imacs multi-object echelle b. sutin, t. hare & a. mcwilliam & many others n *not yet...

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IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

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● Grating + Prism cross-disperser in grating module ● Grating: 245 l/mm, 37-degree blaze?,160x214mm ( 20% overfill loss) ● Prism: fused silica, 13-degree apex angle,300x200mm, 63mm base

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Page 1: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

IMACS Multi-Object Echelle

B. Sutin, T. Hare & A. McWilliam & many others

N

*Not yet released

*

Page 2: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

● IMACS Multi-Object Echelle (MOE)

F/4 focus

Page 3: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

● Grating + Prism cross-disperser in grating module

● Grating: 245 l/mm, 37-degree blaze?,160x214mm (20% overfill loss)

● Prism: fused silica, 13-degree apex angle,300x200mm, 63mm base

Page 4: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

MOE Characteristics ● Wavelength range: (10 orders)● ~10-100 objects● Resolving power (0.6 arc sec): R=21,000● Slit length: 5 arc seconds● 15x15 arc min. field● ~900 counts/pixel in 1hr at H for V~17.0

(~1400 counts/pix/hr at 7600A)● Cost: Parts~$35K, Labor~$20K

Page 5: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

10 13

4

Page 6: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

MOE Engineering

● October/November 2004

● Th-Ar lamp system installed & calibrated

● Problem #1: mechanical clash! (-3mm) IMACS model off by 9mm Solution: move prism

Page 7: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

Slide the prism down. Minimum distance now 1-2 mm.

Page 8: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

MOE Engineering● Problem #2: very tight fit

Solution: move cables & mill the prism mounting

● Problem #3: spectral clash! Design “feature” of grating roll Solution: unique software for mask cutting (empirical vs predicted)

● Problem #4: some spectra fell between CCD gaps Solution: software

Page 9: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *
Page 10: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

MOE Engineering

● Problem #5: blaze not centered on CCD Design flaw or grating blaze 3 degrees off Solution: in progress

Page 11: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

Off-center Blaze for central object

H

O2 B-band

Carina star #1386 V=17.88 (1 hour exposure)

Page 12: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

Object at edge of field

H

O2 B-band

Carina Star # 1107 V=17.79

Page 13: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

MOE Science● 1st Science/Engineering run Dec. 2004● Collaborators: A.Koch (Basel) & V.Smith (Gemini)● Carina dSph mask 20 objects 12 hrs● Fornax dSph mask 20 (10) objects 8 hrs● 4800-7800A blocking filter (4 orders)● 1st night seeing 1.1'' fwhm● Problem?: Nod & Shuffle mode

Solution: software

Page 14: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *
Page 15: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *
Page 16: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *
Page 17: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

H

EuII

NiI

FeI

FeIFeI

VI

CoI

Chip #2

Page 18: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

Procedural difficulties

● Re-alignment, after each exposure, results in a shift of the spectra on the array; requires quartz spectra to be taken each time MOE is moved.

● Number of spectra: 20 obj x 4 orders x 4 ccd x 12 exp = 3840 spectra => Pipeline reduction required

Page 19: IMACS Multi-Object Echelle B. Sutin, T. Hare & A. McWilliam & many others N *Not yet released *

Summary

● MOE works, but the blaze problem needs to be resolved.

● Pipeline reduction is essential.● MOE complements MIKE and MIKE+fibers.● MOE can compete with VLT/UVES+GIRAFFE

and enhances our ability to study the chemical evolution of nearby systems.