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RSS Commissioning Call

RSS Commissioning Call. Announcement : http://www.salt.ac.za/proposing/call-for-rss-commissioning-proposals / Modes: long-slit, multi-object and Fabry-Perot spectroscopy Criteria Applicability for "exercising" the respective instrument modes

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RSS Commissioning Call

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  1. RSS Commissioning Call • Announcement: • http://www.salt.ac.za/proposing/call-for-rss-commissioning-proposals/ • Modes: long-slit, multi-object and Fabry-Perot spectroscopy • Criteria • Applicability for "exercising" the respective instrument modes • Object position(s) and how well filled an observing queue will be • Practicality • Selection: Instr Team, SALT Scientist. Not “charged” • Dates • Proposal deadline: 15 Jan. Use online proposal tool PIPT 1.0 • Observations: Feb - April Galaxies Lunch

  2. SALT/ RSS • SALT features • very large aperture • good field of view (8 arcmin) • excellent ultraviolet throughput • queue scheduling • modest imaging • RSS: emphasize unique observing modes that do not require excellent imaging • UV spectroscopy down to 3200 Ǻ (rare on large telescopes) • higher resolution: high-throughput grating 3200 - 9000 Ǻ;Fabry-Perot 4300 - 9000 Ǻ (Visible Beam); later - 1.7 μm (NIR) • polarimetry (circular and linear) (very rare) • high-speed detector mode (very rare) Galaxies Lunch

  3. Optics • All-refractive UV optics for high throughput • At prime focus for UV and full-field access • NIR upgrade path: simultaneous 3200 Ǻ – 1.7 μ Galaxies Lunch

  4. Mechanisms 6-Grating Magazine Polarizing Beamsplitter(slide) 40-Slitmask Magazine 2 Fabry-Perot Etalons (slides) 3 CCD Mosaic Detector Shutter Camera Articulation 0 - 100° 2 Polarimeter Waveplates (slides) 20-Filter Magazine Galaxies Lunch

  5. RSS on SALT Detector Camera Articulation Rail Etalons Collimator Galaxies Lunch

  6. Fabry-Perot etalons (scans wavelength) Many wavelengths Perseus A in Hydrogen Light Perseus Cluster of Galaxies Imaging/ Fabry-Perot Spectroscopy Filters Galaxies Lunch

  7. Filters "VPH" Grating disperses wavelengths Up to 40 Spectra Hubble Deep Field (South) Longslit/ Multi-Object Grating Spectroscopy Slitmask selects objects Galaxies Lunch

  8. NGC 2023 = λ/Δλ High Efficiency with Volume Phase Holographic Gratings Resolution vs wavelength for 1.25 arcsec slit "Littrow": grating angle = 1/2 camera articulation Constant Efficiency Contours "Bird" NGC 6822 Galaxies Lunch

  9. Detailed Instrument Info • Website: • http://www.sal.wisc.edu/PFIS/ • Operations/Observer’s Guide • Some RSS data previously obtained: Galaxies Lunch

  10. I Hα σ v P-V Longslit Data - the "Bird" • Väisänen, et al 2008 MNRAS 384, 886. • ULIRG, z = 0.048 • grating 1800 l/mm, artic 72º, 1.5" slit: • R = 2800 5860-7150 Å • 3 slit positions • 900 – 1500 sec exposures each • Ne and CuAr arcs, 0.05 Å (2.5 km/s) accuracy Galaxies Lunch

  11. P-V High Res Data: Fluorescence in Reflection Nebulae • Nordsieck (astroph 0809:3802) in AstroPol08 • First detection of atomic fluorescence lines in neutral medium • Prepare for spectropolarimetry: geometry and magnetic field • Robert Stobie Spectrograph on SALT 11m: • NGC2023 RN, HD37903 B1.5V central star • 0.6”x8’ slit, 1st order, R = 7500 - 9500 • ~1000 Ang coverage blue, yellow, red • Many fluorescence lines found! Inner 2’ of nebula, within PDR: Galaxies Lunch

  12. MOS Test Field Courtesy: Petri Väisänen Galaxies Lunch

  13. Position Reference Stars HII and PNe MOS Test Run Spectra 4080 A 7180 A NGC6822 – Oct 20 900 l/mm grating, artic 30º, R = 1200 Galaxies Lunch

  14. Proposing • Visibility Tool • Instrument Simulator • Mask Tool • Proposal Tool Galaxies Lunch

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