Renoir

The RENOIR team (Recherche Energie NOIRe) is a research team in cosmology whose goal is to answer the major open questions of modern cosmology. The main objective is to understand the recent acceleration of the expansion of the Universe. This acceleration of expansion is often associated with a mysterious dark energy that represents 70% of the universe's content. The study of dark energy is done by cosmological measurements based on cosmological probes (supernovae Ia, galaxies and cosmic voids).

The team is involved in several major cosmological surveys:

  • eBOSS/DESI where the CPPM develops cosmological tests on cosmic voids.
  • Euclid, an ESA space mission, where the team is responsible for characterizing the infrared detectors of the NISP spectro-photometer and developing an image simulator of this instrument used to prepare for data processing.
  • LSST, a future imager where the CPPM is in charge of the construction of the auto-changer of the filter exchange system and works in parallel with the preparation of supernovæ analyses and photometric calibrations.

More information available here

eBOSS - Credit eBOSS
Euclid - Credit Euclid
Credit LSST Project/NSF/AURA

Researchers and Research professors

Chaire of excellence

Engineers and Technicians

Post-doctoral fellows and CDD

PHD students

To determine the energy content of the Universe and measure its cosmic history, an observational method is to use Baryonic Acoustic Oscillations (BAO) as the standard scale in the spatial distribution of galaxies.

One of the challenges of BAO is the small amplitude of the signal, requiring the survey of huge cosmic volumes in order to obtain an accurate distance measurement. The BOSS survey, for Baryon Oscillation Spectroscopic Survey (Dawson et al. 2013), of SDSS-III (2009-2014) was part of this new generation of galaxy spectroscopic surveys, proposing to map the three-dimensional distribution of 1.5 million Luminous Red Galaxies (LRGs) located between 0.2 < z < 0.8 over a 10 000 deg2 view field. At the same time, BOSS probed the intergalactic medium (IGM) across the 160,000 quasars line of sight located between 2.3 < z < 2.8 using the Lyman-alpha (Ly-alpha) forest. The eBOSS project, for extended-BOSS (Dawson et al. 2016), succeeded BOSS in 2014. The goal of eBOSS, planned for 6 years until 2019, is to cover the entire domain in intermediate redshift, i.e. 0.6 < z < 3.5.

The group has been involved since 2010 in the study of emission line galaxies (ELG) in order to anticipate future surveys of distant galaxies that should cover the almost unexplored range of redshifts z>0.8. In order to improve our understanding of the nature of dark energy, we also participated in the application of a very promising new cosmological test, the Alcock-Paczynski (AP) test (Alcock et al. 1979). In particular we are interested in cosmic voids using the recent works of (Lavaux et al. 2012) who introduced the idea of extracting cosmological information from stacked cosmic voids.

The DESI (Dark Energy Spectroscopic Instrument) project (Aghamousa et al. 2016) consists of an innovative multi-object spectrograph (10 spectrographs with 3 spectral channels each), powered by 5000 optical fibers that can simultaneously produce 5000 galaxy spectra. The instruments will be installed on the 4-meter diameter Mayall telescope located in Arizona, USA, which has been dedicated to this project. In 2014, we obtained funding from AMIDEX (IDEX of Aix-Marseille University) in support of the DESI project in the context of a call for technology transfer. With this support we participate in the construction of the spectrographs that will be delivered to the project.

DESI will use the 4m Mayall telescope at Kitt Peak (©NOAO/AURA/NSF)
DESI will be composed of ten spectrometers, each equipped with 3 arms, a blue one (360 to 593nm), a red one (566 to 772 nm) and a near infrared one (747 to 980 nm)

Euclid is a space mission dedicated to the study of the acceleration of the Universe. Euclid launched on 1st july 2023 for a period of 6 years to study the large structures of the Universe over more than 15,000 square degrees up to a cosmic time of 10 billion year. The mission is optimized for two cosmological probes, the weak lensing and the galaxy clustering but will also address many other cosmological tests such as cluster measurements.

The CPPM, through the Renoir team, involved in the preparation of the Euclid mission. The group involved in the characterization and integration of near-infrared detectors of the NISP spectrophotometer, one of Euclid's two instruments. The H2RG detectors, delivered by NASA, have been characterized at the CPPM and are integrated into the focal plane of the NISP instrument. The CPPM was also in charge of calibrating the instrument before its delivery to ESA (at may 2020).

The second major involvement of the CPPM team concerns the Euclid ground segment (SGS). Ground segment is responsible for data processing and is distributed in the major European countries participating in the project. It is organized around operational units (OU), in charge of defining processing algorithms, and around Data Centers (SDC), in charge of implementing pipelines and producing catalogues. The CPPM is responsible for the development of the TIPS simulator (spectroscopic images of the NISP instrument), as well as its integration into the consortium's pipeline. The CPPM also participates in the production of simulations at the French SDC (CC-IN2P3).

At the science level, we participate in activities of the Galaxy Clustering Science Working Group (GC-SWG), we are leader of the Work-Package (WP) "New Probes", as well as of the SWG on transients/SNe. We are particularly involved in galaxy clustering analyses, cosmic voids, homogeneity scale and probe combination.

Mechanical model of the Euclid NISP instrument © CPPM
Demonstration model of the NI-DS detection system of the NISP instrument © CPPM

LSST is an 8 m ground-based telescope project that will cover the entire sky (20,000 deg²) in several photometric bands selected using colour filters. It will be built nearby the Gemini South (8.2 m) and SOAR (4.3 m) telescopes at the Cerro Pachón site. It is expected to provide its first images in 2023. During the 10 years of its operating phase (2023-2033), LSST will produce at least 10 times more data than the existing one. With one installation every 15 s, about 20 to 30 Terabytes per night are expected, for a total of about 30 Petabytes of data. Each installation covers 10 deg². The data will be reduced in two major mirror computing centers: the National Center for Supercomputing Applications (NCSA) in Illinois and the IN2P3 Computing Center.

