Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S304(9), p. 108-109, 2013

DOI: 10.1017/s1743921314003494

Links

Tools

Export citation

Search in Google Scholar

The Lockman Hole Project: A Multi-frequency Study of the Faint Radio Population down to LOFAR bands

Journal article published in 2013 by G. Guglielmino, I. Prandoni, R. Morganti, G. Heald ORCID, E. Mahony ORCID, I. van Bemmel
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Green circle
Postprint: archiving allowed
Red circle
Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

AbstractWe are performing a multi-frequency radio analysis of a well-known deep field: the Lockman Hole, which is one of the best studied sky regions in different wavebands. This will provide us with important complementary data (for example redshifts) to the radio data, allowing us to characterize the physical and evolutionary properties of the various classes of sources composing the faint radio population. LOFAR imaging of the Lockman Hole can play an important role in this project, allowing, for the very first time, to observe the sub-mJy source population at very low frequencies (30-200 MHz), where self-absorption phenomena are expected to be very important. Here we present some preliminary results.

Beta version