First observations with the RETICON Spectrophotometer at Cima Ekar Observatory

Details First observations with the RETICON Spectrophotometer at Cima Ekar Observatory First observations with the RETICON Spectrophotometer at Cima Ekar Observatory

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mmsai..49..673d&link_type=abstract

(Consiglio Nazionale delle Ricerche, Convegno sulle Metodologie di Trattamento dell'Informazione, Trieste, Nov. 24, 25, 1977 and

Computer Science

Performance

Astronomical Observatories, Astronomical Photometry, Spectrophotometers, Focal Plane Devices, Planetary Nebulae, Seyfert Galaxies, Stellar Spectrophotometry

Scientific paper

A new spectrophotometer has been used since August 1977 at the Cima Ekar Observatory. The system is based on a linear array of 128 photodiodes mounted at the focal plane of the grating spectrograph. This paper presents first observations performed with the spectrophotometer in order to demonstrate the performances and capabilities of the instrument. Three examples are presented: a bright star (Vega), a Seyfert galaxy (NGC 1068), and a planetary nebula (NGC 7027).

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