Superdense Massive Galaxies in the Nearby Universe
Superdense massive galaxies (re ~ 1 kpc; M ~ 1011 M sun) were common in the early universe (z gsim 1.5). Within some hierarchical merging scenarios, a non...
Surface brightness fluctuations to constrain secondary stellar populations: revealing very low-metallicity stars in massive galaxies
The aim of this work is to explore the potential of surface brightness fluctuations (SBF) for studying composite stellar populations (CSP). To do so, we have...
Surface Rotation and Photometric Activity for Kepler Targets. II. G and F Main-sequence Stars and Cool Subgiant Stars
Dark magnetic spots crossing the stellar disk lead to quasiperiodic brightness variations, which allow us to constrain stellar surface rotation and photometric...
We present the SWIRE Photometric Redshift Catalogue 1 025 119 redshifts of unprecedented reliability and of accuracy comparable with or better than previous...
The SWIRE Photometric Redshift Catalogue consists of 1025119 sources, split between the SWIRE fields as follows: EN1 (218117), EN2 (125364), Lockman (229238)...
Coordinates, redshifts, SDSS (ugriz) and 2MASS (JHK) photometry, IRAC and MIPS fluxes for the 278 SWIRE/SDSS quasars in the SWIRE EN1, EN2 and Lockman fields...
Coordinates, redshifts, SDSS (ugriz) and 2MASS (JHK) photometry, IRAC and MIPS fluxes for the 278 SWIRE/SDSS quasars in the SWIRE EN1, EN2 and Lockman fields...
Testing Microvariability in Quasar Differential Light Curves Using Several Field Stars
Microvariability consists of small timescale variations of low amplitude in the photometric light curves of quasars and represents an important tool to...