activity
20152021
most citedThe upGREAT 1.9 THz multi-pixel high resolution spectrometer for the SOFIA Observatory

113 citations · 544 across the 13 of their papers we have counts for

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12 papers · 1 filter

astro-ph.IM2021★ 3 cited

Holographic surface measurement system for the Fred Young Submillimeter Telescope

Xiaodong Ren, Pablo Astudillo, Urs U. Graf +6

We describe a system being developed for measuring the shapes of the mirrors of the Fred Young Submillimeter Telescope (FYST), now under construction for the CCAT Observatory. "Hol…

astro-ph.IM2020★ 15 cited

4GREAT -- a four-color receiver for high-resolution airborne terahertz spectroscopy

Carlos A. Durán, Rolf Güsten, Christophe Risacher +13

4GREAT is an extension of the German Receiver for Astronomy at Terahertz frequencies (GREAT) operated aboard the Stratospheric Observatory for Infrared Astronomy (SOFIA). The spect…

astro-ph.IM2020★ 53 cited

The large scale polarization explorer (LSPE) for CMB measurements: performance forecast

The LSPE collaboration, G. Addamo, P. A. R. Ade +102

[Abridged] The measurement of the polarization of the Cosmic Microwave Background radiation is one of the current frontiers in cosmology. In particular, the detection of the primor…

astro-ph.IM2020★ 21 cited

Progress report on the Large Scale Polarization Explorer

L. Lamagna, G. Addamo, P. A. R. Ade +96

The Large Scale Polarization Explorer (LSPE) is a cosmology program for the measurement of large scale curl-like features (B-modes) in the polarization of the Cosmic Microwave Back…

astro-ph.IM2019★ 43 cited

Wideband 67-116 GHz receiver development for ALMA Band 2

P. Yagoubov, T. Mroczkowski, V. Belitsky +43

ALMA has been operating since 2011, but has not yet been populated with the full suite of intended frequency bands. In particular, ALMA Band 2 (67-90 GHz) is the final band in the…

astro-ph.IM2018★ 109 cited

The upGREAT dual frequency heterodyne arrays for SOFIA

C. Risacher, R. Güsten, J. Stutzk +30

We present the performance of the upGREAT heterodyne array receivers on the SOFIA telescope after several years of operations. This instrument is a multi-pixel high resolution (R >…

astro-ph.IM2018★ 7 cited

The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds

C. Franceschet, S. Realini, A. Mennella +48

In this paper we discuss the latest developments of the STRIP instrument of the "Large Scale Polarization Explorer" (LSPE) experiment. LSPE is a novel project that combines ground-…

astro-ph.IM2018★ 1 cited

Wideband 67-116 GHz cryogenic receiver development for ALMA Band 2

P. Yagoubov, T. Mroczkowski, L. Testi +25

The Atacama Large Millimeter/sub-millimeter Array (ALMA) is already revolutionising our understanding of the Universe. However, ALMA is not yet equipped with all of its originally…

astro-ph.IM2018★ 28 cited

A Calibrated Digital Sideband Separating Spectrometer for Radio Astronomy Applications

Ricardo Finger, Patricio Mena, Nicolas Reyes +2

Dual sideband (2SB) receivers are well suited for the spectral observation of complex astronomical signals over a wide frequency range. They are extensively used in radio astronomy…

astro-ph.IM2016★ 8 cited

The Atacama Large Millimeter/submillimeter Array (ALMA) Band-1 Receiver

Yau De Huang, Oscar Morata, Patrick Michel Koch +29

The Atacama Large Millimeter/submillimeter Array(ALMA) Band 1 receiver covers the 35-50 GHz frequency band. Development of prototype receivers, including the key components and sub…

astro-ph.IM2016★ 113 cited

The upGREAT 1.9 THz multi-pixel high resolution spectrometer for the SOFIA Observatory

C. Risacher, R. Guesten, J. Stutzki +19

We present a new multi-pixel high resolution (R >10^7) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receiver uses 2 x 7-pixel subarrays in…

astro-ph.IM2015★ 81 cited

First supra-THz Heterodyne Array Receivers for Astronomy with the SOFIA Observatory

Christophe Risacher, Rolf Guesten, Juergen Stutzki +15

We present the upGREAT THz heterodyne arrays for far-infrared astronomy. The Low Frequency Array (LFA) is designed to cover the 1.9-2.5 THz range using 2x7-pixel waveguide-based HE…