papers

Publications (38)

astro-ph.CO2017

Exploring cosmic origins with CORE: gravitational lensing of the CMB

Anthony Challinor, Rupert Allison, Julien Carron +110

Lensing of the CMB is now a well-developed probe of large-scale clustering over a broad range of redshifts. By exploiting the non-Gaussian imprints of lensing in the polarization o…

astro-ph.IM2016

A cryogenic rotation stage with a large clear aperture for the half-wave plates in the Spider instrument

Sean Bryan, Peter Ade, Mandana Amiri +47

We describe the cryogenic half-wave plate rotation mechanisms built for and used in Spider, a polarization-sensitive balloon-borne telescope array that observed the Cosmic Microwav…

astro-ph.IM2017

Photon noise from chaotic and coherent millimeter-wave sources measured with horn-coupled, aluminum lumped-element kinetic inductance detectors

Daniel Flanigan, Heather McCarrick, Glenn Jones +18

We report photon-noise limited performance of horn-coupled, aluminum lumped-element kinetic inductance detectors at millimeter wavelengths. The detectors are illuminated by a milli…

astro-ph.CO2010

EBEX: A balloon-borne CMB polarization experiment

Britt Reichborn-Kjennerud, Asad M. Aboobaker, Peter Ade +43

EBEX is a NASA-funded balloon-borne experiment designed to measure the polarization of the cosmic microwave background (CMB). Observations will be made using 1432 transition edge s…

astro-ph.IM2019

QUBIC: Exploring the primordial Universe with the Q\&U Bolometric Interferometer

Aniello Mennella, Peter Ade, Giorgio Amico +127

In this paper we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the art bolometric de…

astro-ph.IM2011

A New Artificial Dielectric Metamaterial and its Application as a THz Anti-Reflection Coating

Jin Zhang, Peter Ade, Philip Mauskopf +3

We describe a novel artificial dielectric material which has applications at millimetre and submillimetre wavelengths. The material is manufactured from layers of metal mesh patter…

astro-ph.IM2018

BFORE: A CMB Balloon Payload to Measure Reionization, Neutrino Mass, and Cosmic Inflation

Sean Bryan, Peter Ade, J. Richard Bond +21

BFORE is a high-altitude ultra-long-duration balloon mission to map the cosmic microwave background (CMB). During a 28-day mid-latitude flight launched from Wanaka, New Zealand, th…

astro-ph.CO2010

BLAST Observations of the South Ecliptic Pole field: Number Counts and Source Catalogs

Elisabetta Valiante, Peter Ade, James Bock +26

We present results from a survey carried out by the Balloon-borne Large Aperture Submillimeter Telescope (BLAST) on a 9 deg^2 field near the South Ecliptic Pole at 250, 350 and 500…

physics.ins-det2004

Modeling the electromagnetic properties of the SCUBA-2 detectors

Michael Audley, Giampaolo Pisano, Wayne Holland +3

SCUBA-2 is the next-generation replacement for SCUBA (Sub-millimetre Common User Bolometer Array) on the James Clerk Maxwell Telescope. Operating at 450 and 850 microns, SCUBA-2 fi…

astro-ph.IM2017

Measuring Reionization, Neutrino Mass, and Cosmic Inflation with BFORE

Sean Bryan, Peter Ade, J. Richard Bond +21

BFORE is a NASA high-altitude ultra-long-duration balloon mission proposed to measure the cosmic microwave background (CMB) across half the sky during a 28-day mid-latitude flight…

astro-ph.IM2013

A Dual-polarized Broadband Planar Antenna and Channelizing Filter Bank for Millimeter Wavelengths

Roger OBrient, Peter Ade, Kam Arnold +9

We describe the design, fabrication, and testing of a broadband log-periodic antenna coupled to multiple cryogenic bolometers. This detector architecture, optimized here for astrop…

astro-ph.IM2016

Instrumental performance and results from testing of the BLAST-TNG receiver, submillimeter optics, and MKID arrays

