Presentation + Paper
28 August 2024 GRAVITY+ Wide: towards hundreds of z ∼ 2 AGN, larger throughput and improved vibrational control
Author Affiliations +
Abstract
In the GRAVITY+ project, GRAVITY is presently undergoing a series of upgrades to enhance its performance, add wide field capability and thereby expand its sky coverage. Some aspects of these improvements have already been implemented and commissioned by the end of 2021, making them accessible to the community. The augmentation of sky coverage involves increasing the maximum angular separation between the celestial science object and the fringe tracking object from the previous 2 arcseconds (limited by the field of view of the VLTI) to 20 – 30 arcseconds (constrained by atmospheric conditions during observation). Phase 1 of GRAVITY+ Wide utilizes the earlier PRIMA Differential Delay Lines to compensate for the optical path length variation between the science and fringe tracking beams throughout an observation. In phase 2, we are upgrading the existing beam compressors (BC) to integrate optical path length difference compensation directly into the BC. This modification eliminates five optical reflections per beam, thereby enhancing the optical throughput of the VLTI–GRAVITY system and the bandwidth of the vibrational control. We will present the implementation of phase 2 and share preliminary results from our testing activities for GRAVITY+ Wide.
Conference Presentation
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Maximilian Fabricius, Julien Woillez, Roberto Abuter, Guillaume Bourdarot, Pierre Bourget, Wolfgang Brandner, Amit Brara, Denis Defrère, Antonia Drescher, Frank Eisenhauer, Helmut Feuchtgruber, Robert Frahm, Reinhard Genzel, Stefan Gillessen, Frédéric Gonté, Vishaal Gopinath, Jonas Graf, Michael Hartl, Frank Haußmann, Sebastian F. Hönig, Matthew Horrobin, Paulo J. V. Garcia, Tilo Jilg, Laura Kreidberg, Romain Laugier, Jean-Baptiste Le Bouquin, Mari Lena Bolzer, Dieter Lutz, Nikhil More, Thomas Ott, Hakan Özdemir, Thibaut Paumard, Karine Perraut, Guy Perrin, Christian Rau, Christian Rehm, Jonas Sauter, Nicolas Schuhler, Daniel Schuppe, Jinyi Shangguan, Taro Shimizu, Christian Straubmeier, Matthias Subroweit, Sinem Uysal, Patrick Wessely, Felix Widmann, Ekkehard Wieprecht, Lukas Wimmer, Senol Yazici, Hagen Prowatke, and Ralf Böttcher "GRAVITY+ Wide: towards hundreds of z ∼ 2 AGN, larger throughput and improved vibrational control", Proc. SPIE 13095, Optical and Infrared Interferometry and Imaging IX, 130950B (28 August 2024); https://doi.org/10.1117/12.3019984
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Control systems

Beam path

Mirrors

Vibration

Optical benches

Telescopes

Vibration control

RELATED CONTENT

E-ELT vibration modeling, simulation, and budgeting
Proceedings of SPIE (July 05 2016)
HIRDLS functional performance in orbit: a summary
Proceedings of SPIE (September 13 2005)
Imaging beyond the fringe an update on the LINC...
Proceedings of SPIE (July 21 2010)
Design of a space telescope for vibration control
Proceedings of SPIE (October 04 1994)
Secondary mirror chopping system for large infrared telescope
Proceedings of SPIE (February 01 1992)

Back to Top