Deriving stellar parameters from GALANTE photometry: bias and precision
2020
We thank the Centro de Estudios de F´isica del Cosmos de Aragon´
(CEFCA) team in Teruel and Javalambre for supporting us in this
project, giving us the opportunity to use non-J-PLUS useful nights to
develop the GALANTE survey. We also want to recognize the work
of the NGSL team (Gregg et al. 2006; Heap & Lindler 2016) whose
observational catalogue has been of great help for our work. This
research made use of PYTHON (http://www.python.org); NUMPY (van
der Walt, Colbert & Varoquaux 2011); SCIPY (Jones et al. 2001);
and MATPLOTLIB (Hunter 2007), a suite of open-source PYTHON
modules that provides a framework for creating scientific plots. We
also acknowledge the use of STILTS and TOPCAT tools (Taylor
2005). AL-G, EJA, and JMA acknowledge support from the Spanish
Government Ministerio de Ciencia, Innovacion y Universidades ´
though grants AYA2013-40 611-P and AYA2016-75 931-C2-1/2-P.
AL-G and EJA also acknowledge support from the State Agency for
Research of the Spanish MCIU through the ‘Center of Excellence
Severo Ochoa’ award for the Instituto de Astrof´isica de Andaluc´ia
(SEV-2017-0709).
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