The CPPM is responsible for coordinating the construction of the LSST filter changer system and for the construction of one of its subsystems: the auto-changer. Indeed, the camera's filter exchange system is composed of three automated systems: a carousel of 5 optical filters, a filter changer (the Auto Changer) which can, at any time, replace one of the 5 filters in place. The 6th filter can be interchanged in the camera during the day with a filter loading mechanism (the Loader). The system is validated by a test bench to simulate the actual camera configuration.

The team is working on the preparation of supernovæ analyses and photometric calibrations.

We are therefore strongly involved in the use of data reduction software and are working to improve algorithms and procedures for the discovery and photometric measurement of supernovae. We use the expertise acquired in this field with SNLS by using LSST software to reprocess SNLS images and reproduce a more complete Hubble diagram than the one published, not limiting ourselves to supernovae that have benefited from spectroscopic follow up.

The measurement of the Hubble diagram of supernovae is limited, already with current statistics, by systematic errors. In particular, photometric calibration will be a key point. We have therefore started an activity on photometric calibration. We focus on the use of external observations from the Gaia catalogue. We also have an experimental participation in the implementation of the DICE diode calibration project at OHP(obervatoire de haute provence)

Auto-Changer prototype, built at CPPM - Credit CPPM
Detection of a Supernova with LSST software on CFHT images - Credit CPPM
PhD started in 2023
Subject: Preparation and Exploitation of Euclid Data for Gravitational Wave Cosmology
Fundings: Cotutelle IPhU/AMIDEX - La Sapienza (Italie)
PhD director : Eric Kajfasz
PhD started in 2022
Subject: Tester la relativité générale en mesurant le taux de croissance des structures avec les observations de supernovas de Rubin/LSST
Fundings: CNRS ANR DEEPDIP et IPHU/A*MIDEX
PhD director : Dominique Fouchez
Co-supervisor: Stéphane Arnouts
Subject: Testing dark energy with the ISW effect in the Euclid mission
Fundings: IN2P3 et CNES
PhD director : Stéphanie Escoffier
Co-supervisor: William Gillard
Subject: Modélisation de la réponse instrumentale du NISP
Fundings: CNES et ANR
PhD director : Stéphanie Escoffier
Co-supervisor: William Gillard
PhD started in 2021
Subject: Préparation de la mission spatiale Euclid : étude des corrélations, au niveau du pixel, de la réponse des détecteurs infrarouges
Fundings: CNRS/CNES
PhD director : Eric Kajfasz
Co-supervisor: Aurélia Secroun
Subject: Growth-rate measurements with peculiar velocities using models based on n-body simulations
Fundings: A*midex chaire d'excellence darkuni
PhD director : Julian Bautista
Subject: Growth-rate measurements from redshift-space distortions of DESI galaxies
Fundings: A*midex chaire d'excellence darkuni
PhD director : Julian Bautista
Subject: Contraintes cosmologiques par analyse tomographique des données Euclid
Fundings: Contrat doctoral AMU
PhD director : William Gillard
Co-supervisor: Stéphanie Escoffier
See old PhDs (16)

Publications RENOIR

Articles

2024: 2 articles

  • Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument, A. G. Adame et al. , DESI Collaboration, Astron. J. 167 (2024) 62
  • Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracy, S. Paltani et al. , Euclid Collaboration, Astron. Astrophys. 681 (2024) A66

2023: 26 articles

  • Astrophysics with the Laser Interferometer Space Antenna, Amaro-Seoane, Pau et al. , LISA Collaboration, Living Rev.Rel. 26 (2023) 2.
  • Cosmology with the Laser Interferometer Space Antenna, P. Auclair et al. , LISA Collaboration, Living Rev.Rel. 26 (2023) 5
  • Euclid: Forecasts from the void-lensing cross-correlation, M. Bonici et al. , Euclid Collaboration, Astron. Astrophys. 670 (2023) A47
  • Euclid preparation: XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images, L. Bisigello et al. , Euclid Collaboration, Mon. Not. Roy. Astron. Soc 520 (2023) 3529
  • Euclid: Testing the Copernican principle with next-generation surveys, D. Camarena et al. , Euclid Collaboration, Astron. Astrophys. 671 (2023) A68
  • Euclid preparation: XXIV. Calibration of the halo mass function in Λ(ν)\Lambda(\nu) CDM cosmologies, Castro, T. et al. , Euclid Collaboration, Astron. Astrophys. 671 (2023) A100
  • Void BAO measurements on quasars from eBOSS, A. Tamone et al. , Mon. Not. Roy. Astron. Soc 526 (2023) 2889-2902
  • The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies, Lan, Ting-Wen et al. , DESI Collaboration, Astrophys. J 943 (2023) 68
  • Euclid: Calibrating photometric redshifts with spectroscopic cross-correlations, K. Naidoo et al. , Euclid Collaboration, Astron. Astrophys. 670 (2023) A149
  • The PAU Survey & Euclid: Improving broad-band photometric redshifts with multi-task learning, L. Cabayol et al. , Euclid Collaboration, Astron. Astrophys. 671 (2023) A153
  • Euclid preparation: XXV. The Euclid Morphology Challenge -- Towards model-fitting photometry for billions of galaxies, E. Merlin et al. , Euclid Collaboration, Astron. Astrophys. 671 (2023) A101.
  • Euclid preparation: XXII. Selection of Quiescent Galaxies from Mock Photometry using Machine Learning, A. Humphrey et al. , Euclid Collaboration, Astron. Astrophys. 671 (2023) A99
  • Euclid preparation: XXVI. The Euclid Morphology Challenge. Towards structural parameters for billions of galaxies, H. Bretonnière et al. , Euclid Collaboration, Astron. Astrophys. 671 (2023) A102
  • Efficient Computation of Super-Sample Covariance for Stage IV Galaxy Surveys, F. Lacasa et al. , Astron. Astrophys. 671 (2023) A115
  • BICEP/Keck XVI. Characterizing Dust Polarization through Correlations with Neutral Hydrogen, Ade, P.A. R. et al. , Astrophys. J 945 (2023) 72
  • Bump Morphology of the CMAGIC Diagram, L. Aldoroty et al. , Astrophys. J 948 (2023) 10
  • Cosmic void exclusion models and their impact on the distance scale measurements from large-scale structure, A. Variu et al. , Mon. Not. Roy. Astron. Soc 521 (2023) 4731-4749
  • Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations, C. Giocoli et al. , Euclid Collaboration, Astron. Astrophys. 676 (2023) A67
  • Euclid: Cosmology forecasts from the void-galaxy cross-correlation function with reconstruction, S. Radinovic et al. , Euclid Collaboration, Astron. Astrophys. 677 (2023) A78
  • Data release of the AST3-2 automatic survey from Dome A, Antarctica, X. Yang et al. , Mon. Not. Roy. Astron. Soc 520 (2023) 5635-5650
  • Euclid preparation. XXX. Performance assessment of the NISP Red-Grism through spectroscopic simulations for the Wide and Deep surveys, L. Gabarra et al. , Euclid Collaboration, Astron. Astrophys. 676 (2023) A34
  • Growth-rate measurement with type-Ia supernovae using ZTF survey simulations, B. Carreres et al. , ZTF Collaboration, Astron. Astrophys. 674 (2023) A197
  • DEMNUni: the imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing, P. Vielzeuf et al. , J. Cosmol. Astropart. P 08 (2023) 010
  • Euclid preparation: XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibration, K. Paterson et al. , Euclid Collaboration, Astron. Astrophys. 674 (2023) A172
  • Euclid preparation: XXIX. Water ice in spacecraft part I: The physics of ice formation and contamination, M. Schirmer et al. , Euclid Collaboration, Astron. Astrophys. 675 (2023) A142
  • The Dark Energy Spectroscopic Instrument: one-dimensional power spectrum from first Ly α forest samples with Fast Fourier Transform, C. Ravoux et al. , DESI Collaboration, Mon. Not. Roy. Astron. Soc 526 (2023) 5118-5140

