FMOS: Fiber Multi Object Spectrograph

ATTENTION: In S10A and S10B, FMOS will be operated in a shared-risk mode. Observers will be only allowed to use IRS1 in the Low Resolution (LR) mode.

Introduction

FMOS is a fiber-fed multi-object spectrograph. The Echidna fiber positioner system configures 400 fibers with an accuracy of 0.2" rms in the 30-arcmin diamter field of view at the Subaru prime focus and these fibers are extracted as spectra by the two spectrographs (IRS1 & IRS2). A mask mirror is installed in these spectrographs for OH airglow suppression (OHS). The spectral coverage is from 0.9 μm to 1.8 μm. This is observed at one exposure entirely with R=500 in the Low Resolution (LR) mode, while it is divided into four parts ("J-short", "J-long", "H-short" & "H-long") with a ~0.2 μm coverage and one of them is observed at one exposure with R=2200 in the High Resolution (HR) mode.

Contents

Further information

Questions regarding these pages should be directed to Naoyuki Tamura. Please note that all numbers on these pages are subject to change as the characteristics and performance of FMOS are better determined.

References

Readers can also refer to the papers as listed below and references therein for more details of this instrument:
"FMOS: the fiber multiple-object spectrograph: Part VI. Onboard performances and results of the engineering observations"
Iwamuro, F. et al. 2008, Proc. of SPIE, Vol. 7014, 26
"Performance of Echidna fiber positioner for FMOS on Subaru"
Akiyama, M., et al. 2008, Proc. of SPIE, Vol. 7018, 94
"Echidna: the engineering challenges"
Brzeski, J., et al. 2004, Proc. of SPIE, Vol. 5492, 1228
"FMOS: the Fibre Multi-Object Spectrograph: Part VII. Results of PIR engineering run"
Kimura, M., et al., 2008, Proc. of SPIE, Vol. 7014, 185
"Integration, commissioning, and performance of the UK FMOS spectrograph"
Dalton, G., et al. 2008, Proc. of SPIE, Vol. 7014, 127
"Design and construction of the fibre system for FMOS"
Murray, G., et al. 2008, Proc. of SPIE, Vol. 7014, 186
"Cryogenic tests of volume-phase holographic gratings: results at 100 K"
Tamura, N. et al. 2006, Applied Optics, Vol. 45, 5923

Last updated: February 13, 2010



Copyright© 2000-200Subaru Telescope, NAOJ. All rights reserved.