activity
20102026
most citedPlanck Early Results: The Planck mission

525 citations · 1k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.CO2026

Euclid: Galaxy SED reconstruction in the PHZ processing function: impact on the PSF and the role of medium-band filters

Euclid Collaboration, F. Tarsitano, C. Schreiber +301

Weak lensing surveys require accurate correction for the point spread function (PSF) when measuring galaxy shapes. For a diffraction-limited PSF, as arises in space-based missions,…

astro-ph.GA2025★ 1 cited

Euclid Quick Data Release (Q1). Photometric redshifts and physical properties of galaxies through the PHZ processing function

Euclid Collaboration, M. Tucci, S. Paltani +344

The ESA Euclid mission will measure the photometric redshifts of billions of galaxies in order to provide an accurate 3D view of the Universe at optical and near-infrared wavelengt…

astro-ph.IM2023★ 10 cited

Euclid preparation. XXIX. Water ice in spacecraft part I: The physics of ice formation and contamination

Euclid Collaboration, M. Schirmer, K. Thürmer +218

Molecular contamination is a well-known problem in space flight. Water is the most common contaminant and alters numerous properties of a cryogenic optical system. Too much ice mea…

astro-ph.GA2021★ 80 cited

Euclid preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields

Andrea Moneti, H. J. McCracken, M. Shuntov +194

We present a new infrared survey covering the three Euclid deep fields and four other Euclid calibration fields using Spitzer's Infrared Array Camera (IRAC). We have combined these…

astro-ph.GA2021★ 32 cited

Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using Deep Generative Models

Euclid Collaboration, H. Bretonnière, M. Huertas-Company +193

We present a machine learning framework to simulate realistic galaxies for the Euclid Survey. The proposed method combines a control on galaxy shape parameters offered by analytic…

astro-ph.IM2017★ 9 cited

The Euclid Data Processing Challenges

Pierre Dubath, Nikolaos Apostolakos, Andrea Bonchi +37

Euclid is a Europe-led cosmology space mission dedicated to a visible and near infrared survey of the entire extra-galactic sky. Its purpose is to deepen our knowledge of the dark…

astro-ph.IM2011★ 88 cited

Planck Early Results. V. The Low Frequency Instrument data processing

A. Zacchei, D. Maino, C. Baccigalupi +146

We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discus…

astro-ph.IM2011★ 143 cited

Planck Early Results. II. The thermal performance of Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +225

The performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative…

astro-ph.IM2011★ 525 cited

Planck Early Results: The Planck mission

Planck Collaboration, P. A. R. Ade, N. Aghanim +272

The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in li…

astro-ph.IM2010★ 4 cited

A systematic approach to the Planck LFI end-to-end test and its application to the DPC Level 1 pipeline

M. Frailis, M. Maris, A. Zacchei +23

The Level 1 of the Planck LFI Data Processing Centre (DPC) is devoted to the handling of the scientific and housekeeping telemetry. It is a critical component of the Planck ground…

astro-ph.IM2010★ 5 cited

LFI Radiometric Chain Assembly (RCA) data handling "Rachel"

M. Malaspina, E. Franceschi, P. Battaglia +26

This paper is part of the Prelaunch status LFI papers published on JINST (http://www.iop.org/EJ/journal/-page=extra.proc5/1748-0221). Planck's Low Frequency Instrument is an array…

astro-ph.IM2010★ 12 cited

Optimization of Planck/LFI on--board data handling

M. Maris, M. Tomasi, S. Galeotta +34

To asses stability against 1/f noise, the Low Frequency Instrument (LFI) onboard the Planck mission will acquire data at a rate much higher than the data rate allowed by its teleme…

astro-ph.IM2010★ 5 cited

Level 1 on-ground telemetry handling in Planck LFI

A. Zacchei, M. Frailis, M. Maris +31

The Planck Low Frequency Instrument (LFI) will observe the Cosmic Microwave Background (CMB) by covering the frequency range 30-70 GHz in three bands. The primary instrument data s…

astro-ph.IM2010★ 10 cited

Off-line radiometric analysis of Planck/LFI data

M. Tomasi, A. Mennella, S. Galeotta +35

The Planck Low Frequency Instrument (LFI) is an array of 22 pseudo-correlation radiometers on-board the Planck satellite to measure temperature and polarization anisotropies in the…

astro-ph.CO2010★ 119 cited

Planck pre-launch status: the Planck-LFI programme

N. Mandolesi, M. Bersanelli, R. C. Butler +140

This paper provides an overview of the Low Frequency Instrument (LFI) programme within the ESA Planck mission. The LFI instrument has been developed to produce high precision maps…