The Sound of the Digital Global City

Madrid has been the center of Spanish musical scene and industry since the 80s, when “la movida” becomes the metaphor for the new colorful, young and cosmopolitan country established with the arrival of democracy. The city, in this way, is basically a place. But this sense of place started to crash with the arrival of digital music. In the new paradigm, intermediaries were supposed to disappear and music was something contained in networks and computers. The question now is how to integrate digital music, a nonphysical, individual experience, with the way in which the city of Madrid is lived through in musical terms. With the advent of digital music, concerts became the primary source of income for musicians. The centrality of the gig can be understood as the confirmation that we are living in an economy of experience. This centrality also reorganized the way in which music is produced and consumed: now, records are produced in order to create the opportunity of a musical event (band promote their tour as presentation of their latest recordings) that can be promoted in social networks and media; concerts are the places where musicians construct their fans’ communities and are the places were records are sold, not a way to know the band but to demonstrate both the support for the band and the status of the listeners. To study the place of music in the process of metropolization in Madrid we need to understand music as a field of tension

The SCUBA HAlf degree extragalactic survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies

Determining an accurate position for a submillimetre (submm) galaxy (SMG) is the crucial step that enables us to move from the basic properties of an SMG sample - source counts and 2D clustering - to an assessment of their detailed, multiwavelength properties, their contribution to the history of cosmic star formation and their links with present-day galaxy populations. In this paper, we identify robust radio and/or infrared (IR) counterparts, and hence accurate positions, for over two-thirds of the SCUBA HAlf-Degree Extragalactic Survey (SHADES) Source Catalogue, presenting optical, 24-μm and radio images of each SMG. Observed trends in identification rate have given no strong rationale for pruning the sample. Uncertainties in submm position are found to be consistent with theoretical expectations, with no evidence for significant additional sources of error. Employing the submm/radio redshift indicator, via a parametrization appropriate for radio-identified SMGs with spectroscopic redshifts, yields a median redshift of 2.8 for the radio-identified subset of SHADES, somewhat higher than the median spectroscopic redshift. We present a diagnostic colour-colour plot, exploiting Spitzer photometry, in which we identify regions commensurate with SMGs at very high redshift. Finally, we find that significantly more SMGs have multiple robust counterparts than would be expected by chance, indicative of physical associations. These multiple systems are most common amongst the brightest SMGs and are typically separated by 2-6 arcsec, similar to 15-20/sin i kpc at z~ 2, consistent with early bursts seen in merger simulations.