Precision single mode fibre integral field spectroscopy with the RHEA spectrograph

Adam D. Rains; Michael J. Ireland; Nemanja Jovanovic; Tobias Feger; Joao Bento; Christian Schwab; David W. Coutts; Olivier Guyon; Alexander Arriola; Simon Gross

doi:10.1117/12.2233743

Precision single mode fibre integral field spectroscopy with the RHEA spectrograph

Adam D. Rains, Michael J. Ireland, Nemanja Jovanovic, Tobias Feger, Joao Bento, Christian Schwab, David W. Coutts, Olivier Guyon, Alexander Arriola, Simon Gross

Optical Sciences

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

27 Scopus citations

Abstract

The RHEA Spectrograph is a single-mode echelle spectrograph designed to be a replicable and cost effective method of undertaking precision radial velocity measurements. Two versions of RHEA currently exist, one located at the Australian National University in Canberra, Australia (450 - 600nm wavelength range), and another located at the Subaru Telescope in Hawaii, USA (600 - 800 nm wavelength range). Both instruments have a novel fibre feed consisting of an integral field unit injecting light into a 2D grid of single mode fibres. This grid of fibres is then reformatted into a 1D array at the input of the spectrograph (consisting of the science fibres and a reference fibre capable of receiving a white-light or xenon reference source for simultaneous calibration). The use of single mode fibres frees RHEA from the issue of modal noise and significantly reduces the size of the optics used. In addition to increasing the overall light throughput of the system, the integral field unit allows for cutting edge science goals to be achieved when operating behind the 8.2m Subaru Telescope and the SCExAO adaptive optics system. These include, but are not limited to: resolved stellar photospheres; resolved protoplanetary disk structures; resolved Mira shocks, dust and winds; and sub-arcsecond companions. We present details and results of early tests of RHEA@Subaru and progress towards the stated science goals.

Original language	English (US)
Title of host publication	Ground-Based and Airborne Instrumentation for Astronomy VI
Editors	Luc Simard, Christopher J. Evans, Hideki Takami
Publisher	SPIE
ISBN (Electronic)	9781510601956
DOIs	https://doi.org/10.1117/12.2233743
State	Published - 2016
Event	Ground-Based and Airborne Instrumentation for Astronomy VI - Edinburgh, United Kingdom Duration: Jun 26 2016 → Jun 30 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9908
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Ground-Based and Airborne Instrumentation for Astronomy VI
Country/Territory	United Kingdom
City	Edinburgh
Period	6/26/16 → 6/30/16

Keywords

Difraction-limited spectrograph
Fiber injection
High resolution
Integral-field unit
Optical fibers
Radial Velocity
Spectrograph

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2233743

Cite this

Rains, A. D., Ireland, M. J., Jovanovic, N., Feger, T., Bento, J., Schwab, C., Coutts, D. W., Guyon, O., Arriola, A., & Gross, S. (2016). Precision single mode fibre integral field spectroscopy with the RHEA spectrograph. In L. Simard, C. J. Evans, & H. Takami (Eds.), Ground-Based and Airborne Instrumentation for Astronomy VI Article 990876 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9908). SPIE. https://doi.org/10.1117/12.2233743

Precision single mode fibre integral field spectroscopy with the RHEA spectrograph. / Rains, Adam D.; Ireland, Michael J.; Jovanovic, Nemanja et al.
Ground-Based and Airborne Instrumentation for Astronomy VI. ed. / Luc Simard; Christopher J. Evans; Hideki Takami. SPIE, 2016. 990876 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9908).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Rains, AD, Ireland, MJ, Jovanovic, N, Feger, T, Bento, J, Schwab, C, Coutts, DW, Guyon, O, Arriola, A & Gross, S 2016, Precision single mode fibre integral field spectroscopy with the RHEA spectrograph. in L Simard, CJ Evans & H Takami (eds), Ground-Based and Airborne Instrumentation for Astronomy VI., 990876, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9908, SPIE, Ground-Based and Airborne Instrumentation for Astronomy VI, Edinburgh, United Kingdom, 6/26/16. https://doi.org/10.1117/12.2233743

Rains AD, Ireland MJ, Jovanovic N, Feger T, Bento J, Schwab C et al. Precision single mode fibre integral field spectroscopy with the RHEA spectrograph. In Simard L, Evans CJ, Takami H, editors, Ground-Based and Airborne Instrumentation for Astronomy VI. SPIE. 2016. 990876. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2233743

