activity
20212026
most citedThe Vera C. Rubin Observatory Data Preview 1

14 citations · 24 across the 15 of their papers we have counts for

collaborators

17 papers

astro-ph.IM2026

The LSST Science Pipelines Software: Optical Survey Pipeline Reduction and Analysis Environment

Rubin Observatory Science Pipelines Developers, Yusra AlSayyad, Robert Armstrong +83

The NSF-DOE Vera C. Rubin Observatory is executing the Legacy Survey of Space and Time (LSST) as its prime mission, producing a series of data releases over the ten-year survey. Th…

astro-ph.IM2026★ 14 cited

The Vera C. Rubin Observatory Data Preview 1

Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325

We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…

gr-qc2025

Amplitude constraints on dark energy

Scott Melville

This talk gives a short introduction to the ``UV/EFT correspondence", which uses scattering amplitudes to relate the Effective Field Theory (EFT) coefficients probed by low-energy…

astro-ph.GA2025

photoD with Rubin's Data Preview 1: first stellar photometric distances and deficit of faint blue stars. Stellar distances with Rubin's DP1

L. Palaversa, E. Donev, Ž. Ivezić +96

Aims: We investigate the utility of Rubin's Data Preview 1 for estimating stellar number density profile in the Milky Way halo. Methods: Stellar broad-band near-UV to near-IR $ugri…

astro-ph.IM2025

StarDICE IV: correcting visible photometry from atmospheric gray extinction using thermal infrared observations

Kélian Sommer, Bertrand Plez, Johann Cohen-Tanugi +11

Ground-based surveys such as the Vera C. Rubin Observatory's Legacy Survey of Space and Time require photometric calibration that is both long-term stable and spatially uniform at…

astro-ph.IM2025★ 1 cited

Photometric Redshift Estimation for Rubin Observatory Data Preview 1 with Redshift Assessment Infrastructure Layers (RAIL)

T. Zhang, E. Charles, J. F. Crenshaw +87

We present the first systematic analysis of photometric redshifts (photo-z) estimated from the Rubin Observatory Data Preview 1 (DP1) data taken with the Legacy Survey of Space and…

astro-ph.IM2025

A transmission hologram for slitless spectrophotometry on a convergent telescope beam. Optimisation and characterization

Sylvie Dagoret-Campagne, Marc Moniez, Jeremy Neveu +9

This article details the optimization and the characterization of the hologram described in a companion paper published in 2021, which showed the superiority of a holographic optic…

astro-ph.HE2025

Enabling Early Transient Discovery in LSST via Difference Imaging with DECam

Yize Dong, Kaylee de Soto, V. Ashley Villar +58

We present SLIDE, a pipeline that enables transient discovery in data from the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST), using archival images from the Da…

astro-ph.IM2024

StarDICE III: Characterization of the photometric instrument with a Collimated Beam Projector

Thierry Souverin, Jérémy Neveu, Marc Betoule +18

The measurement of type Ia supernovae magnitudes provides cosmological distances, which can be used to constrain dark energy parameters. Large photometric surveys require a substan…

astro-ph.IM2024

How the StarDICE photometric calibration of standard stars can improve cosmological constraints?

T. Souverin, J. Neveu, M. Betoule +16

The number of type Ia supernova (SNe Ia) observations will grow significantly within the next decade, mainly thanks to the Legacy Survey of Space and Time (LSST) undertaken by the…

astro-ph.IM2023★ 4 cited

Slitless spectrophotometry with forward modelling: principles and application to atmospheric transmission measurement

Jérémy Neveu, Vincent Brémaud, Pierre Antilogus +9

In the next decade, many optical surveys will aim to tackle the question of dark energy nature, measuring its equation of state parameter at the permil level. This requires trustin…

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

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…

astro-ph.IM2021★ 5 cited

A transmission hologram for slitless spectrophotometry on a convergent telescope beam. 1. Focus and resolution

Marc Moniez, Jérémy Neveu, Sylvie Dagoret-Campagne +2

We report in this paper the test of a plane holographic optical element to be used as an aberration-corrected grating for a slitless spectrograph, inserted in a convergent telescop…