P. Natoli

The far-infrared emitting region in local galaxies and QSOs: Size and scaling relations

RELION: Implementation of a Bayesian approach to cryo-EM structure determination

Particle migration analysis in iterative classification of cryo-EM single-particle data

An absorption profile centred at 78 megahertz in the sky-averaged spectrum

On CCC-predicted concentric low-variance circles in the CMB sky

Scanamorphos: A Map-making Software for Herschel and Similar Scanning Bolometer Arrays

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION

Far-Infrared Surveys of Galaxy Evolution

Cosmic microwave background lensing reconstruction on the full sky

High resolution foreground cleaned CMB map from WMAP

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THEWMAPDATA

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: The Angular Power Spectrum

Uncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1–3

HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the Sphere

f(R,T)gravity

The Galaxy in Context: Structural, Kinematic, and Integrated Properties

Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters

Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

unimap: a generalized least-squares map maker for Herschel data

First results from the IllustrisTNG simulations: the galaxy colour bimodality

The HIPASS survey of the Galactic plane in radio recombination lines

Weak gravitational lensing

Ellipticity in cosmic microwave background as a tracer of large-scale universe

Making sky maps from Planck data

Variations of the spectral index of dust emissivity from Hi-GALobservations of the Galactic plane

Fast Spherical Harmonic Analysis: A Quick Algorithm for Generating and/or InvertingFull-Sky, High-Resolution Cosmic Microwave Background Anisotropy Maps

ELLIPTICITY OF LARGE SPOTS IN CMB ANISOTROPY MAPS

The pros and cons of the inversion method approach to derive 3D dust emission properties in the ISM: the Hi-GAL field centred on (l, b) = (30 , 0 )

New estimates of the CMB angular power spectra from theWMAP5 year low-resolution data

Artifact Removal for GLS Map Makers by Means of Post-Processing

Data reduction pipeline for the Hi-GAL survey