Abstract
We present FLEX, an instrument to demonstrate the power of fibre Bragg grating OH suppression. This ground breaking technology promises great gains in sensitivity for near infrared instrumentation and the time is now right for a pioneer instrument to prove the effectiveness of the technique. Our proposal is for an adaptive optics fed integral field unit for an 8 metre class telescope. We envisage a 61 element IFU with 0.22" sampling and a 2.2" field of view. J and H-band OH suppression units would cleanly suppress the atmospheric emission lines,effectively lowering the sky background by 3 or 4 magnitudes respectively. The capabilities of FLEX will make it ideal for deep Epoch of Reionisation studies, as well as studies of star formation at z ̃1-4. To enable rapid and economical deployment FLEX would use an existing near infrared spectrograph with R ≈ 1000 and employ facility adaptive optics.
| Language | English |
|---|---|
| Title of host publication | Ground-based and Airborne Instrumentation for Astronomy II |
| Editors | Ian S. McLean, Mark M. Casali |
| Publisher | SPIE |
| Pages | 1-8 |
| Number of pages | 8 |
| Volume | 7014 |
| ISBN (Electronic) | 9780819472243 |
| DOIs | |
| Publication status | Published - 1 Dec 2008 |
| Externally published | Yes |
| Event | Ground-based and Airborne Instrumentation for Astronomy II - Marseille, France Duration: 23 Jun 2008 → 28 Jun 2008 |
Conference
| Conference | Ground-based and Airborne Instrumentation for Astronomy II |
|---|---|
| Country | France |
| City | Marseille |
| Period | 23/06/08 → 28/06/08 |
Fingerprint
Keywords
- Adaptive optics
- Fibre Bragg grating
- FLEX
- Integral field spectroscopy
- Near infrared
- OH suppression
- Photonic lantern
Cite this
}
FLEX-the first light explorer : A pathfinder instrument for fibre Bragg grating OH suppression. / Horton, Anthony J.; Ellis, Simon C.; Bland-Hawthorn, Joss; Haynes, Roger; McGrath, Andrew J.
Ground-based and Airborne Instrumentation for Astronomy II. ed. / Ian S. McLean; Mark M. Casali. Vol. 7014 SPIE, 2008. p. 1-8 701435.Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › Research › peer-review
TY - GEN
T1 - FLEX-the first light explorer
T2 - A pathfinder instrument for fibre Bragg grating OH suppression
AU - Horton, Anthony J.
AU - Ellis, Simon C.
AU - Bland-Hawthorn, Joss
AU - Haynes, Roger
AU - McGrath, Andrew J.
PY - 2008/12/1
Y1 - 2008/12/1
N2 - We present FLEX, an instrument to demonstrate the power of fibre Bragg grating OH suppression. This ground breaking technology promises great gains in sensitivity for near infrared instrumentation and the time is now right for a pioneer instrument to prove the effectiveness of the technique. Our proposal is for an adaptive optics fed integral field unit for an 8 metre class telescope. We envisage a 61 element IFU with 0.22" sampling and a 2.2" field of view. J and H-band OH suppression units would cleanly suppress the atmospheric emission lines,effectively lowering the sky background by 3 or 4 magnitudes respectively. The capabilities of FLEX will make it ideal for deep Epoch of Reionisation studies, as well as studies of star formation at z ̃1-4. To enable rapid and economical deployment FLEX would use an existing near infrared spectrograph with R ≈ 1000 and employ facility adaptive optics.
AB - We present FLEX, an instrument to demonstrate the power of fibre Bragg grating OH suppression. This ground breaking technology promises great gains in sensitivity for near infrared instrumentation and the time is now right for a pioneer instrument to prove the effectiveness of the technique. Our proposal is for an adaptive optics fed integral field unit for an 8 metre class telescope. We envisage a 61 element IFU with 0.22" sampling and a 2.2" field of view. J and H-band OH suppression units would cleanly suppress the atmospheric emission lines,effectively lowering the sky background by 3 or 4 magnitudes respectively. The capabilities of FLEX will make it ideal for deep Epoch of Reionisation studies, as well as studies of star formation at z ̃1-4. To enable rapid and economical deployment FLEX would use an existing near infrared spectrograph with R ≈ 1000 and employ facility adaptive optics.
KW - Adaptive optics
KW - Fibre Bragg grating
KW - FLEX
KW - Integral field spectroscopy
KW - Near infrared
KW - OH suppression
KW - Photonic lantern
UR - http://www.scopus.com/inward/record.url?scp=66249110824&partnerID=8YFLogxK
U2 - 10.1117/12.788629
DO - 10.1117/12.788629
M3 - Conference proceeding contribution
VL - 7014
SP - 1
EP - 8
BT - Ground-based and Airborne Instrumentation for Astronomy II
A2 - McLean, Ian S.
A2 - Casali, Mark M.
PB - SPIE
ER -