2022: 39 articles

  • The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids, M. Aubert et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 513 (2022) 186
  • HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps, Wolz, Laura et al. , Mon. Not. Roy. Astron. Soc 510 (2022) 3495–3511
  • Euclid preparation: XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis, Ilić, S. et al. , Euclid Collaboration, Astron. Astrophys. 657 (2022) A91
  • Euclid preparation: XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis, S. Ilić et al. , Euclid Collaboration, Astron. Astrophys. 657 (2022) A91
  • Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects, D. Forero-Sánchez et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 513 (2022) 5407
  • Euclid preparation: I. The Euclid Wide Survey, Scaramella, R. et al. , Euclid Collaboration, Astron. Astrophys. 662 (2022) A112
  • Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids, Hamaus, N. et al. , Euclid Collaboration, Astron. Astrophys. (2022)
  • Impact of survey geometry and super-sample covariance on future photometric galaxy surveys, S. Gouyou Beauchamps et al. , Astron. Astrophys. 659 (2022) A128
  • Euclid: Constraining ensemble photometric redshift distributions with stacked spectroscopy, Cagliari, M.S. et al. , Euclid Collaboration, Astron. Astrophys. 660 (2022) A9
  • Euclid: Constraining ensemble photometric redshift distributions with stacked spectroscopy, Cagliari, M.S. et al. , Euclid Collaboration, Astron. Astrophys. 660 (2022) A9
  • On the maximum luminosities of normal stripped-envelope supernovae -- brighter than explosion models allow, J. Sollerman et al. , Astron. Astrophys. 657 (2022) A64
  • The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids, C. Zhao et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 511 (2022) 5492
  • Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering, Lepori, F. et al. , Euclid Collaboration, Astron. Astrophys. 662 (2022) A93
  • KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography, Loureiro, A. et al. , Euclid Collaboration, Astron. Astrophys. 665 (2022) A56
  • Angular systematics-free cosmological analysis of galaxy clustering in configuration space, R. Paviot et al. , Mon. Not. Roy. Astron. Soc 512 (2022) 1341-1356
  • Euclid: Forecast constraints on consistency tests of the Λ\Lambda CDM model, Nesseris, S. et al. , Euclid Collaboration, Astron. Astrophys. 660 (2022) A67
  • Euclid: Forecast constraints on consistency tests of the ΛCDM model, S. Nesseris et al. , Euclid Collaboration, Astron. Astrophys. 660 (2022) A67
  • Euclid preparation: XVII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields, Moneti, Andrea et al. , Euclid Collaboration, Astron. Astrophys. 658 (2022) A126
  • Euclid preparation: XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields, Moneti, Andrea et al. , Euclid Collaboration, Astron. Astrophys. 658 (2022) A126
  • SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy, B. Sánchez et al. , LSST Dark Energy Science Collaboration, Astrophys. J 934 (2022) 96
  • The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data, Abdurro'uf et al. , SDSS Collaboration, Astrophys. J. Suppl. S 259 (2022) 35
  • Euclid: Covariance of weak lensing pseudo-Cℓ estimates - Calculation, comparison to simulations, and dependence on survey geometry, R. E. Upham et al. , Euclid Collaboration, Astron. Astrophys. 660 (2022) A114
  • Euclid preparation: XVIII. The NISP photometric system, M. Schirmer et al. , Euclid Collaboration, Astron. Astrophys. 662 (2022) A92
  • Model BOSS & eBOSS Luminous Red Galaxies at 0.2 < z < 1.0 using SubHalo Abundance Matching with 3 parameters, Yu, Jiaxi et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 516 (2022) 57
  • Euclid: Searching for pair-instability supernovae with the Deep Survey, T. J. Moriya et al. , Euclid Collaboration, Astron. Astrophys. 666 (2022) A157
  • Tracing the environmental history of observed galaxies via extended fast action minimization method, E. Sarpa et al. , Mon. Not. Roy. Astron. Soc 516 (2022) 231-244
  • The detection efficiency of Type Ia supernovae from the Zwicky Transient Facility: limits on the intrinsic rate of early flux excesses, M. R. Magee et al. , Mon. Not. Roy. Astron. Soc 513 (2022) 3035-3049
  • Uniform Recalibration of Common Spectrophotometry Standard Stars onto the CALSPEC System using the SuperNova Integral Field Spectrograph, Rubin, David et al. , Nearby Supernova Factory Collaboration, Astrophys. J. Suppl. S 263 (2022) 1
  • New horizons for fundamental physics with LISA, K. G. Arun et al. , Living Rev.Rel. 25 (2022) 4
  • Euclid preparation: XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey, van Mierlo, S.E. et al. , Euclid Collaboration, Astron. Astrophys. 666 (2022) A200
  • The effect of quasar redshift errors on Lyman-α\alpha forest correlation functions, Youles, Samantha et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 516 (2022) 421
  • Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument, B. Abareshi et al. , DESI Collaboration, Astron. J. 164 (2022) 207
  • Euclid: Cosmological forecasts from the void size function, S. Contarini et al. , Euclid Collaboration, Astron. Astrophys. 667 (2022) A162
  • Euclid: Fast two-point correlation function covariance through linear construction, E. Keihanen et al. , Euclid Collaboration, Astron. Astrophys. 666 (2022) A129
  • Euclid preparation: XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data release, R. Saglia et al. , Euclid Collaboration, Astron. Astrophys. 664 (2022) A196
  • Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey II: measurements in Fourier space with optimal weights, Mueller, Eva-Maria et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 514 (2022) 3396-3409
  • A Probabilistic Autoencoder for Type Ia Supernova Spectral Time Series, G. Stein et al. , Nearby Supernova Factory Collaboration, Astrophys. J 935 (2022) 5
  • SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Massive Helium-Shell Detonation in a Star-Forming Galaxy, C. Liu et al. , indéfini (2022)
  • Baryon acoustic oscillations from a joint analysis of the large-scale clustering in Fourier and configuration space, T. Dumerchat et al. , Astron. Astrophys. 667 (2022) A80

