High-angular resolution and high-contrast VLTI observations from Y to L band with the Asgard instrumental suite Article Swipe
Marc-Antoine Martinod
,
Denis Defrère
,
Michael Ireland
,
Stefan Kraus
,
Frantz Martinache
,
Peter Tuthill
,
Azzurra Bigioli
,
Julia J. Bryant
,
Sorabh Chhabra
,
Benjamin Courtney-Barrer
,
Fred Crous
,
Nick Cvetojevic
,
Colin Dandumont
,
Germain Garreau
,
Tiphaine Lagadec
,
Romain Laugier
,
Daniel J. Mortimer
,
Barnaby Norris
,
Gordon L. Robertson
,
Adam Taras
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2301.06518
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2301.06518
The Very Large Telescope Interferometer is one of the most proficient observatories in the world for high angular resolution. Since its first observations, it has hosted several interferometric instruments operating in various bandwidths in the infrared. As a result, the VLTI has yielded countless discoveries and technological breakthroughs. Here, we introduce a new concept for the VLTI, Asgard: an instrumental suite comprised of four natively collaborating instruments: BIFROST, a combiner whose main science case is studying the formation processes and properties of stellar and planetary systems; NOTT, a nulling interferometer dedicated to imaging young nearby planetary systems in the L band; HEIMDALLR, an all-in-one instrument performing both fringe tracking and stellar interferometry with the same optics; Baldr, a Strehl optimiser. These instruments share common goals and technologies. The goals are diverse astrophysical cases such as the study of the formation and evolution processes of binary systems, exoplanetary systems and protoplanetary disks, the characterization of orbital parameters and spin-orbit alignment of multiple systems, the characterization of the exoplanets, and the study of exozodiacal disks. Thus, the idea of this suite is to make the instruments interoperable and complementary to deliver unprecedented sensitivity and accuracy from the J to M bands to meet these goals. The interoperability of the Asgard instruments and their integration in the VLTI are major challenges for this project.
Related Topics
Concepts
Metadata
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2301.06518
- https://arxiv.org/pdf/2301.06518
- OA Status
- green
- Cited By
- 1
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4317462012
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4317462012Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.48550/arxiv.2301.06518Digital Object Identifier
- Title
-
High-angular resolution and high-contrast VLTI observations from Y to L band with the Asgard instrumental suiteWork title
- Type
-
preprintOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2023Year of publication
- Publication date
-
2023-01-16Full publication date if available
- Authors
-
Marc-Antoine Martinod, Denis Defrère, Michael Ireland, Stefan Kraus, Frantz Martinache, Peter Tuthill, Azzurra Bigioli, Julia J. Bryant, Sorabh Chhabra, Benjamin Courtney-Barrer, Fred Crous, Nick Cvetojevic, Colin Dandumont, Germain Garreau, Tiphaine Lagadec, Romain Laugier, Daniel J. Mortimer, Barnaby Norris, Gordon L. Robertson, Adam TarasList of authors in order
- Landing page
-
https://arxiv.org/abs/2301.06518Publisher landing page
- PDF URL
-
https://arxiv.org/pdf/2301.06518Direct link to full text PDF
- Open access
-
YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
-
https://arxiv.org/pdf/2301.06518Direct OA link when available
- Concepts
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Exoplanet, Interferometry, Angular resolution (graph drawing), Suite, Very Large Telescope, Physics, Planet, Astronomy, Astronomical interferometer, Planetary system, Telescope, Interoperability, Remote sensing, Computer science, Geology, Stars, Operating system, Mathematics, Archaeology, Combinatorics, HistoryTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
1Total citation count in OpenAlex
- Citations by year (recent)
-
2024: 1Per-year citation counts (last 5 years)
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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