activity
20062025
most citedVOSA: Virtual Observatory SED Analyzer. An application to the Collinder 69 open cluster

604 citations · 4.1k across the 56 of their papers we have counts for

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astro-ph2008★ 604 cited

VOSA: Virtual Observatory SED Analyzer. An application to the Collinder 69 open cluster

A. Bayo, C. Rodrigo, D. Barrado y Navascues +4

The physical properties of almost any kind of astronomical object can be derived by fitting synthetic spectra or photometry extracted from theoretical models to observational data.…

astro-ph2008★ 42 cited

A deep look into the cores of young clusters I. sigma-Orionis

H. Bouy, N. Huelamo, E. L. Martin +9

Nearby young clusters are privileged places to study the star formation history. Over the last decade, the sigma-Orionis cluster has been a prime location for the study of young ve…

astro-ph2007

Cool objects: From SED fitting to age estimation

A. Bayo, D. Barrado y Navascues, M. Morales-Calderon +4

The physical properties of almost any kind of astronomical object can be derived by fitting synthetic spectra or photometry extracted from theoretical models to observational data.…

astro-ph2007★ 18 cited

The young, wide and very low mass visual binary LOri167

D. Barrado y Navascues, A. Bayo, M. Morales-Calderon +3

We look for wide, faint companions around members of the 5 Myr Lambda Orionis open cluster. We used optical, near-infrared, and Spitzer/IRAC photometry. We report the discovery of…

astro-ph2007★ 65 cited

SPITZER: Accretion in Low Mass Stars and Brown Dwarfs in the Lambda Orionis Cluster

D. Barrado y Navascues, J. R. Stauffer, M. Morales-Calderon +6

We present multi-wavelength optical and infrared photometry of 170 previously known low mass stars and brown dwarfs of the 5 Myr Collinder 69 cluster (Lambda Orionis). The new phot…

astro-ph2006★ 52 cited

A search for substellar members in the Praesepe and sigma Orionis clusters

B. M. Gonzalez-Garcia, M. R. Zapatero Osorio, V. J. S. Bejar +4

(Abridged). We have conducted deep photometric searches for substellar members of the Praesepe (0.5-1 Gyr) and sigma Orionis (3 Myr) star clusters using the Sloan i' and z' filters…