papers

Publications (19)

physics.atom-ph2017

First international comparison of fountain primary frequency standards via a long distance optical fiber link

J. Guéna, S. Weyers, M. Abgrall +25

We report on the first comparison of distant caesium fountain primary frequency standards (PFSs) via an optical fiber link. The 1415 km long optical link connects two PFSs at LNE-S…

astro-ph.GA2018

Gaia Data Release 2: Processing the spectroscopic data

P. Sartoretti, D. Katz, M. Cropper +50

The Gaia Data Release 2 contains the 1st release of radial velocities complementing the kinematic data of a sample of about 7 million relatively bright, late-type stars. Aims: This…

astro-ph2006

Low-excitation blobs in the Magellanic Clouds

F. Meynadier, M. Heydari-Malayeri

Aims : We study an unknown, or very poorly known, interstellar HII component in the Magellanic Clouds. This is the first study ever devoted to this class of objects, which we call…

astro-ph.CO2019

Search for transient variations of the fine structure constant and dark matter using fiber-linked optical atomic clocks

B. M. Roberts, P. Delva, A. Al-Masoudi +51

We search for transient variations of the fine structure constant using data from a European network of fiber-linked optical atomic clocks. By searching for coherent variations in…

astro-ph2007

HST's view of the youngest massive stars in the Magellanic Clouds

M. Heydari-Malayeri, M. R. Rosa, V. Charmandaris +5

Accurate physical parameters of newborn massive stars are essential ingredients to shed light on their formation, which is still an unsolved problem. The rare class of compact H II…

gr-qc2019

Testing the gravitational redshift with Galileo satellites

P. Delva, N. Puchades, E. Schönemann +11

We present the results of the analysis of the GREAT (Galileo gravitational Redshift test with Eccentric sATellites) experiment from SYRTE (Observatoire de Paris), funded by the Eur…

astro-ph2003

Tight LMC massive star clusters R 127 and R 128

M. Heydari-Malayeri, F. Meynadier, Nolan R. Walborn

We study the Large Magellanic Cloud (LMC) star clusters R 127 and R 128 using imaging and spectroscopy obtained at the ESO NTT telescope. An advanced image restoration technique al…

gr-qc2017

Test of special relativity using a fiber network of optical clocks

P. Delva, J. Lodewyck, S. Bilicki +28

Phase compensated optical fiber links enable high accuracy atomic clocks separated by thousands of kilometers to be compared with unprecedented statistical resolution. By searching…

hep-ph2016

Constraints on SME Coefficients from Lunar Laser Ranging, Very Long Baseline Interferometry, and Asteroid Orbital Dynamics

C. Le Poncin-Lafitte, A. Bourgoin, A. Hees +9

Lorentz symmetry violations can be parametrized by an effective field theory framework that contains both General Relativity and the Standard Model of particle physics, called the…

astro-ph.SR2017

Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars

Gaia Collaboration, G. Clementini, L. Eyer +588

Parallaxes for 331 classical Cepheids, 31 Type II Cepheids and 364 RR Lyrae stars in common between Gaia and the Hipparcos and Tycho-2 catalogues are published in Gaia Data Release…

astro-ph2004

Stellar populations associated with the LMC Papillon Nebula

F. Meynadier, M. Heydari-Malayeri, L. Deharveng +5

We study the Large Magellanic Cloud Papillon Nebula (N159-5), a conspicuous High Excitation Blob (HEB) lying in the star forming complex N159. Using JHK near-infrared photometry ob…

physics.atom-ph2015

A clock network for geodesy and fundamental science

C. Lisdat, G. Grosche, N. Quintin +32

Leveraging the unrivaled performance of optical clocks in applications in fundamental physics beyond the standard model, in geo-sciences, and in astronomy requires comparing the fr…

astro-ph2001

Resolving the compact HII regions in N160A with HST

M. Heydari-Malayeri, V. Charmandaris, L. Deharveng +4

Using high-resolution imaging with the Hubble Space Telescope, we study the Large Magellanic Cloud HII region N160A and uncover several striking features of this complex massive st…

physics.atom-ph2023

Roadmap towards the redefinition of the second

N. Dimarcq, M. Gertsvolf, G. Mileti +34

This paper outlines the roadmap towards the redefinition of the second, which was recently updated by the CCTF Task Force created by the CCTF in 2020. The main achievements and the…

astro-ph2003

The stellar environment of SMC N81

M. Heydari-Malayeri, F. Meynadier, V. Charmandaris +4

We present near infrared JHK imaging of the Small Magellanic Cloud compact H II region N81 using the ISAAC camera at the ESO Very Large Telescope (Antu). Our analysis of the stella…

gr-qc2018

A gravitational redshift test using eccentric Galileo satellites

P. Delva, N. Puchades, E. Schönemann +11

We report on a new test of the gravitational redshift and thus of local position invariance, an integral part of the Einstein equivalence principle, which is the foundation of gene…

astro-ph.IM2018

Gaia Data Release 2: Properties and validation of the radial velocities

D. Katz, P. Sartoretti, M. Cropper +51

For Gaia DR2 (GDR2), 280 million spectra, collected by the RVS instrument on-board Gaia, were processed and median radial velocities were derived for 9.8 million sources brighter t…

physics.space-ph2012

Time and frequency transfer with a microwave link in the ACES/PHARAO mission

P. Delva, F. Meynadier, P. Wolf +2

The Atomic Clocks Ensemble in Space (ACES/PHARAO mission), which will be installed on board the International Space Station (ISS), uses a dedicated two-way Micro-Wave Link (MWL) in…

astro-ph.SR2017

Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects

Gaia Collaboration, F. van Leeuwen, A. Vallenari +589

Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a subset of about 2 million stars for which, besides the position and photometry,…