Nicholas Galitzki, Peter Ade, Francesco E. Angile +39

Polarized thermal emission from interstellar dust grains can be used to map magnetic fields in star forming molecular clouds and the diffuse interstellar medium (ISM). The Balloon-…

astro-ph.IM2011

Polypropylene Embedded Metal-Mesh Broadband Achromatic Half Wave Plate for Millimeter Wavelengths

Jin Zhang, Peter Ade, Philip Mauskopf +3

We describe a novel multi-layered metal mesh achromatic half wave plate for use in astronomical polarimetric instruments. The half wave plate is designed to operate across the freq…

astro-ph.IM2018

Optical Characterization of the SPT-3G Focal Plane

Zhaodi Pan, Peter Ade, Zeeshan Ahmed +73

The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-e…

astro-ph2006

SCUBA-2: a 10,000 pixel submillimeter camera for the James Clerk Maxwell Telescope

Wayne Holland, Michael MacIntosh, Alasdair Fairley +30

SCUBA-2 is an innovative 10,000 pixel submillimeter camera due to be delivered to the James Clerk Maxwell Telescope in late 2006. The camera is expected to revolutionize submillime…

astro-ph.IM2021

Overview and status of EXCLAIM, the experiment for cryogenic large-aperture intensity mapping

Giuseppe Cataldo, Peter Ade, Christopher Anderson +41

The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a balloon-borne far-infrared telescope that will survey star formation history over cosmological time sca…

astro-ph.IM2013

Empirical modelling of the BLASTPol achromatic half-wave plate for precision submillimetre polarimetry

Lorenzo Moncelsi, Peter Ade, Francesco Elio Angile +18

A cryogenic achromatic half-wave plate (HWP) for submillimetre astronomical polarimetry has been designed, manufactured, tested, and deployed in the Balloon-borne Large-Aperture Su…

astro-ph.IM2010

Software systems for operation, control, and monitoring of the EBEX instrument

Michael Milligan, Peter Ade, François Aubin +35

We present the hardware and software systems implementing autonomous operation, distributed real-time monitoring, and control for the EBEX instrument. EBEX is a NASA-funded balloon…

astro-ph.IM2018

The EBEX Balloon Borne Experiment - Detectors and Readout

The EBEX Collaboration, Maximilian Abitbol, Asad M. Aboobaker +37

EBEX was a long-duration balloon-borne experiment to measure the polarization of the cosmic microwave background. The experiment had three frequency bands centered at 150, 250, and…

astro-ph.IM2022

CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths

Alessandro Fasano, Alexandre Beelen, Alain Benoit +37

CarbON CII line in post-rEionization and ReionizaTiOn (CONCERTO) is a low-resolution spectrometer with an instantaneous field-of-view of 18.6 arcmin, operating in the 130-310 GHz t…

astro-ph.IM2010

Absolute polarization angle calibration using polarized diffuse Galactic emission observed by BICEP

Tomotake Matsumura, Peter Ade, Denis Barkats +25

We present a method of cross-calibrating the polarization angle of a polarimeter using BICEP Galactic observations. \bicep\ was a ground based experiment using an array of 49 pairs…

astro-ph.IM2023

CONCERTO: instrument and status

Alessandro Fasano, Peter Ade, Manuel Aravena +36

CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of…

astro-ph.IM2024

CONCERTO: Instrument model of Fourier transform spectroscopy, white-noise components

Alessandro Fasano, Peter Ade, Manuel Aravena +34

Modern astrophysics relies on intricate instrument setups to meet the demands of sensitivity, sky coverage, and multi-channel observations. An example is the CONCERTO project, empl…

astro-ph2004

An update on the SCUBA-2 project

Michael Audley, Wayne Holland, Trevor Hodson +16

SCUBA-2, which replaces SCUBA (the Submillimeter Common User Bolometer Array) on the James Clerk Maxwell Telescope (JCMT) in 2006, is a large-format bolometer array for submillimet…

astro-ph.GA2013

Cold Dust in Hot Regions

Gopika Sreenilayam, Michel Fich, Peter Ade +12

We mapped five massive star forming regions with the SCUBA-2 camera on the James Clerk Maxwell Telescope (JCMT). Temperature and column density maps are obtained from the SCUBA-2 4…

astro-ph.IM2019

The Simons Observatory: Astro2020 Decadal Project Whitepaper

The Simons Observatory Collaboration, Maximilian H. Abitbol, Shunsuke Adachi +280

