StarDICE III: Characterization of the photometric instrument with a Collimated Beam Projector
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arXiv
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| Autori principali: | , , , , , , , , , , , , , , , , , , , , |
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| Natura: | Preprint |
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2024
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| author | Souverin, Thierry Neveu, Jérémy Betoule, Marc Bongard, Sébastien Stubbs, Christopher W. Urbach, Elana Brownsberger, Sasha Blanc, Pierre Éric Tanugi, Johann Cohen Dagoret-Campagne, Sylvie Feinstein, Fabrice Hardin, Delphine Juramy, Claire Guillou, Laurent Le Van Suu, Auguste Le Moniez, Marc Plez, Bertrand Regnault, Nicolas Sepulveda, Eduardo Sommer, Kélian Collaboration, the LSST Dark Energy Science |
| author_facet | Souverin, Thierry Neveu, Jérémy Betoule, Marc Bongard, Sébastien Stubbs, Christopher W. Urbach, Elana Brownsberger, Sasha Blanc, Pierre Éric Tanugi, Johann Cohen Dagoret-Campagne, Sylvie Feinstein, Fabrice Hardin, Delphine Juramy, Claire Guillou, Laurent Le Van Suu, Auguste Le Moniez, Marc Plez, Bertrand Regnault, Nicolas Sepulveda, Eduardo Sommer, Kélian Collaboration, the LSST Dark Energy Science |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_24173 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | StarDICE III: Characterization of the photometric instrument with a Collimated Beam Projector Souverin, Thierry Neveu, Jérémy Betoule, Marc Bongard, Sébastien Stubbs, Christopher W. Urbach, Elana Brownsberger, Sasha Blanc, Pierre Éric Tanugi, Johann Cohen Dagoret-Campagne, Sylvie Feinstein, Fabrice Hardin, Delphine Juramy, Claire Guillou, Laurent Le Van Suu, Auguste Le Moniez, Marc Plez, Bertrand Regnault, Nicolas Sepulveda, Eduardo Sommer, Kélian Collaboration, the LSST Dark Energy Science Instrumentation and Methods for Astrophysics 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. |
| title | StarDICE III: Characterization of the photometric instrument with a Collimated Beam Projector |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2410.24173 |