSPEC, in seeing limited mode in a second campaign to ‘screen’ all promising targets in advance of undertaking the more demanding resolved studies with the LGSAO-fed integral field unit spectrograph OSIRIS.”
- THE LICK AGN MONITORING PROJECT: THE MBH–σ* RELATION FOR REVERBERATION-MAPPED ACTIVE GALAXIES (2010, methodology): “Imaging Spectrograph (OSIRIS; Larkin et al. 2006) at the Keck-II telescope, operated with the laser guide-star adaptive optics (LGS-AO) system (Wizinowich et al. 2006).”
- Measuring Distance and Properties of the Milky Way’s Central Supermassive Black Hole with Stellar Orbits (2008, methodology): “Since 2005OSIRIS, which is an integral field spectrograph with a 2 m spectral resolution of 3600 (Larkin et al. 2006) has been used.”
- NEAR-INFRARED SPECTROSCOPY OF THE EXTRASOLAR PLANET HR 8799 b (2010, methodology): “Our observations of HR 8799 b were carried out with the OH-Suppressing InfraRed Integral-field Spectrograph (OSIRIS; Larkin et al. 2006) with natural guide star AO at Keck II on 2009 July 21 UT.”