M. Vitale
Max Planck Society
14 Papers
21 Citations
M. Vitale is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Radio galaxy. The author has an hindex of 6, co-authored 12 publications. Previous affiliations of M. Vitale include University of Cologne.
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Papers
Classifying radio emitters from the Sloan Digital Sky Survey - Spectroscopy and diagnostics
M. Vitale,Jens Zuther,Macarena Garcia-Marin,Andreas Eckart,M. N. Bremer,Monica Valencia-S.,Anton Zensus +6 more
TL;DR: In this paper, a cross-correlation of the SDSS data release 7 (DR7) with the Very Large Array (VLA) survey Faint Images of the Radio Sky at Twenty-centimeters (FIRST) makes it possible to conduct a joined multiwavelength statistical study of radio-optical galaxy properties on a very large number of sources.
High-resolution observations of SDSS J080800.99+483807.7 in the optical and radio domains. A possible example of jet-triggered star formation
Y. E. Rashed,Y. E. Rashed,Jens Zuther,Andreas Eckart,Andreas Eckart,Gerold Busch,Monica Valencia-S.,M. Vitale,M. Vitale,Silke Britzen,T. W. B. Muxlow +10 more
TL;DR: In this article, the authors derived the main physical properties of SDSS J080800.99+483807.7 and studied the possible interaction between the radio jets and the interstellar medium of the host galaxy.
A low-luminosity type-1 QSO sample; III. Optical spectroscopic properties and activity classification
Evangelia Tremou,Evangelia Tremou,Macarena Garcia-Marin,Jens Zuther,Andreas Eckart,Andreas Eckart,M. Valencia-Schneider,M. Vitale,M. Vitale,C. Shan +9 more
TL;DR: In this paper, optical spectroscopic analysis of a sample of 99 low-luminosity quasi-stellar objects (LLQSOs) at 0.06$ base the Hamburg/ESO QSO survey (HES) is presented.
Classifying Radio Emitters from the Sloan Digital Sky Survey: Spectroscopy and Diagnostics
M. Vitale,Jens Zuther,Macarena Garcia-Marin,Andreas Eckart,M. N. Bremer,Monica Valencia-S.,Anton Zensus +6 more
TL;DR: In this paper, a cross-correlation of the SDSS DR7 with the FIRST radio survey makes it possible to conduct a joined multiwavelength statistical study of radio-optical galaxy properties on a very large number of sources.