@inproceedings{00e9770c0758450bbc878f1bf04cef4d,

title = "Precision single mode fibre integral field spectroscopy with the RHEA spectrograph",

abstract = "The RHEA Spectrograph is a single-mode echelle spectrograph designed to be a replicable and cost effective method of undertaking precision radial velocity measurements. Two versions of RHEA currently exist, one located at the Australian National University in Canberra, Australia (450 - 600nm wavelength range), and another located at the Subaru Telescope in Hawaii, USA (600 - 800 nm wavelength range). Both instruments have a novel fibre feed consisting of an integral field unit injecting light into a 2D grid of single mode fibres. This grid of fibres is then reformatted into a 1D array at the input of the spectrograph (consisting of the science fibres and a reference fibre capable of receiving a white-light or xenon reference source for simultaneous calibration). The use of single mode fibres frees RHEA from the issue of modal noise and significantly reduces the size of the optics used. In addition to increasing the overall light throughput of the system, the integral field unit allows for cutting edge science goals to be achieved when operating behind the 8.2m Subaru Telescope and the SCExAO adaptive optics system. These include, but are not limited to: resolved stellar photospheres; resolved protoplanetary disk structures; resolved Mira shocks, dust and winds; and sub-arcsecond companions. We present details and results of early tests of RHEA@Subaru and progress towards the stated science goals.",

keywords = "Difraction-limited spectrograph, Fiber injection, High resolution, Integral-field unit, Optical fibers, Radial Velocity, Spectrograph",

author = "Rains, {Adam D.} and Ireland, {Michael J.} and Nemanja Jovanovic and Tobias Feger and Joao Bento and Christian Schwab and Coutts, {David W.} and Olivier Guyon and Alexander Arriola and Simon Gross",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Ground-Based and Airborne Instrumentation for Astronomy VI ; Conference date: 26-06-2016 Through 30-06-2016",

year = "2016",

doi = "10.1117/12.2233743",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Luc Simard and Evans, {Christopher J.} and Hideki Takami",

booktitle = "Ground-Based and Airborne Instrumentation for Astronomy VI",

}

TY - GEN

T1 - Precision single mode fibre integral field spectroscopy with the RHEA spectrograph

AU - Rains, Adam D.

AU - Ireland, Michael J.

AU - Jovanovic, Nemanja

AU - Feger, Tobias

AU - Bento, Joao

AU - Schwab, Christian

AU - Coutts, David W.

AU - Guyon, Olivier

AU - Arriola, Alexander

AU - Gross, Simon

PY - 2016

Y1 - 2016

N2 - The RHEA Spectrograph is a single-mode echelle spectrograph designed to be a replicable and cost effective method of undertaking precision radial velocity measurements. Two versions of RHEA currently exist, one located at the Australian National University in Canberra, Australia (450 - 600nm wavelength range), and another located at the Subaru Telescope in Hawaii, USA (600 - 800 nm wavelength range). Both instruments have a novel fibre feed consisting of an integral field unit injecting light into a 2D grid of single mode fibres. This grid of fibres is then reformatted into a 1D array at the input of the spectrograph (consisting of the science fibres and a reference fibre capable of receiving a white-light or xenon reference source for simultaneous calibration). The use of single mode fibres frees RHEA from the issue of modal noise and significantly reduces the size of the optics used. In addition to increasing the overall light throughput of the system, the integral field unit allows for cutting edge science goals to be achieved when operating behind the 8.2m Subaru Telescope and the SCExAO adaptive optics system. These include, but are not limited to: resolved stellar photospheres; resolved protoplanetary disk structures; resolved Mira shocks, dust and winds; and sub-arcsecond companions. We present details and results of early tests of RHEA@Subaru and progress towards the stated science goals.

AB - The RHEA Spectrograph is a single-mode echelle spectrograph designed to be a replicable and cost effective method of undertaking precision radial velocity measurements. Two versions of RHEA currently exist, one located at the Australian National University in Canberra, Australia (450 - 600nm wavelength range), and another located at the Subaru Telescope in Hawaii, USA (600 - 800 nm wavelength range). Both instruments have a novel fibre feed consisting of an integral field unit injecting light into a 2D grid of single mode fibres. This grid of fibres is then reformatted into a 1D array at the input of the spectrograph (consisting of the science fibres and a reference fibre capable of receiving a white-light or xenon reference source for simultaneous calibration). The use of single mode fibres frees RHEA from the issue of modal noise and significantly reduces the size of the optics used. In addition to increasing the overall light throughput of the system, the integral field unit allows for cutting edge science goals to be achieved when operating behind the 8.2m Subaru Telescope and the SCExAO adaptive optics system. These include, but are not limited to: resolved stellar photospheres; resolved protoplanetary disk structures; resolved Mira shocks, dust and winds; and sub-arcsecond companions. We present details and results of early tests of RHEA@Subaru and progress towards the stated science goals.

KW - Difraction-limited spectrograph

KW - Fiber injection

KW - High resolution

KW - Integral-field unit

KW - Optical fibers

KW - Radial Velocity

KW - Spectrograph

UR - http://www.scopus.com/inward/record.url?scp=84996676229&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84996676229&partnerID=8YFLogxK

U2 - 10.1117/12.2233743

DO - 10.1117/12.2233743

M3 - Conference contribution

AN - SCOPUS:84996676229

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Ground-Based and Airborne Instrumentation for Astronomy VI

A2 - Simard, Luc

A2 - Evans, Christopher J.

A2 - Takami, Hideki

PB - SPIE

T2 - Ground-Based and Airborne Instrumentation for Astronomy VI

Y2 - 26 June 2016 through 30 June 2016

ER -

Precision single mode fibre integral field spectroscopy with the RHEA spectrograph

Abstract

Publication series

Other

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this