Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph

Simon Ellis; Joss Bland-Hawthorn; Anthony Horton; Roger Haynes

doi:10.1007/978-1-4020-9190-2_79

Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph

Simon Ellis^*, Joss Bland-Hawthorn, Anthony Horton, Roger Haynes

^*Corresponding author for this work

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

1 Citation (Scopus)

Abstract

The ability to achieve deep near infrared spectroscopy is of great importance to the future of astronomy. Our understanding of the early Universe depends on our ability to observe highly redshifted spectroscopic diagnostic features. Observations of H-α at wavelengths 0.9≤λ≤1.8 μm would allow accurate star-formation rates to be measured over the period 0.4≤z≤1.7—a crucial period in the formation of galaxies. Observations of Lyman-α at the same wavelengths would probe 6≤z≤13—the epoch at which the Universe underwent a major (and poorly understood) phase change from neutral to ionised. Similarly our understanding of low mass stars and unbound planets relies on NIR spectroscopy, since these objects emit most of their light at NIR wavelengths.

Original language	English
Title of host publication	Science with the VLT in the ELT era
Editors	Alan Moorwood
Place of Publication	Dordrecht ; London
Publisher	Springer, Springer Nature
Pages	437-441
Number of pages	5
ISBN (Electronic)	9781402091902
ISBN (Print)	9781402091896
DOIs	https://doi.org/10.1007/978-1-4020-9190-2_79
Publication status	Published - 2009
Externally published	Yes
Event	Workshop on Science with the VLT in the ELT Era, 2007 - Garching, Germany Duration: 8 Oct 2007 → 12 Oct 2007

Publication series

Name	Astrophysics and Space Science Proceedings
ISSN (Print)	1570-6591

Conference

Conference	Workshop on Science with the VLT in the ELT Era, 2007
Country	Germany
City	Garching
Period	8/10/07 → 12/10/07

Keywords

Fibre Bragg Grating
Near Infrared Spectroscopy
Crucial Period
Large Core Diameter
Excite Hydroxyl Radical

Access to Document

10.1007/978-1-4020-9190-2_79

Link to publication in Scopus

Fingerprint Dive into the research topics of 'Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph'. Together they form a unique fingerprint.

Cite this

@inproceedings{c751a6e14415434b9bf27672eacb26e6,

title = "Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph",

abstract = "The ability to achieve deep near infrared spectroscopy is of great importance to the future of astronomy. Our understanding of the early Universe depends on our ability to observe highly redshifted spectroscopic diagnostic features. Observations of H-α at wavelengths 0.9≤λ≤1.8 μm would allow accurate star-formation rates to be measured over the period 0.4≤z≤1.7—a crucial period in the formation of galaxies. Observations of Lyman-α at the same wavelengths would probe 6≤z≤13—the epoch at which the Universe underwent a major (and poorly understood) phase change from neutral to ionised. Similarly our understanding of low mass stars and unbound planets relies on NIR spectroscopy, since these objects emit most of their light at NIR wavelengths.",

keywords = "Fibre Bragg Grating, Near Infrared Spectroscopy, Crucial Period, Large Core Diameter, Excite Hydroxyl Radical",

author = "Simon Ellis and Joss Bland-Hawthorn and Anthony Horton and Roger Haynes",

year = "2009",

doi = "10.1007/978-1-4020-9190-2_79",

language = "English",

isbn = "9781402091896",

series = "Astrophysics and Space Science Proceedings",

publisher = "Springer, Springer Nature",

pages = "437--441",

editor = "Alan Moorwood",

booktitle = "Science with the VLT in the ELT era",

address = "United States",

note = "Workshop on Science with the VLT in the ELT Era, 2007 ; Conference date: 08-10-2007 Through 12-10-2007",

}

Ellis, S, Bland-Hawthorn, J, Horton, A & Haynes, R 2009, Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph. in A Moorwood (ed.), Science with the VLT in the ELT era. Astrophysics and Space Science Proceedings, Springer, Springer Nature, Dordrecht ; London, pp. 437-441, Workshop on Science with the VLT in the ELT Era, 2007, Garching, Germany, 8/10/07. https://doi.org/10.1007/978-1-4020-9190-2_79

Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph. / Ellis, Simon; Bland-Hawthorn, Joss; Horton, Anthony; Haynes, Roger.

Science with the VLT in the ELT era. ed. / Alan Moorwood. Dordrecht ; London : Springer, Springer Nature, 2009. p. 437-441 (Astrophysics and Space Science Proceedings).

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

TY - GEN

T1 - Flex (The first light explorer)—the science case for a fully OH suppressed IFU spectrograph

AU - Ellis, Simon

AU - Bland-Hawthorn, Joss

AU - Horton, Anthony

AU - Haynes, Roger

PY - 2009

Y1 - 2009

N2 - The ability to achieve deep near infrared spectroscopy is of great importance to the future of astronomy. Our understanding of the early Universe depends on our ability to observe highly redshifted spectroscopic diagnostic features. Observations of H-α at wavelengths 0.9≤λ≤1.8 μm would allow accurate star-formation rates to be measured over the period 0.4≤z≤1.7—a crucial period in the formation of galaxies. Observations of Lyman-α at the same wavelengths would probe 6≤z≤13—the epoch at which the Universe underwent a major (and poorly understood) phase change from neutral to ionised. Similarly our understanding of low mass stars and unbound planets relies on NIR spectroscopy, since these objects emit most of their light at NIR wavelengths.

AB - The ability to achieve deep near infrared spectroscopy is of great importance to the future of astronomy. Our understanding of the early Universe depends on our ability to observe highly redshifted spectroscopic diagnostic features. Observations of H-α at wavelengths 0.9≤λ≤1.8 μm would allow accurate star-formation rates to be measured over the period 0.4≤z≤1.7—a crucial period in the formation of galaxies. Observations of Lyman-α at the same wavelengths would probe 6≤z≤13—the epoch at which the Universe underwent a major (and poorly understood) phase change from neutral to ionised. Similarly our understanding of low mass stars and unbound planets relies on NIR spectroscopy, since these objects emit most of their light at NIR wavelengths.

KW - Fibre Bragg Grating

KW - Near Infrared Spectroscopy

KW - Crucial Period

KW - Large Core Diameter

KW - Excite Hydroxyl Radical

UR - http://www.scopus.com/inward/record.url?scp=85034627999&partnerID=8YFLogxK

U2 - 10.1007/978-1-4020-9190-2_79

DO - 10.1007/978-1-4020-9190-2_79

M3 - Conference proceeding contribution

AN - SCOPUS:85034627999

SN - 9781402091896

T3 - Astrophysics and Space Science Proceedings

SP - 437

EP - 441

BT - Science with the VLT in the ELT era

A2 - Moorwood, Alan

PB - Springer, Springer Nature

CY - Dordrecht ; London

T2 - Workshop on Science with the VLT in the ELT Era, 2007

Y2 - 8 October 2007 through 12 October 2007

ER -