Poster
19 July 2024 GNIRS integral field spectroscopy modes: on-sky performance
Rubén J. Díaz, Mark G. Rawlings, Ray M. Sharples, Emanuele P. Farina, Brian C. Lemaux, Andrew W. Stephens, Damián Mast, John White, Eduardo Tapia, Ariadna Calcines, Cornelis M. Dubbeldam, Jennifer Miller, Cyril J. Bourgenot, David A. Ryder, Ken Parkin, Paul A. White, Turner E. H. James, Thomas R. Geballe, Hawi Stecher, Jennifer E. Andrews, Zachary D. Hartman, Hyewon Suh, Siyi Xu, Cicero X. Lu, Natalia McCarthy
Author Affiliations +
Conference Poster
Abstract
We report the commissioning progress and on-sky performance of two new integral field units (IFUs) for the Gemini Near-Infrared Spectrograph (GNIRS). The commissioning of these modes opens up new scientific opportunities for spatially resolved spectroscopy on Gemini. The IFUs were designed and built at the Centre for Advanced Instrumentation in Durham University, as part of Gemini’s Instrument Upgrade Program. The Low Resolution IFU (LR-IFU) has a field-of-view of 3.15" x 4.80" sampled with a pixel scale of 0.15”It currently covers the X,J,H, and K bands with a spectral resolution of R~1700−7200 depending on the grating. The High Resolution IFU (HR-IFU) has a 1.80" x 1.25" field-of-view at a 0.05” sampling, and is optimized for fully adaptively corrected images delivered by the Gemini North ALTAIR AO system.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rubén J. Díaz, Mark G. Rawlings, Ray M. Sharples, Emanuele P. Farina, Brian C. Lemaux, Andrew W. Stephens, Damián Mast, John White, Eduardo Tapia, Ariadna Calcines, Cornelis M. Dubbeldam, Jennifer Miller, Cyril J. Bourgenot, David A. Ryder, Ken Parkin, Paul A. White, Turner E. H. James, Thomas R. Geballe, Hawi Stecher, Jennifer E. Andrews, Zachary D. Hartman, Hyewon Suh, Siyi Xu, Cicero X. Lu, and Natalia McCarthy "GNIRS integral field spectroscopy modes: on-sky performance", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 1309629 (19 July 2024); https://doi.org/10.1117/12.3020524
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