most citedStarDICE I: sensor calibration bench and absolute photometric calibration of a Sony IMX411 sensor

7 citations · 7 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2023

Distant foreground and the Hubble constant tension

Vladimir Yershov

It is possible to explain the discrepancy (tension) between the local measurement of the cosmological parameter (the Hubble constant) and its value derived from the Planck-mi…

astro-ph.IM2022★ 7 cited

StarDICE I: sensor calibration bench and absolute photometric calibration of a Sony IMX411 sensor

Marc Betoule, Sarah Antier, Emmanuel Bertin +18

The Hubble diagram of type-Ia supernovae (SNe-Ia) provides cosmological constraints on the nature of dark energy with an accuracy limited by the flux calibration of currently avail…

astro-ph.IM2022

Measurement of telescope transmission using a Collimated Beam Projector

Thierry Souverin, Jérémy Neveu, Marc Betoule +17

The number of type Ia supernova observations will see a significant growth within the next decade, especially thanks to the Legacy Survey of Space and Time undertaken by the Vera R…

astro-ph.CO2022

The Latest Constraints on Inflationary B-modes from the BICEP/Keck Telescopes

Keck Collaboration, P. A. R. Ade, Z. Ahmed +92

For the past decade, the BICEP/Keck collaboration has been operating a series of telescopes at the Amundsen-Scott South Pole Station measuring degree-scale -mode polarization im…

astro-ph.IM2022

How in situ atmospheric transmission can affect cosmological constraints from type Ia supernovae ?

Jérémy Neveu, Vincent Brémaud, Sébastien Bongard +3

The measurement of type Ia supernova colours in photometric surveys is the key to access to cosmological distances. But for future large surveys like the Large Survey of Space and…

astro-ph.CO2022

An Estimator for Lensing Potential from Galaxy Number Counts

Viraj Nistane

We derive an estimator for the lensing potential from galaxy number counts which contains a linear and a quadratic term. We show that this estimator has a much larger signal-to-noi…