SHARC II: a Caltech submillimeter observatory facility camera with 384 pixels

By C. Dowell, C. Allen, R. Babu, M. Freund, M. Gardner, J. Groseth, M. Jhabvala, A. Kovács, D. Lis, S. Moseley and 4 more. SPIE Astronomical Telescopes + Instrumentation, 2003

137 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Civil and Structural Engineering

View Paper: https://www.semanticscholar.org/paper/6e7a81faa112b06d7cde5cf8bfeaa314fcdda075

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In Aerospace Engineering

1. N. Evans II
2. L. Allen

In Astronomy and Astrophysics

1. N. Evans II
2. C. Carilli
3. R. Ivison
4. I. Smail
5. S. Chapman
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Citations in the corpus

• Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective (2005, methodology): “The Submillimeter High Angular Resolution Camera (SHARC-II: Dowell et al. 2003) on the 10m Caltech Submillimeter Observatory (CSO) telescope was also used to image 39 YSOs in the 350 µm continuum between 2004 March and 2005 January.”
• Terahertz detectors and focal plane arrays (2011, unknown): “49(a) [186].”
• YOUNG STELLAR OBJECTS IN THE GOULD BELT (2015, methodology): “22 Available at http://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-scan?mission=irsa 23 Available at http://irsa.ipac.caltech.edu/data/SPITZER/docs/ mips/mipsinstrumenthandbook/ 24 The Submillimeter High Angular Resolution Camera II (SHARC-II) was a 350 µm bolometer array operated at the Caltech Submill”
• Lumped Element Kinetic Inductance Detectors (2008, methodology): “Ground based astronomy has been demonstrated in FIR bands at 350 μm using the SHARC II instrument on the CSO [7] and at 200 μm using Thumper on the JCMT [8].”
• 350 μm Dust Emission from High-Redshift Quasars (2006, methodology): “…of the Caltech Submillimeter Observatory (CSO) on the summit of Mauna Kea, Hawaii, during excellent weather conditions, with stable zenith atmospheric opacities of 1.0 at 350 m.We used the CSO bolometer camera, SHARC II, described by Dowell et al. (2003), mounted at the reimaged Cassegrain focus.”
• SHARC-2 350 μm Observations of Distant Submillimeter-selected Galaxies (2006, methodology): “Here we present results at 350 m, using the second-generation Submillimeter High Angular Resolution Camera (SHARC-2; Dowell et al. 2003) at the Caltech Submillimeter Observatory (CSO).”
• Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting Observed SEDs Using a Large Grid of Precomputed Models (2006, methodology): “As for MIPS, we have Fν0 [quoted] = ∫ Fν [actual] Rν(ν) dν ∫ (ν/ν0) 2 Rν(ν) dν (A11) The values of Rν(ν) are taken from Dowell et al. (2003) for the SHARC II observations, and the SCUBA website10 for the SCUBA 450WB and 850WB observations.”
• A Submillimeter View of Circumstellar Dust Disks in ρ Ophiuchi (2007, methodology): “Images of the 350 m continuum for seven YSOs were obtainedwith the SubmillimeterHighAngular Resolution Camera II (SHARC II; Dowell et al. 2003) on the 10 m Caltech Submillimeter Observatory (CSO) telescope in 2004 March and June.”