TY  - GEN 
AU  - Miret-Roig, N.
AU  - Bouy, H.
AU  - Olivares, J.
AU  - Sarro, L.M.
AU  - Tamura, M.
AU  - Allen, L.
AU  - Bertin, E.
AU  - Serre, S.
AU  - Berihuete Macías, Ángel
AU  - Beletsky, Y.
AU  - Barrado, D.
AU  - Huélamo, N.
AU  - Cuillandre, J.-C.
AU  - Moraux, E.
AU  - Bouvier, J.
A4  - Estadística e Investigación Operativa
PY  - 2019
SN  - 0004-6361
SN  - 1432-0746
UR  - http://hdl.handle.net/10498/22000
AB  - Context. The study of star formation is extremely challenging, due to the lack of complete and clean samples of young nearby clusters
and star-forming regions. The recent Gaia DR2 catalogue complemented with the deep ground-based COSMIC DANCe...
LA  - eng
PB  - EDP SCIENCES S A
KW  - proper motions
KW  - stars: luminosity function, mass function
KW  - mass function
KW  - open clusters and associations: individual: IC 4665
KW  - stars: low-mass
TI  - IC 4665 DANCe I. Members, empirical isochrones, magnitude distributions, present-day system mass function, and spatial distribution
DO  - 10.1051/0004-6361/201935518
ER  -