2021: 21 articles

  • The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: one thousand multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release, C. Zhao et al. , Mon. Not. Roy. Astron. Soc 503 (2021) 1149-1173
  • The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body mock challenge for galaxy clustering measurements, G. Rossi et al. , Mon. Not. Roy. Astron. Soc 505 (2021) 377-407
  • The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body mock challenge for the eBOSS Emission Line Galaxy sample, S. Alam et al. , Mon. Not. Roy. Astron. Soc 504 (2021) 4667.
  • Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory, S. Alam et al. , Phys. Rev. D 103 (2021) 083533
  • Fink, a new generation of broker for the LSST community, A. Möller et al. , Mon. Not. Roy. Astron. Soc 501 (2021) 3272-3288
  • Euclid preparation: IX. EuclidEmulator2 – power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations, M. Knabenhans et al. , Euclid Collaboration, Mon. Not. Roy. Astron. Soc 505 (2021) 2840-2869
  • Euclid: Impact of non-linear and baryonic feedback prescriptions on cosmological parameter estimation from weak lensing cosmic shear, M. Martinelli et al. , Euclid Collaboration, Astron. Astrophys. 649 (2021) A100
  • BICEP/Keck XII: Constraints on axionlike polarization oscillations in the cosmic microwave background, P.A.R. Ade et al. , Phys. Rev. D 103 (2021) 042002
  • Euclid: Forecasts for kk -cut 3×23 \times 2 Point Statistics, P. L. Taylor et al. , Euclid Collaboration, The Open Journal of Astrophysics 4 (2021) 6.
  • Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography, O. Ilbert et al. , Euclid Collaboration, Astron. Astrophys. 647 (2021) A117
  • Gravitation and the Universe from large scale-structures: The GAUSS mission concept Mapping the cosmic web up to the reionization era, A. Blanchard et al. , Exper. Astron 51 (2021) 1623-1640
  • Euclid: Effect of sample covariance on the number counts of galaxy clusters, A. Fumagalli et al. , Euclid Collaboration, Astron. Astrophys. 652 (2021) A21
  • Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses, A. Pocino et al. , Euclid Collaboration, Astron. Astrophys. 655 (2021) A44
  • Euclid: Estimation of the Impact of Correlated Readout Noise for Flux Measurements with the Euclid NISP Instrument, A. Jiménez Muñoz et al. , Euclid Collaboration, Publ. Astron. Soc. Pac 133 (2021) 094502
  • Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using Deep Generative Models, H. Bretonnière et al. , Euclid Collaboration, Astron. Astrophys. 657 (2021) A90
  • The Twins Embedding of Type Ia Supernovae I: The Diversity of Spectra at Maximum Light, K. Boone et al. , Nearby Supernova Factory Collaboration, Astrophys. J 912 (2021) 70
  • The Twins Embedding of Type Ia Supernovae II: Improving Cosmological Distance Estimates, K. Boone et al. , Nearby Supernova Factory Collaboration, Astrophys. J 912 (2021) 71
  • Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data, M. Martinelli et al. , Euclid Collaboration, Astron. Astrophys. 654 (2021) A148.
  • Euclid Preparation: XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3, Stanford, S.A. et al. , Euclid Collaboration, Astrophys. J. Suppl. S 256 (2021) 9
  • The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the growth rate of structure from the small-scale clustering of the luminous red galaxy sample, M. J. Chapman et al. , eBOSS Collaboration, Mon. Not. Roy. Astron. Soc 516 (2021) 617
  • BICEP/Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season, P.A.R. Ade et al. , Phys. Rev. Lett 127 (2021) 151301

