A Wide-Field Infrared Camera for the Palomar 200-inch Telescope

By John C. Wilson, S. Eikenberry, C. Henderson, T. Hayward, J. Carson, B. Pirger, D. Barry, B. Brandl, J. Houck, G. Fitzgerald and 1 more. SPIE Astronomical Telescopes + Instrumentation, 2003

154 citations recorded by the source corpus.

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

View Paper: https://www.semanticscholar.org/paper/8d6f205d88e3552f2165d58b03f775f3cfe73c1b

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Citations in the corpus

Ultraviolet to Mid-Infrared Observations of Star-forming Galaxies at z ~ 2: Stellar Masses and Stellar Populations (2005, methodology): “Near-IR Imaging We observed the HS1700+64 field during two observing runs, 2003 May and 2003 October, using the Palomar 5.1m Hale telescope and the Wide Field Infrared Camera (WIRC; Wilson et al. 2003).”
The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs (2020, background): “…the 1.3 m Peters Automated Infrared Imaging Telescope (PAIRITEL; Bloom et al. 2006) on Mt. Hopkins, Arizona; the Wide-field Infrared Camera (WIRC; Wilson et al. 2003b) at the 5 m Hale Telescope at Palomar Mountain, California; and the Ohio State Infrared Imager/Spectrometer (OSIRIS) at the 4.1…”
A Spectroscopic Survey of Redshift 1.4 ≲ z ≲ 3.0 Galaxies in the GOODS-North Field: Survey Description, Catalogs, and Properties (2006, methodology): “We have obtained very deep wide-area near-IR imaging at J andKs band in the GOODS-N field from observations with the Wide Field Infrared Camera (WIRC; Wilson et al. 2003) on the PalomarHale 5m telescope.”
The Mass Assembly Histories of Galaxies of Various Morphologies in the GOODS Fields (2005, methodology): “′6 on a side, using the Wide-field Infrared Camera (WIRC, Wilson et al. 2003) on the Hale 5m telescope at Palomar Observatory.”
A Census of Optical and Near-Infrared Selected Star-forming and Passively Evolving Galaxies at Redshift z ~ 2 (2005, methodology): “The Ks and J imaging was accomplished with the Wide Field Infrared Camera (WIRC) on the Palomar Hale 5 m telescope (Wilson et al. 2003), providing 8.”
PHYSICAL CONDITIONS IN A YOUNG, UNREDDENED, LOW-METALLICITY GALAXY AT HIGH REDSHIFT (2010, methodology): “Near-IR J and K band observations were conducted with the Wide-Field Infrared Camera (WIRC, Wilson et al. 2003), also on the Palomar telescope.”
A Wide-Field Survey of Two z ~ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s (2007, methodology): “Ground based data include panoramic Ks-band imaging of both clusters, along withJ-band imaging of Cl 0024, obtained with the WIRC camera on the Hale 200” telescope at Palomar Observatory (Wilson et al. 2003).”
Chandra and Spitzer Unveil Heavily Obscured Quasars in the Chandra/SWIRE Survey (2006, methodology): “Near-IR Ks imaging observations were carried out with the 20000 Hale Telescope of the Palomar Observatory using theWide Infrared Camera (WIRC; Wilson et al. 2003) on 2004 March 29 under photometric conditions.”
The Mass-Metallicity Relation at z≳2 (2006, methodology): “The near-IR imaging was carried out with the Widefield IR Camera (WIRC, Wilson et al. 2003) on the Palomar 5-m Hale telescope.”