Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Jagiellonian Uniwersity
OAUJ, Poland
Jagiellonian Univ.
Jagiellonian University
Astronomical Observatory of the Jagiellonian Univerity, Krakow
Jagiellonian University, Cracow, Poland
Jagiellonian University, Poland
Obserwatorium Astronomiczne Uniwersytetu Jagellonskiego, Krakow
Astronomical Observatory, Jagiellonian University
Jagiellonian Univ, Cracow, Poland
Astronomical Observatory, Jagiellonian University, Poland
Uniwersytet Jagiellonski, Krakow
Astronomical Observatory, Jagellonian University, ul. Orla 171, 30244 Cracow, Poland Astronomiczne, Krakow, Poland
Krakow, Uniwersytet, Obserwatorium Astronomiczne, Poland
National Radio Astronomy Observatory, Charlottesville, VA; Obserwatorium Astronomiczne, Krakow, Poland
Obserwatorium Astronomiczne, Krakow, Poland
Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla 171, 30244 Kraków, Poland
Observatorium Astronomiczne, Krakow, Poland; National Radio Astronomy Observatory, Charlottesville, VA
Obserwatorium Astronomiczne, Uniwersytet Jagiellonski, ul. Orla 171, 30-244 Krakow, Poland
Obserwatorium Astronomiczne, Krakow, Poland; National Radio Astronomy Observatory, Charlottesville, VA
National Radio Astronomy Observatory, Green Bank, W. Va; Obserwatorium Astronomiczne, Krakow, Poland
Astronomical Observatory, Jagiellonian University, ul. Orla 171
National Radio Astronomy Observatory, Charlottesville, VA; Krakow, Uniwersytet, Krakow, Poland
Astronomical Observatory, Krakow, Poland
Jagiellonian University, Astronomical Observatory, ul. Orla 171, 30-244 Cracow, Poland
1.4 GHz luminosity function of galaxies in the Las Campanas redshift survey and its evolution
1.4-GHz Luminosity Function of Galaxies from the Las Campanas Redshift Survey
1308 + 328 : a new highly variable extragalactic object
1308+328 - a New Highly Variable Extragalactic Object
A complete sample of intermediate-strength radio sources selected from the GB/GB2 1400-MHz surveys. I - Radio spectra and optical identifications of sources stronger than 0.55 Jy
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