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

TL;DR

This paper presents the development and application of the Collimated Beam Projector (CBP) for precise calibration of the StarDICE telescope's optical throughput and filter transmissions, achieving sub-nanometer accuracy essential for cosmological measurements.

Contribution

The paper introduces a novel CBP device capable of calibrating telescope throughput and filter transmissions with sub-nanometer precision, improving calibration accuracy for supernova cosmology surveys.

Findings

Achieved sub-nanometer accuracy in filter wavelength determination

Measured filter transmission with 0.5% precision per 1nm bin

Detected out-of-band leakages at 0.01% level

Abstract

The measurement of type Ia supernovae magnitudes provides cosmological distances, which can be used to constrain dark energy parameters. Large photometric surveys require a substantial improvement in the calibration precision of their photometry to reduce systematic uncertainties in cosmological constraints. The StarDICE experiment is designed to establish accurate broadband flux references for these surveys, aiming for sub-percent precision in magnitude measurements. This requires a precise measurement of the filter bandpasses of both the StarDICE and survey instruments with sub-nanometer accuracy. To that end, we have developed the Collimated Beam Projector (CBP), an optical device capable of calibrating the throughput of an astronomical telescope and of its filters. The CBP is built from a tunable laser source and a reversed telescope to emit a parallel monochromatic light beam that is continuously monitored in flux and wavelength. The CBP output light flux is measured using a large area photodiode, previously calibrated relative to a NIST photodiode. We derive the StarDICE telescope throughput and filter transmissions from the CBP measurements, anchoring it to the absolute calibration provided by the NIST. After analyzing the systematic uncertainties, we achieved sub-nanometer accuracy in determining filter central wavelengths, measured each filter transmission with a precision of 0.5% per 1nm bin, and detected out-of-band leakages at 0.01%. Furthermore, we have synthesized the equivalent transmission for full pupil illumination from four sample positions in the StarDICE telescope mirror, with an accuracy of approximately 0.2nm for central wavelengths and 7mmag for broadband fluxes. We demonstrated our ability to characterize a telescope throughput down to the mmag, and paved the way for future developments, such as a portable CBP version for in-situ transmission monitoring.