| DOI | Resolve DOI: https://doi.org/10.1117/12.3020305 |
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| Author | Search for: Sivanandam, Suresh; Search for: Chapman, Scott1ORCID identifier: https://orcid.org/0000-0002-8487-3153; Search for: Muzzin, Adam; Search for: Christie, Scott; Search for: Hickson, Paul; Search for: McConnachie, Alan1ORCID identifier: https://orcid.org/0000-0003-4666-6564; Search for: Thibault, Simon; Search for: Atwood, Jenny1; Search for: Anthony, Andre1; Search for: Sawicki, Marcin1ORCID identifier: https://orcid.org/0000-0002-7712-7857; Search for: Dunn, Jennifer; Search for: Lee, Jae-Joon; Search for: Venn, Kim; Search for: Diaz, Ruben; Search for: Goodsell, Stephen; Search for: Barbod, Shawn; Search for: Tschimmel, Martin; Search for: Barnet, Mark; Search for: Hay, Gavin; Search for: Roberts, Scott1; Search for: Sivo, Gaetano; Search for: Lamb, Masen; Search for: Chen, Shaojie; Search for: Dutt, Saugata; Search for: Nkwari, Patrick; Search for: Lardière, Olivier1; Search for: Conod, Uriel1; Search for: Jeram, Sarik; Search for: Scharwächter, Julia |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Conference | Ground-based and Airborne Instrumentation for Astronomy X, June 16-22, 2024, Yokohama, Japan |
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| Subject | multi-object adaptive optics; integral field spectroscopy; near-infrared instrumentation; high angular resolution imaging; image slicer; extragalactic astronomy |
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| Abstract | The Gemini Infrared Multi-Object Spectrograph (GIRMOS) is a new facility instrument being designed in close partnership with the upcoming facility adaptive optics (AO) system at Gemini-North observatory called GNAO. GIRMOS will carry out high angular resolution (0.83 – 2.4 µm) imaging and multi-object integral field (0.95 – 2.35 µm) spectroscopy within GNAO’s two arcminute field-of-regard. GIRMOS consists of an imager and four identical deployable integral field spectrographs with a multi-object AO system that provides an additional image quality improvement for each spectrograph over GNAO across the full field. We present the final design overview of GIRMOS, which will be entering the construction phase in 2024 with an expected delivery in 2027. GIRMOS is a pathfinder for future extremely large telescope instrumentation that requires high angular resolution, highly multiplexed spectroscopy. |
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| Publication date | 2024-06-16 |
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| Publisher | SPIE |
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| In | |
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| Series | |
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| Language | English |
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| Peer reviewed | Yes |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | f4145f75-7ad3-4fd1-9a94-93f39d3d4324 |
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| Record created | 2024-12-11 |
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| Record modified | 2024-12-11 |
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