activity
20102024
most citedPlanck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

422 citations · 3.5k across the 102 of their papers we have counts for

collaborators

103 papers

astro-ph.IM2024★ 1 cited

In-Flight Performance of Spider's 280 GHz Receivers

Elle C. Shaw, P. A. R. Ade, S. Akers +84

SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky…

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.GA2024★ 6 cited

The magnetic field of the Radcliffe Wave: starlight polarization at nearest approach to the Sun

G. V. Panopoulou, C. Zucker, D. Clemens +6

We investigate the geometry of the magnetic field towards the Radcliffe Wave, a coherent 3-kpc-long part of the nearby Local Arm recently discovered via three-dimensional dust mapp…

astro-ph.GA2023

Evidence for Spatial Separation of Galactic Dust Populations

Corwin Shiu, Steven J. Benton, Jeffrey P. Filippini +5

We present an implementation of a Bayesian mixture model using Hamiltonian Monte Carlo (HMC) techniques to search for spatial separation of Galactic dust populations. Utilizing int…

astro-ph.IM2023★ 4 cited

A new tool to derive simultaneously exponent and extremes of power-law distributions

S. Pezzuto, A. Coletta, R. S. Klessen +6

Many experimental quantities show a power-law distribution . In astrophysics, examples are: size distribution of dust grains or luminosity function of galaxies.…

astro-ph.GA2023★ 13 cited

A comparison of the Milky Way's recent star formation revealed by dust thermal emission and high-mass stars

J. D. Soler, E. Zari, D. Elia +10

We present a comparison of the Milky Way's star formation rate (SFR) surface density () obtained with two independent state-of-the-art observational methods. The first…