The MIXR sample: AGN activity versus star formation across the cross-correlation of WISE, 3XMM, and FIRST/NVSS
2016
This work has made use of data/facilities
and financial support from the ARCHES project (7th Framework of
the European Union no. 313146). SM, FJC and AR acknowledge
financial support by the Spanish Ministry of Economy and Competitiveness
through grant AYA2012-31447, which is partly funded by
the FEDER programme. FJC also acknowledges financial support
through grant AYA2015-64346-C2-1-P (MINECO/FEDER). This
work is based on observations obtained with XMM–Newton, an
ESA science mission with instruments and contributions directly
funded by ESA Member States and NASA. It also makes use of
data products from the Wide-field Infrared Survey Explorer, which
is a joint project of the University of California, Los Angeles, and
the Jet Propulsion Laboratory/California Institute of Technology,
funded by the National Aeronautics and Space Administration. We
acknowledge the use of the FIRST and NVSS catalogues, provided
by the NRAO. Optical magnitudes and redshifts were obtained
from the SDSS Data Release 12. Funding for the SDSS IV has been
provided by the Alfred P. Sloan Foundation and the Participating
Institutions. SDSS-IV acknowledges support and resources from
the Center for High-Performance Computing at the University of
Utah. The SDSS website is www.sdss.org.
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