PEPSI

PEPSI

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  • Overview
  • Description
    • General
    • PFU
    • Spectrograph
    • Polarimeter
    • Calibration unit
  • Users
    • About
    • Observing modes
    • User manual for PEPSI PFU
    • Data reduction
    • Current technical status
    • Wiki
    • Exposure Time Calculator
  • SDI
  • VATT
    • Overview
    • Installation of the VATT adapter
    • Observing with VATT
    • The VATT-PEPSI-TESS survey
  • Library
    • Paper I: The Sun as a star
    • Paper II: Gaia benchmark stars and other M-K standards
    • Paper III: Kepler-444
    • WallPosters
  • News
    • All news
    • Publications
    • Announcements
    • First light
    • Technical Notes
  • Contact

Contact

PESPI team group photo (2013).
PESPI team group photo (2013).

The P.I. of PEPSI is Prof. Dr. Klaus G. Strassmeier.  The project scientist is Dr. Ilya Ilyin, and the instrument scientist is Dr. Michael Weber. While PEPSI is a PI instrument at LBT, the point of contact for users is the P.I.

AIP instrument page

Latest news

  • Mono-enriched stars and Galactic chemical evolution — Possible biases in observations and theory October 1, 2020
  • Pepsi Exoplanet Transit Survey Workshop September 7, 2020
  • On the Chemical Abundance of HR 8799 and the Planet c September 3, 2020
  • Benchmark stars, benchmark spectrographs: Detailed spectroscopic comparison of ESPRESSO, PEPSI, and HARPS data for Gaia benchmark stars August 31, 2020
  • Probing the atmosphere of HD 189733b with the Na I and K I spectral lines August 31, 2020

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