The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough…

astro-ph.IM2017

The EBEX Balloon-Borne Experiment - Gondola, Attitude Control, and Control Software

The EBEX Collaboration, Asad Aboobaker, Peter Ade +33

The E and B Experiment (EBEX) was a long-duration balloon-borne instrument designed to measure the polarization of the cosmic microwave background (CMB) radiation. EBEX was the fir…

astro-ph.IM2021

The Simons Observatory Large Aperture Telescope Receiver

Ningfeng Zhu, Tanay Bhandarkar, Gabriele Coppi +68

The Simons Observatory (SO) Large Aperture Telescope Receiver (LATR) will be coupled to the Large Aperture Telescope located at an elevation of 5,200 m on Cerro Toco in Chile. The…

astro-ph.IM2010

The EBEX Cryostat and Supporting Electronics

Ilan Sagiv, Asad M. Aboobaker, Chaoyun Bao +41

We describe the cryostat and supporting electronics for the EBEX experiment. EBEX is a balloon-borne polarimeter designed to measure the B-mode polarization of the cosmic microwave…

astro-ph.IM2018

Intensity-Coupled-Polarization in Instruments with a Continuously Rotating Half-Wave Plate

Joy Didier, Amber D. Miller, Derek Araujo +31

We discuss a systematic effect associated with measuring polarization with a continuously rotating half-wave plate. The effect was identified with the data from the E and B Experim…

astro-ph.IM2016

Temperature calibration of the E and B experiment

Francois Aubin, Asad M. Aboobaker, Peter Ade +40

The E and B Experiment (EBEX) is a balloon-borne polarimeter designed to measure the polarization of the cosmic microwave background radiation and to characterize the polarization…

astro-ph.IM2021

The Simons Observatory: the Large Aperture Telescope (LAT)

Zhilei Xu, Shunsuke Adachi, Peter Ade +57

The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at

astro-ph.IM2018

Mexico-UK Sub-millimeter Camera for AsTronomy

Edgar Castillo-Dominguez, Peter Ade, Peter Barry +15

MUSCAT is a large format mm-wave camera scheduled for installation on the Large Millimeter Telescope Alfonso Serrano (LMT) in 2018. The MUSCAT focal plane is based on an array of h…

astro-ph.CO2017

Exploring Cosmic Origins with CORE: Cosmological Parameters

Eleonora Di Valentino, Thejs Brinckmann, Martina Gerbino +125

We forecast the main cosmological parameter constraints achievable with the CORE space mission which is dedicated to mapping the polarisation of the Cosmic Microwave Background (CM…

astro-ph.IM2017

The EBEX Balloon Borne Experiment - Optics, Receiver, and Polarimetry

The EBEX Collaboration, Asad M. Aboobaker, Peter Ade +35

The E and B Experiment (EBEX) was a long-duration balloon-borne cosmic microwave background polarimeter that flew over Antarctica in 2013. We describe the experiment's optical syst…

astro-ph.IM2015

BFORE: The B-mode Foreground Experiment

Michael D. Niemack, Peter Ade, Francesco de Bernardis +19

The B-mode Foreground Experiment (BFORE) is a proposed NASA balloon project designed to make optimal use of the sub-orbital platform by concentrating on three dust foreground bands…

astro-ph.CO2019

The Simons Observatory: Science goals and forecasts

The Simons Observatory Collaboration, Peter Ade, James Aguirre +247

The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scient…

astro-ph.IM2014

The performance of the bolometer array and readout system during the 2012/2013 flight of the E and B experiment (EBEX)

Kevin MacDermid, Asad M. Aboobaker, Peter Ade +38

EBEX is a balloon-borne telescope designed to measure the polarization of the cosmic microwave background radiation. During its eleven day science flight in the Austral Summer of 2…