activity
20122026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 13.9k across the 55 of their papers we have counts for

collaborators

55 papers

physics.ins-det2026

A low-cost ice melt monitoring system using wind-induced motion of mass-balance stakes

Felix St-Amour, H. Cynthia Chiang, Jamie Cox +4

Surface ablation measurements of glaciers are critical for understanding mass change over time. Mass-balance stakes are commonly used for localized measurements, with the exposed l…

physics.geo-ph2025★ 2 cited

Estimating Soil Electrical Parameters in the Canadian High Arctic from Impedance Measurements of the MIST Antenna Above the Surface

I. Hendricksen, R. A. Monsalve, V. Bidula +13

The MIST experiment aims to detect the cosmological 21-cm signal through sky observations at 25-125 MHz using a wide-beam antenna. The antenna is mounted above the soil and the bea…

astro-ph.IM2025★ 1 cited

Using the antenna impedance to estimate soil electrical parameters for the MIST global 21-cm experiment

Cinthia Altamirano, Ricardo Bustos, Raul A. Monsalve +11

Radio experiments trying to detect the global ~cm signal from the early Universe are very sensitive to the electrical properties of their environment. For ground-based experime…

astro-ph.GA2024★ 9 cited

Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER

SPIDER Collaboration, P. A. R. Ade, M. Amiri +67

Using data from the first flight of SPIDER and from Planck HFI, we probe the properties of polarized emission from interstellar dust in the SPIDER observing region. Component separ…

astro-ph.CO2024★ 25 cited

First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations

S. Raghunathan, P. A. R. Ade, A. J. Anderson +121

We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel{'}dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and {…

astro-ph.CO2024★ 7 cited

SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos

S. Bocquet, S. Grandis, L. E. Bleem +193

We present cosmological constraints from the abundance of galaxy clusters selected via the thermal Sunyaev-Zel'dovich (SZ) effect in South Pole Telescope (SPT) data with a simultan…

astro-ph.CO2023★ 55 cited

Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey

L. E. Bleem, M. Klein, T. M. C. Abbott +125

We present a catalog of 689 galaxy cluster candidates detected at significance via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-…

astro-ph.IM2023★ 17 cited

Simulating the Detection of the Global 21 cm Signal with MIST for Different Models of the Soil and Beam Directivity

Raul A. Monsalve, Christian H. Bye, Jonathan L. Sievers +10

The Mapper of the IGM Spin Temperature (MIST) is a new ground-based, single-antenna, radio experiment attempting to detect the global 21 cm signal from the Dark Ages and Cosmic Daw…

astro-ph.IM2023★ 50 cited

Mapper of the IGM spin temperature: instrument overview

R. A. Monsalve, C. Altamirano, V. Bidula +17

The observation of the global 21 cm signal produced by neutral hydrogen gas in the intergalactic medium (IGM) during the Dark Ages, Cosmic Dawn, and Epoch of Reionization requires…

astro-ph.IM2021★ 1 cited

In-flight gain monitoring of SPIDER's transition-edge sensor arrays

J. P. Filippini, A. E. Gambrel, A. S. Rahlin +67

Experiments deploying large arrays of transition-edge sensors (TESs) often require a robust method to monitor gain variations with minimal loss of observing time. We propose a sens…

astro-ph.CO2021★ 7 cited

A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra

J. S. -Y. Leung, J. Hartley, J. M. Nagy +67

Modern CMB analysis pipelines regularly employ complex time-domain filters, beam models, masking, and other techniques during the production of sky maps and their corresponding ang…

astro-ph.CO2021★ 4 cited

The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps

A. E. Gambrel, A. S. Rahlin, X. Song +64

We present the XFaster analysis package. XFaster is a fast, iterative angular power spectrum estimator based on a diagonal approximation to the quadratic Fisher matrix estimator. X…

astro-ph.CO2021★ 2 cited

A Constraint on Primordial -Modes from the First Flight of the SPIDER Balloon-Borne Telescope

SPIDER Collaboration, P. A. R. Ade, M. Amiri +68

We present the first linear polarization measurements from the 2015 long-duration balloon flight of SPIDER, an experiment designed to map the polarization of the cosmic microwave b…

astro-ph.CO2020★ 55 cited

Optimal CMB Lensing Reconstruction and Parameter Estimation with SPTpol Data

M. Millea, C. M. Daley, T-L. Chou +66

We perform the first simultaneous Bayesian parameter inference and optimal reconstruction of the gravitational lensing of the cosmic microwave background (CMB), using 100 deg o…

astro-ph.CO2018★ 217 cited

Planck 2018 results. VI. Cosmological parameters

Planck Collaboration, N. Aghanim, Y. Akrami +179

We present cosmological parameter results from the final full-mission Planck measurements of the CMB anisotropies. We find good consistency with the standard spatially-flat 6-param…

astro-ph.CO2017★ 56 cited

SPIDER: CMB polarimetry from the edge of space

R. Gualtieri, J. P. Filippini, P. A. R. Ade +61

SPIDER is a balloon-borne instrument designed to map the polarization of the millimeter-wave sky at large angular scales. SPIDER targets the B-mode signature of primordial gravitat…

astro-ph.IM2017★ 11 cited

280 GHz Focal Plane Unit Design and Characterization for the SPIDER-2 Suborbital Polarimeter

A. S. Bergman, P. A. R. Ade, S. Akers +76

We describe the construction and characterization of the 280 GHz bolometric focal plane units (FPUs) to be deployed on the second flight of the balloon-borne SPIDER instrument. The…

astro-ph.CO2017★ 195 cited

Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol Data

J. W. Henning, J. T. Sayre, C. L. Reichardt +64

We present measurements of the -mode polarization angular auto-power spectrum () and temperature--mode cross-power spectrum () of the cosmic microwave background (CMB…

astro-ph.CO2017★ 45 cited

A New Limit on CMB Circular Polarization from SPIDER

J. M. Nagy, P. A. R. Ade, M. Amiri +58

We present a new upper limit on CMB circular polarization from the 2015 flight of SPIDER, a balloon-borne telescope designed to search for -mode linear polarization from cosmic…

astro-ph.CO2017★ 68 cited

CMB Polarization B-mode Delensing with SPTpol and Herschel

A. Manzotti, K. T. Story, W. L. K. Wu +60

We present a demonstration of delensing the observed cosmic microwave background (CMB) B-mode polarization anisotropy. This process of reducing the gravitational-lensing generated…

astro-ph.GA2016★ 26 cited

Planck intermediate results. XLV. Radio spectra of northern extragalactic radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on f…

astro-ph.HE2016★ 32 cited

Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey

N. Whitehorn, T. Natoli, P. A. R. Ade +55

The millimeter transient sky is largely unexplored, with measurements limited to follow-up of objects detected at other wavelengths. High-angular-resolution telescopes designed for…

astro-ph.CO2015★ 79 cited

Planck 2015 results. XII. Full Focal Plane simulations

Planck Collaboration, P. A. R. Ade, N. Aghanim +228

We present the 8th Full Focal Plane simulation set (FFP8), deployed in support of the Planck 2015 results. FFP8 consists of 10 fiducial mission realizations reduced to 18144 maps,…

astro-ph.CO2015★ 428 cited

Planck 2015 results. XVI. Isotropy and statistics of the CMB

Planck Collaboration, P. A. R. Ade, N. Aghanim +242

We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly…