activity
19982026
most citedPICO: Probe of Inflation and Cosmic Origins

72 citations · 202 across the 9 of their papers we have counts for

collaborators

11 papers

physics.ins-det2026

The Solar Neutrino and Astro-Particle PhYsics (SNAPPY) CubeSat Development

Brian M. Sutin, Edward Bierens, Brian Doty +14

The SNAPPY CubeSat, which was launched May 3, 2026, will demonstrate and space qualify the nuSol neutrino-detection technology. The nuSol technology detects solar neutrinos using a…

astro-ph.EP2023★ 1 cited

Radiometry for Nighttime Sub-Cloud Imaging of Venus' Surface in the Near-InfraRed Spectrum

Brian M. Sutin, Anthony B. Davis, Kevin H. Baines +2

Does radiometry (e.g., signal-to-noise ratio) limit the performance of near-IR subcloud imaging of our sister planet's surface at night? It does not. We compute subcloud radiometry…

astro-ph.IM2023★ 2 cited

Statistics of electron-multiplying charge-coupled devices

Brian M. Sutin

EMCCDs are efficient imaging devices for low surface brightness UV astronomy from space. The large amplification allows photon counting, the detection of events versus non-events.…

astro-ph.EP2023

Determining the Shape, Size, and Sources of the Zodiacal Dust Cloud using Polarized Ultraviolet Scattered Sunlight

Geoffrey Bryden, Neal J. Turner, Petr Pokorny +7

The solar system's Zodiacal Cloud is visible to the unaided eye, yet the origin of its constituent dust particles is not well understood, with a wide range of proposed divisions be…

astro-ph.IM2019★ 72 cited

PICO: Probe of Inflation and Cosmic Origins

S. Hanany, M. Alvarez, E. Artis +79

The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. W…

astro-ph.IM2019★ 45 cited

PICO: Probe of Inflation and Cosmic Origins

Shaul Hanany, Marcelo Alvarez, Emmanuel Artis +79

The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce f…

astro-ph.IM2018

Optical Design of PICO, a Concept for a Space Mission to Probe Inflation and Cosmic Origins

Karl Young, Marcelo Alvarez, Nicholas Battaglia +28

The Probe of Inflation and Cosmic Origins (PICO) is a probe-class mission concept currently under study by NASA. PICO will probe the physics of the Big Bang and the energy scale of…

astro-ph.IM2018

PICO - the probe of inflation and cosmic origins

Brian Sutin, Marcelo Alvarez, Nicholas Battaglia +31

The Probe of Inflation and Cosmic Origins (PICO) is a NASA-funded study of a Probe-class mission concept. The top-level science objectives are to probe the physics of the Big Bang…

math.NA2008★ 1 cited

Accurate Evaluation of Polynomials

Brian M. Sutin

For a large class of polynomials, the standard method of polynomial evaluation, Horner's method, can be very inaccurate. The alternative method given here is on average 100 to 1000…

astro-ph2000★ 47 cited

Performance characteristics of the new Keck Observatory echelle spectrograph and imager

A. I. Sheinis, J. Miller, M. Bolte +1

The Echelle Spectrograph and Imager (ESI) is a multipurpose instrument which has been delivered by the Instrument Development Laboratory of Lick Observatory for use at the Cassegra…

astro-ph1998★ 34 cited

An IR Search for Extinguished Supernovae in Starburst Galaxies

Bruce Grossan, Earl Spillar, Robert Tripp +3

IR and Radio band observations of heavily extinguished regions in starburst galaxies suggest a very high SN rate associated with such regions. Optically measured supernova (SN) rat…