The Gemini Near‐Infrared Imager (NIRI)

By K. Hodapp, J. Jensen, Everett M. Irwin, H. Yamada, Randolph Chung, Kent Fletcher, L. Robertson, J. Hora, D. Simons, Wendy Mays and 4 more. Astronomical Telescopes and Instrumentation, 2000

270 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/8fc0d95c2cc608b90870c28c3c872a06182b6eac

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1. M. Marley
2. B. Bowler
3. E. Berger
4. Michael C. Liu
5. Jon Fortney
6. Bing Zhang
7. D. Saumon
8. A. Filippenko

Citations in the corpus

• THE 0.8–14.5 μm SPECTRA OF MID-L TO MID-T DWARFS: DIAGNOSTICS OF EFFECTIVE TEMPERATURE, GRAIN SEDIMENTATION, GAS TRANSPORT, AND SURFACE GRAVITY (2009, methodology): “We also obtained new 3.0–4.1 µm spectra for five targets using the Near InfraRed Imager and Spectrograph (NIRI; Hodapp et al. 2003) at Gemini North Observatory.”
• The Volume-limited A-Star (VAST) survey – I. Companions and the unexpected X-ray detection of B6–A7 stars (2011, methodology): “The data were acquired with several instruments listed in Table 3 – VisIm (Roberts & Neyman 2002) on AEOS, KIR (Doyon et al. 1998) on Canada–France–Hawaii Telescope (CFHT), NIRI (Hodapp et al. 2003) on Gemini-North and PHARO (Hayward et al. 2001) on Palomar.”
• FUNDAMENTAL PARAMETERS AND SPECTRAL ENERGY DISTRIBUTIONS OF YOUNG AND FIELD AGE OBJECTS WITH MASSES SPANNING THE STELLAR TO PLANETARY REGIME (2015, unknown): “…et al. (2006), (10)Wilson et al. (2004), (11) Mountain et al. (1990), (12) Depoy et al. (1993), (13) Eisenhauer et al. (2003), (14) Bonnet et al. (2004), (15) Matthews & Soifer (1994), (16) Kobayashi et al. (2000), (17) Hodapp et al. (2003), (18) Woodgate et al. (1998), (19) Houck et al. (2004).”
• The Gemini Deep Planet Survey (2007, methodology): “The last column of the table (“saturationradius”) indicates the separation at which the radial profile of the PSF reaches 75% of the detector full well capacity; linear- The Gemini Deep Planet Survey 9 ity should be better than 1% at this level (Hodapp et al. 2003).”
• A PHOTOMETRIC REDSHIFT OF z ∼ 9.4 FOR GRB 090429B (2011, methodology): “We gathered optical i ′z′ imaging with the Gemini Multi-Object Spectrograph (GMOS; Hook et al. 2004) and NIR JHK imaging with the NearInfared Imager (NIRI; Hodapp et al. 2003).”
• Direct Imaging and Spectroscopy of a Planetary-Mass Candidate Companion to a Young Solar Analog (2008, methodology): “1-210524 was done on 2008 April 27 in Ks using the NIRI camera (Hodapp et al. 2003) and the ALTAIR adaptive optics system (Herriot et al. 2000) at the Gemini North Telescope.”
• SPHERE: the exoplanet imager for the Very Large Telescope (2019, result): “…opticsequipped, near-infrared (NIR) instruments on large groundbased telescopes like the VLT/NaCo (Lenzen et al. 2003; Rousset et al. 2003) or Gemini/NIRI (Hodapp et al. 2003; Herriot et al. 1998) was greatly improved as compared to previous systems on smaller telescopes (e.g., Beuzit et al. 1997).”
• SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 < z < 1.12 AND THE UNION2 COMPILATION (2010, methodology): “The NIRI observations were done in queue mode and the data were taken on 4 separate nights, starting on 2001 May 25 and ending 2002 Aug 5.”
• NEGLECTED CLOUDS IN T AND Y DWARF ATMOSPHERES (2012, methodology): “65−225025.2, using the near-infrared imager NIRI (Hodapp et al. 2003) on the Gemini-North telescope on Mauna Kea, Hawaii.”
• Discovery of a Planetary-sized Object in the Scattered Kuiper Belt (2005, methodology): “Medium resolution near-infrared spectra were obtained on the nights of 25-27 January UT with the Near Infrared Imager and Spectrograph (NIRI, Hodapp et al. 2003) instrument on the Gemini North telescope.”
• Near-Infrared Spectroscopy of Charon: Possible Evidence for Cryovolcanism on Kuiper Belt Objects (2006, methodology): “H- and K-band spectra were obtained in 2005 using NIRI (Hodapp et al. 2003) and the Altair adaptive optics (AO) system.”
• SN 2008ha: AN EXTREMELY LOW LUMINOSITY AND EXCEPTIONALLY LOW ENERGY SUPERNOVA (2009, methodology): “We have followed SN 2008ha photometrically with the 0.76 m Katzman Automatic Imaging Telescope (KAIT; Filippenko et al. 2001), the 1 m Nickel 1 m, the 1.3 m Peters Automated Infrared Imaging Telescope (PAIRITEL), the 6.5 m Magellan Baade telescope (with PANIC; Martini et al. 2004), and the 8-m Gemin”
• The VAST Survey - III. The multiplicity of A-type stars within 75 pc (2013, methodology): “The wide band filter was not used for data obtained with PHARO KIR – Doyon et al. (1998) NIRI (Near InfraRed Imager and Spectrometer) – Hodapp et al.(2003) IRCAL (IR Camera for Adaptive Optics at Lick) – Lloyd et al. (2000) PHARO (Palomar High Angular Resolution Observer) – Haywardet al. (2001) alog”
• A POPULATION OF MASSIVE, LUMINOUS GALAXIES HOSTING HEAVILY DUST-OBSCURED GAMMA-RAY BURSTS: IMPLICATIONS FOR THE USE OF GRBs AS TRACERS OF COSMIC STAR FORMATION (2013, methodology): “Gemini/NIRI Deep imaging observations from the Near-Infrared Imager (NIRI; Hodapp et al. 2003) on Gemini-North were used to constrain the properties of host galaxies in the sample.”