Publication type: Refereed

  • Publication
    SPIDER - I. Sample and galaxy parameters in the grizYJHK wavebands
    This is the first paper of a series presenting the Spheroids Panchromatic Investigation in Different Environmental Regions (SPIDER). The sample of spheroids...
  • Publication
    SPIDER - II. The Fundamental Plane of early-type galaxies in grizYJHK
    We present a complete analysis of the Fundamental Plane (FP) of early-type galaxies (ETGs) in the nearby Universe (z 0.1). The sample, as defined in Paper I...
  • Publication
    SPIDER - III. Environmental dependence of the Fundamental Plane of early-type galaxies
    We analyse the Fundamental Plane (FP) relation of 39993 early-type galaxies (ETGs) in the optical (griz) and 5080 ETGs in the near-infrared (NIR; YJHK)...
  • Publication
    SPIDER - X. Environmental effects in central and satellite early-type galaxies through the stellar fossil record
    A detailed analysis of how environment affects the star formation history of early-type galaxies (ETGs) is undertaken via high signal-to-noise ratio stacked...
  • Publication
    SPIDER VIII - constraints on the stellar initial mass function of early-type galaxies from a variety of spectral features
    We perform a spectroscopic study to constrain the stellar initial mass function (IMF) by using a large sample of 24 781 early-type galaxies from the Sloan...
  • Publication
    Spider-Webb: JWST Near Infrared Camera resolved galaxy star formation and nuclear activities in the Spiderweb protocluster at z = 2.16
    Near-infrared (NIR) emission is less affected by dust than ultraviolet and optical emission and is therefore useful for studying the properties of dust-obscured...
  • Publication
    Spider. IV. Optical and Near-infrared Color Gradients in Early-type Galaxies: New Insight into Correlations with Galaxy Properties
    We present an analysis of stellar population gradients in 4546 early-type galaxies (ETGs) with photometry in grizYHJK along with optical spectroscopy. ETGs were...
  • Publication
    Spin alignment of dark matter haloes in the shells of the largest voids
    Using the high-resolution cosmological N-body simulation MareNostrum universe we study the orientation of shape and angular momentum of galaxy-size dark matter...
  • Publication
    Spin alignment of stars in old open clusters
    Stellar clusters form by gravitational collapse of turbulent molecular clouds, with up to several thousand stars per cluster1. They are thought to be the...