2020: 24 articles

  • Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies, C. Zhao et al. , SDSS Collaboration, Mon. Not. Roy. Astron. Soc 491 (2020) 4554-4572
  • Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate, M. Rigault et al. , Nearby Supernova Factory Collaboration, Astron. Astrophys. 644 (2020) A176
  • High-precision Monte-Carlo modelling of galaxy distribution, P. Baratta et al. , Astron. Astrophys. 633 (2020) A26
  • Constraints on the growth of structure around cosmic voids in eBOSS DR14, A. J. Hawken et al. , J. Cosmol. Astropart. P 2006 (2020) 012
  • SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features, P.-F. Léget et al. , Nearby Supernova Factory Collaboration, Astron. Astrophys. 636 (2020) A46
  • Euclid: Reconstruction of Weak Lensing mass maps for non-Gaussianity studies, S. Pires et al. , Euclid Collaboration, Astron. Astrophys. 638 (2020) A141
  • Euclid preparation: VI. Verifying the Performance of Cosmic Shear Experiments, P. Paykari et al. , Euclid Collaboration, Astron. Astrophys. 635 (2020) A139
  • Euclid preparation: VII. Forecast validation for Euclid cosmological probes, A. Blanchard et al. , Euclid Collaboration, Astron. Astrophys. 642 (2020) A191
  • The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra, R. Ahumada et al. , SDSS Collaboration, Astrophys. J. Suppl. S 249 (2020) 3
  • Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments, A. C. Deshpande et al. , Euclid Collaboration, Astron. Astrophys. 636 (2020) A95
  • Prospects for Fundamental Physics with LISA, E. Barausse et al. , Gen. Relat. Gravit 52 (2020) 81
  • PhotoWeb redshift: boosting photometric redshift accuracy with large spectroscopic surveys, M. Shuntov et al. , Astron. Astrophys. 636 (2020) A90
  • Euclid: the selection of quiescent and star-forming galaxies using observed colours, L. Bisigello et al. , Euclid Collaboration, Mon. Not. Roy. Astron. Soc 494 (2020) 2337-2354
  • Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey, I. Tutusaus et al. , Euclid Collaboration, Astron. Astrophys. 643 (2020) A70
  • Euclid preparation: VIII. The Complete Calibration of the Colour–Redshift Relation survey: VLT/KMOS observations and data release, V. Guglielmo et al. , Euclid Collaboration, Astron. Astrophys. 642 (2020) A192
  • The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space, Y. Wang et al. , Mon. Not. Roy. Astron. Soc 498 (2020) 3470-3483
  • The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues for cosmological analysis, A. J. Ross et al. , Mon. Not. Roy. Astron. Soc 498 (2020) 2354-2371
  • The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0, H. Gil-Marin et al. , Mon. Not. Roy. Astron. Soc 498 (2020) 2492-2531
  • The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample, A. Tamone et al. , Mon. Not. Roy. Astron. Soc 499 (2020) 5527-5546
  • The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1, J. E. Bautista et al. , Mon. Not. Roy. Astron. Soc 500 (2020) 736-762
  • Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes, M. Martinelli et al. , Euclid Collaboration, Astron. Astrophys. 644 (2020) A80
  • The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample, S. Nadathur et al. , Mon. Not. Roy. Astron. Soc 499 (2020) 4140-4157
  • Euclid preparation: X. The Euclid photometric-redshift challenge, G. Desprez et al. , Euclid Collaboration, Astron. Astrophys. 644 (2020) A31
  • Euclid: Identification of asteroid streaks in simulated images using StreakDet software, M. Pöntinen et al. , Euclid Collaboration, Astron. Astrophys. 644 (2020) A35

