Journal: Monthly Notices of the Royal Astronomical Society

  • Publication
    Spectroscopy of the optical counterpart to Ser X-1
    We present William Herschel Telescope (WHT) and Very Large Telescope (VLT) spectroscopy of MM Ser, the optical counterpart to Ser X-1. We deblend the red...
  • Publication
    Spectrum analysis of bright Kepler late B- to early F-stars
    The Kepler satellite mission was designed to search for transiting exoplanets and delivers single band-pass light curves of a huge number of stars observed in...
  • 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
    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...