Jenna Moore
A5035350814- Radio Astronomy Observations and Technology
- Superconducting and THz Device Technology
- Cosmology and Gravitation Theories
- Scientific Research and Discoveries
- Galaxies: Formation, Evolution, Phenomena
- Geophysics and Gravity Measurements
- Astrophysics and Cosmic Phenomena
- Spacecraft and Cryogenic Technologies
- Cryospheric studies and observations
- Astrophysics and Star Formation Studies
- Astronomy and Astrophysical Research
- Advanced Frequency and Time Standards
- Radio, Podcasts, and Digital Media
- Physics of Superconductivity and Magnetism
- Pulsars and Gravitational Waves Research
Arizona State University
2019-2023
University of California, San Diego
2020
California University of Pennsylvania
2020
Abstract The Simons Observatory (SO) is a cosmic microwave background survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5200 m in the Atacama Desert Chile. SO SATs will cover six spectral bands between 27 and 280 GHz to search for primordial B-modes sensitivity σ ( r ) = 0.002, with quantified systematic errors well below this value. Each SAT self-contained cryogenic telescope 35° field view, 42 cm diameter optical aperture, 40 K half-wave plate,...
Abstract The Simons Observatory will map the temperature and polarization over half of sky at millimeter wavelengths in six spectral bands from Atacama Desert Chile. These data provide new insights into genesis, content, history our Universe, astrophysics galaxies galaxy clusters, objects solar system, time-varying astrophysical phenomena. This ambitious instrument suite, initially comprising three 0.5 m diameter small aperture telescopes one 6 large telescope, is designed using a common...
The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) survey experiment that currently consists of three 0.42m small-aperture telescopes (SATs) and one 6m large-aperture telescope (LAT), located at an elevation 5200m in the Atacama Desert Chile. At LAT's focal plane, SO will install >62,000 transition-edge sensor detectors across 13 optics tubes (OTs) within Large Aperture Telescope Receiver (LATR), largest cryogenic camera ever built to observe CMB. Here we report...
Abstract We use public data from the South Pole Telescope (SPT) and Atacama Cosmology (ACT) to measure radial profiles of thermal Sunyaev–Zel’dovich (tSZ) effect dust emission around massive quiescent galaxies at z ≈ 1. Using survey Dark Energy Survey Wide-Field Infrared Explorer, we selected 387,627 within ACT field, with a mean stellar <?CDATA ${\mathrm{log}}_{10}({M}_{\star }/{M}_{\odot })$?> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msub> <mml:mrow>...
The Simons Observatory (SO) will observe the cosmic microwave background (CMB) from Cerro Toco in Atacama Desert of Chile. observatory consists three 0.5m Small Aperture Telescopes (SATs) and one 6m Large Telescope (LAT), covering six frequency bands centering around 30, 40, 90, 150, 230, 280 GHz. SO observations transform our understanding universe by characterizing properties early universe, measuring number relativistic species mass neutrinos, improving galaxy evolution, constraining...
Abstract The Simons Observatory is a ground-based cosmic microwave background experiment that consists of three 0.4 m small-aperture telescopes and one 6 Large Aperture Telescope, located at an elevation 5300 on Cerro Toco in Chile. Telescope Receiver (LATR) the cryogenic camera will be coupled to Telescope. resulting instrument produce arcminute-resolution millimeter-wave maps half sky with unprecedented precision. LATR largest built date, diameter 2.4 length 2.6 m. coldest stage cooled 100...
The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment located in the Atacama Desert Chile at an elevation of 5200 meters, nominally consisting array three 0.42-meter small aperture telescopes (SATs) and one 6-meter large telescope (LAT). SO will make accurate measurements CMB temperature polarization spanning six frequency bands ranging from 27 to 280 GHz, fielding total $\sim$68,000 detectors covering angular scales between arcminute tens degrees. In this...
The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) survey experiment that consists of three 0.5 m small-aperture telescopes and one 6 large-aperture telescope, sited at an elevation 5200 in the Atacama Desert Chile. SO will utilize more than 60,000 transition edge sensors (TES) to observe CMB temperature polarization six frequency bands from 27-280 GHz. Common both small large aperture telescope receivers (LATR) 300K-4K Universal Readout Harness (URH), which...
We use public data from the South Pole Telescope (SPT) and Atacama Cosmology (ACT) to measure radial profiles of thermal Sunyaev-Zel'dovich (tSZ) effect dust emission around massive quiescent galaxies at $z\approx1.$ Using survey Dark Energy Survey (DES) Wide-Field infrared Explorer (WISE), we selected $387,627$ within ACT field, with a mean stellar $\log_{10}(M_{\star}/\rm{M_{\odot}})$ $11.40$. A subset $94,452$ galaxies, $11.36,$ are also covered by SPT. In $0.5$ arcminute bins these...