Conference proceedings

2022: 6 conference proceedings

  • Snowmass 2021 CMB-S4 White Paper, K. Abazajian, A. Abdulghafour, G. E. Addison, P. Adshead, Z. Ahmed, M. Ajello, D. Akerib, S. W. Allen, D. Alonso, M. Alvarez, M. A. Amin, M. Amiri, A. Anderson, B. Ansarinejad, M. Archipley, K. S. Arnold, M. Ashby, H. Aung, C. Baccigalupi, C. Baker, A. Bakshi, D. Bard, D. Barkats, D. Barron, P. S. Barry, J. G. Bartlett, P. Barton, R. Basu Thakur, N. Battaglia, J. Beall, R. Bean, D. Beck, S. Belkner, K. Benabed, A. N. Bender, B. A. Benson, B. Besuner, M. Bethermin, S. Bhimani, F. Bianchini, S. Biquard, I. Birdwell, C. A. Bischoff, L. Bleem, P. Bocaz, J. J. Bock, S. Bocquet, K. K. Boddy, J. R. Bond, J. Borrill, F. R. Bouchet, T. Brinckmann, M. L. Brown, S. Bryan, V. Buza, K. Byrum, E. Calabrese, V. Calafut, R. Caldwell, J. E. Carlstrom, J. Carron, T. Cecil, A. Challinor, V. Chan, C. L. Chang, S. Chapman, E. Charles, E. Chauvin, C. Cheng, G. Chesmore, K. Cheung, Y. Chinone, J. Chluba, H.-M.S. Cho, S. Choi, J. Clancy, S. Clark, A. Cooray, G. Coppi, J. Corlett, W. Coulton, T. M. Crawford, A. Crites, A. Cukierman, F.-Y. Cyr-Racine, W.-M. Dai, C. Daley, E. Dart, G. Daues, T. de Haan, C. Deaconu, J. Delabrouille, G. Derylo, M. Devlin, E. Di Valentino, M. Dierickx, B. Dober, R. Doriese, S. Duff, D. Dutcher, C. Dvorkin, R. Dunner, T. Eftekhari, J. Eimer, H. E. Bouhargani, T. Elleflot, N. Emerson, J. Errard, T. Essinger-Hileman, G. Fabbian, V. Fanfani, A. Fasano, C. Feng, S. Ferraro, J. P. Filippini, R. Flauger, B. Flaugher, A. A. Fraisse, J. Frisch, A. Frolov, N. Galitzki, P. A. Gallardo, S. Galli, K. Ganga, M. Gerbino, C. Giannakopoulos, M. Gilchriese, V. Gluscevic, N. GoecknerWald, D. Goldfinger, D. Green, P. Grimes, D. Grin, E. Grohs, R. Gualtieri, V. Guarino, J. E. Gudmundsson, I. Gullett, S. Guns, S. Habib, G. Haller, M. Halpern, N. W. Halverson, S. Hanany, E. Hand, K. Harrington, M. Hasegawa, M. Hasselfield, M. Hazumi, K. Heitmann, S. Henderson, B. Hensley, R. Herbst, C. Hervias-Caimapo, J. C. Hill, R. Hills, E. Hivon, R. Hlozek, A. Ho, G. Holder, M. Hollister, W. Holzapfel, J. Hood, S. Hotinli, A. Hryciuk, J. Hubmayr, K. M. Huffenberger, H. Hui, R. Ibanez, A. Ibitoye, M. Ikape, K. Irwin, C. Jacobus, O. Jeong, B. R. Johnson, D. Johnstone, W. C. Jones, J. Joseph, B. Jost, J. H. Kang, A. Kaplan, K. S. Karkare, N. Katayama, R. Keskitalo, C. King, T. Kisner, M. Klein, L. Knox, B. J. Koopman, A. Kosowsky, J. Kovac, E. D. Kovetz, A. Krolewski, D. Kubik, S. Kuhlmann, C.-L. Kuo, A. Kusaka, A. Lahteenmaki, K. Lau, C. R. Lawrence, A. T. Lee, L. Legrand, M. Leitner, C. Leloup, A. Lewis, D. Li, E. Linder, I. Liodakis, J. Liu, K. Long, T. Louis, M. Loverde, L. Lowry, C. Lu, P. Lubin, Y.-Z. Ma, T. Maccarone, M. S. Madhavacheril, F. Maldonado, A. Mantz, G. Marques, F. Matsuda, P. Mauskopf, J. May, H. McCarrick, K. McCracken, J. McMahon, P. D. Meerburg, J.-B. Melin, F. Menanteau, J. Meyers, M. Millea, V. Miranda, D. Mitchell, J. Mohr, L. Moncelsi, M. E. Monzani, M. Moshed, T. Mroczkowski, S. Mukherjee, M. Munchmeyer, D. Nagai, C. Nagarajappa, J. Nagy, T. Namikawa, F. Nati, T. Natoli, S. Nerval, L. Newburgh, H. Nguyen, E. Nichols, A. Nicola, M. D. Niemack, B. Nord, T. Norton, V. Novosad, R. O'Brient, Y. Omori, G. Orlando, B. Osherson, R. Osten, S. Padin, S. Paine, B. Partridge, S. Patil, D. Petravick, M. Petroff, E. Pierpaoli, M. Pilleux, L. Pogosian, K. Prabhu, C. Pryke, G. Puglisi, B. Racine , S. Raghunathan, A. Rahlin, M. Raveri, B. Reese, C. L. Reichardt, M. Remazeilles, A. Rizzieri, G. Rocha, N. A. Roe, K. Rotermund, A. Roy, J. E. Ruhl, J. Saba, N. Sailer, M. Salatino, B. Saliwanchik, L. Sapozhnikov, M. S. Rao, L. Saunders, E. Schaan, A. Schillaci, B. Schmitt, D. Scott, N. Sehgal, S. Shandera, B. D. Sherwin, E. Shirokoff, C. Shiu, S. M. Simon, B. Singari, A. Slosar, D. Spergel, T. St. Germaine, S. T. Staggs, A. A. Stark, G. D. Starkman, B. Steinbach, R. Stompor, C. Stoughton, A. Suzuki, O. Tajima, C. Tandoi, G. P. Teply, G. Thayer, K. Thompson, B. Thorne, P. Timbie, M. Tomasi, C. Trendafilova, M. Tristram, C. Tucker, G. Tucker, C. Umilta, A. van Engelen, J. van Marrewijk, E. M. Vavagiakis, C. Verges, J. D. Vieira, A. G. Vieregg, K. Wagoner, B. Wallisch, G. Wang, G.-J. Wang, S. Watson, D. Watts, C. Weaver, L. Wenzl, B. Westbrook, M. White, N. Whitehorn, A. Wiedlea, P. Williams, R. Wilson, H. Winch, E. J. Wollack, W. L. K. Wu, Z. Xu, V. G. Yefremenko, C. Yu, D. Zegeye, J. Zivick, A. Zonca, indéfini, (2022), indéfini,
  • The Latest Constraints on Inflationary B-modes from the BICEP/Keck Telescopes, Ade, P.A.R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, Beck, D., Bischoff, C., Bock, J.J., Boenish, H., Bullock, E., Buza, V., Cheshire, J.R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E.V., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.P., Fliescher, S., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D.C., Grayson, J., Grimes, P., Halal, G., Hall, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S.R., Hilton, G.C., Hubmayr, J., Hui, H., Irwin, K.D., Kang, J., Karkare, K.S., Karpel, E., Kefeli, S., Kernasovskiy, S.A., Kovac, J.M., Kuo, C.L., Lau, K., Leitch, E.M., Lennox, A., Megerian, K.G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.T., O'Brient, R., Ogburn, R.W., Palladino, S., Petroff, M., Prouve, T., Pryke, C., Racine, B., Reintsema, C.D., Richter, S., Schillaci, A., Schmitt, B.L., Schwarz, R., Sheehy, C.D., Singari, B., Soliman, A., Germaine, T. St, Steinbach, B., Sudiwala, R.V., Teply, G.P., Thompson, K.L., Tolan, J.E., Tucker, C., Turner, A., Umilta, C., Verges, C., Vieregg, A.G., Wandui, A., Weber, A.C., Wiebe, D.V., Willmert, J., Wong, C.L., Wu, W.L.K., Yang, H., Yoon, K.W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S., indéfini, 56th Rencontres de Moriond on Cosmology (2022), La Thuile, Italy, 23-30 Jan 2022
  • Measurement of telescope transmission using a Collimated Beam Projector, T. Souverin, J. Neveu, M. Betoule, S. Bongard, S. Brownsberger, J. Cohen-Tanugi, S. Dagoret-Campagne, F. Feinstein , C. Juramy, L. Le Guillou, A. L. Van Suu, P. E. Blanc, F. Hazenberg, E. Nuss, B. Plez, E. Sepulveda, K. Sommer, C. Stubbs, N. Regnault, E. Urbach, indéfini, Moriond 2022 Cosmology 23-30 January 2022 (2022), La Thuile, Italy,
  • Improved polarization calibration of the BICEP3 CMB polarimeter at the South Pole, Cornelison, J., Vergès, C., Ade, P.A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Beck, D., Bischoff, C.A., Bock, J.J., Buza, V., IV, J.R. Cheshire, Connors, J., Crumrine, M., Cukierman, A.J., Denison, E.V., Dierickx, M.I., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.P., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D.C., Grayson, J., Grimes, P.K., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S.A., Henderson, S., Hildebrandt, S.R., Hilton, G.C., Hubmayr, J., Hui, H., Irwin, K.D., Kang, J., Karkare, K.S., Kefeli, S., Kovac, J.M., Kuo, C.L., Lau, K., Leitch, E.M., Lennox, A., Liu, T., Look, K., Megerian, K.G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.T., O'Brient, R., Palladino, S., Petroff, M.A., Prouve, T., Pryke, C., Racine, B., Reintsema, C.D., Salatino, M., Schillaci, A., Schmitt, B.L., Singari, B., Soliman, A., Germaine, T.St., Steinbach, B., Sudiwala, R.V., Thompson, K.L., Tsai, C., Tucker, C., Turner, A.D., Umiltà, C., Vieregg, A.G., Wandui, A., Weber, A.C., Wiebe, D.V., Willmert, J., Wu, W.L. K., Yang, H., Yoon, K.W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S., Proc. SPIE Int. Soc. Opt. Eng., 12190, SPIE Astronomical Telescopes + Instrumentation 2022 (2022) 829, Montréal, Canada, 17-22 Jul 2022
  • 2022 upgrade and improved low frequency camera sensitivity for CMB observation at the South Pole, Sr., A.Soliman, Ade, P.A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C.A., Beck, D., Bock, J.J., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A.J., Denison, E.V., Dierickx, M.I., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.P., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D.C., Grayson, J., Grimes, P.K., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S.A., Henderson, S., Hildebrandt, S.R., Hilton, G.C., Hubmayr, J., Hui, H., Irwin, K.D., Kangh, J., Karkare, K.S., Kefeli, S., Kovac, J.M., Kuo, C.L., Lau, K., Leitch, E.M., Lennox, A., Liu, T., Megerian, K.G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.T., O'Brient, R., Palladino, S., Petroff, M.A., Precup, N., Prouve, T., Pryke, C., Racine, B., Reintsema, C.D., Salatino, M., Schillaci, A., Schmitt, B.L., Singari, B., Germaine, T.St., Steinbach, B., Sudiwala, R.V., Thompson, K.L., Tsai, C., Tucker, C., Turner, A.D., Umiltà, C., Vergès, C., Vieregg, A.G., Wandui, A., Weber, A.C., Wiebe, D.V., Willmert, J., Wu, W.L. K., Yang, H., Yoon, K.W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S., Proc. SPIE Int. Soc. Opt. Eng., 12190, SPIE Astronomical Telescopes + Instrumentation 2022 (2022) 533, Montréal, Canada, 17-22 Jul 2022
  • Thermal testing for cryogenic CMB instrument optical design, Goldfinger, D.C., Ade, P.A.R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Beck, D., Bischoff, C.A., Bock, J.J., Buza, V., IV, J.Cheshire, Connors, J., Cornelison, J., Crumrine, M., Cukierman, A.J., Denison, E.V., Dierickx, M.I., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.P., Giannakopoulos, C., Goeckner-Wald, N., Grayson, J., Grimes, P.K., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S.A., Henderson, S., Hildebrandt, S.R., Hilton, G.C., Hubmayk, J., Hui, H., Irwin, K.D., Kang, J., Karkare, K.S., Kefeli, S., Kovac, J.M., Kuo, C.L., Lau, K., Leitch, E.M., Lennox, A., Liu, T., Megerian, K.G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.T., O'Brient, R., Palladino, S., Petroff, M.A., Prouve, T., Pryke, C., Racine, B., Reintsema, C.D., Salatino, M., Schillaci, A., Schmitt, B.L., Singari, B., Sr., A.Soliman, Smith, A.G., Germaine, T.St., Steinbach, B., Sudiwala, R.V., Thompson, K.L., Tsai, C., Tucker, C., Turner, A.D., Umiltà, C., Vergès, C., Vieregg, A.G., Wandui, A., Weber, A.C., Wiebe, D.V., Willmert, J., Wu, W.L. K., Yang, H., Yoon, K.W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S., Proc. SPIE Int. Soc. Opt. Eng., 12190, SPIE Astronomical Telescopes + Instrumentation 2022 (2022) 805, Montréal, Canada, 17-22 Jul 2022

2021: 1 conference proceeding

  • Galaxy Image Translation with Semi-supervised Noise-reconstructed Generative Adversarial Networks, Q. Lin , D. Fouchez , J. Pasquet, indéfini, 2020 25th International Conference on Pattern Recognition (ICPR) (2021), Milan, Italy, 10-15 Jan 2021

2020: 2 conference proceedings

  • Euclid mission status after mission critical design, Laureijs, R., Racca, G., Mellier, Y., Musi, P., Brouard, L., Boenke, T., Venancio, L.Gaspar, Maiorano, E., Short, A., Strada, P., Altieri, B., Buenadicha, G., Dupac, X., Alvarez, P.Gomez, Hoar, J., Kohley, R., Vavrek, R., Rudolph, A., Schmidt, M., Amiaux, J., Aussel, H., Berthé, M., Cropper, M., Cuillandre, J.C., Dabin, C., Dinis, J., Nakajima, R., Maciaszek, T., Scaramella, R., Silva, A. da, Tereno, I., Williams, O.R., Zacchei, A., Azzollini, R., Bernardeau, F., Brinchmann, J., Brockley-Blatt, C., Castander, F., Cimatti, A., Conselice, C., Ealet, A., Fosalba, P., Gillard, W., Guzzo, L., Hoekstra, H., Hudelot, P., Jahnke, K., Kitching, T., Miller, L., Mohr, J., Percival, W., Pettorino, V., Rhodes, J., Sanchez, A., Sauvage, M., Serrano, S., Teyssier, R., Weller, J., Zoubian, J., Proc. SPIE Int. Soc. Opt. Eng., 11443, SPIE Astronomical Telescopes + Instrumentation 2020 (2020) 114430F, Online, United States, 14-18 Dec 2020
  • Testing the 10 spectrograph units for DESI: approach and results, S. Perruchot, P.-É. Blanc, J. Guy, L. Le Guillou, S. Ronayette, X. Régal, G. Castagnoli, A. Le Van Suu, E. Sepulveda, E. Jullo, J.-G. Cuby, S. Karkar, P. Ghislain, P. Repain, P. H. Carton, C. Magneville, A. Ealet , S. Escoffier , A. Secroun , K. Honscheid, A. Elliott, P. Jelinsky, B. David, D. Peter, Y. Duan, J. Edelstein, J. C. Estrada, E. Gastañaga, A. Karcher, M. Landriau, M. Levi, P. Martini, N. Palanque-Delabrouille, F. Prada, G. Tarle, K. Zhang, Proc. SPIE Int. Soc. Opt. Eng., 11447, SPIE Astronomical Telescopes + Instrumentation 2020 (2020) 1144786, Online, United States, 14-18 Dec 2020

Talks

2021: 1 talk

  • Cosmology from spectroscopic galaxy surveys, S. Escoffier , Workshop “Massively Parallel Large Area Spectroscopy from Space”, remote, France, 21-23 Jun 2021

2020: 1 talk

  • Cosmology with cosmic voids, S. Escoffier , Theory meeting experiments: particle astrophysics and cosmology (TMEX 2020), Quy Nhon, Vietnam, 5-11 Jan 2020

Mémoires

2024: 1 mémoire

  • Advancements towards precision cosmology with Void-Lensing: Observational aspects and modeling, R. Isquierdo Boschetti, Aix-Marseille Université, 06 Fev 2024

2023: 3 mémoires

  • Détermination du taux de croissance des structures avec les supernovae de type Ia à partir du relevé photométrique ZTF, B. Carreres, Aix-Marseille Université, 29 Sep 2023
  • Searching for Primordial Gravitational Waves in the B-mode Polarization of the CMB, B. Racine, Aix-Marseille Université, 14 Sep 2023
  • Dark Energy with Spectroscopic Observations of the Universe, J. Bautista, Aix-Marseille Université, 24 Oct 2023

2021: 4 mémoires

  • A new Monte Carlo method for galaxy clustering analysis, P. Baratta , Aix Marseille Université, 15 Jan 2021
  • Étude cosmologique de la structure à grande échelle dans le sondage spectroscopique eBOSS, R. Paviot, Aix Marseille Université, 15 Nov 2021
  • Deep Learning methods applied to large astrophysical imaging surveys, Q. Lin, Aix Marseille Université, 01 Dec 2021
  • Extraction optimale des paramètres cosmologiques en préparation de la mission Euclid, S. Gouyou Beauchamps, Aix Marseille Université, 15 Dec 2021

2020: 1 mémoire

  • Contraintes cosmologiques avec les vides cosmiques dans eBOSS, M. Aubert, Aix Marseille Université, 16 Dec 2020


Complete list (PDF)
  • LSST: on May 15, 2018, the prototype of the filter changer system, one of the main components of the LSST camera, was inaugurated. This technical feat is the result of collaboration between five CNRS IN2P3 laboratories.In this unique project, France plays a very special role alongside the United States and Chile.
LSST filter exchanger © CPPM
Transport of the LSST filter exchanger © CPPM
  • Euclid: CPPM had just completed the characterization of the 16 flight detectors of the Euclid NISP. Twenty flight detectors, selected by NASA, were delivered to the CPPM, characterized in our clean rooms in 2017-2018. They will be integrated on the NISP instrument in 2019, at LAM (Laboratoire d'Astrophysique de Marseille), with which the CPPM is working closely.
Characterization testbenches for the infrared detectors of the NISP instrument of the Euclid space mission. The flight detectors are tested for 45 days under vacuum at -200°C with a view to evaluate their performance © C.Moirenc
Integration of a Euclid infrared detector for its characterization. This work takes place within an ISO5 environment in a clean room (less than 100 particles of dust per m3) © C.Moirenc
Infrared detector on its transporting stand. This detector is manufactured by the American company Teledyne and characterized at CPPM for the Euclid space mission. © C.Moirenc