BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Opening Session
DTSTART;VALUE=DATE-TIME:20171106T083000Z
DTEND;VALUE=DATE-TIME:20171106T090000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5305@indico.ific.uv.es
DESCRIPTION:Speakers: Carmen Vela Olmo (Secretary of State of I+D+i (MINEC
 O))\, Emilio Lora-Tamayo (President of CSIC)\, Esteban MORCILLO SANCHEZ (R
 ector of the University of Valencia)\, Juan Jose Hernandez (IFIC)\, Lourde
 s Verdes-Montenegro (Coordinator of the Spanish participation in SKA (IAA-
 CSIC))\, Vicent Martínez (RIA Coordinator (Observatori Astrònomic\, UV))
 \nhttps://indico.ific.uv.es/event/3046/contributions/5305/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5305/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Concluding remarks
DTSTART;VALUE=DATE-TIME:20171107T143000Z
DTEND;VALUE=DATE-TIME:20171107T150000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5304@indico.ific.uv.es
DESCRIPTION:Speakers: Jesús Martín-Pintado (RIA Radioastronomy Infrastru
 ctures Coordinator (INTA-CAB-CSIC))\, Jose Carlos Guirado (Observatori Ast
 ronòmic Director\, UV)\, Lourdes Verdes-Montenegro (Coordinator of the Sp
 anish participation in the SKA (IAA-CSIC))\nhttps://indico.ific.uv.es/even
 t/3046/contributions/5304/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5304/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Fundamental Physics with Pulsars
DTSTART;VALUE=DATE-TIME:20171107T130000Z
DTEND;VALUE=DATE-TIME:20171107T133000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5303@indico.ific.uv.es
DESCRIPTION:Speakers: Jason Hessels ()\nPulsars have proven to be unique a
 nd powerful laboratories for studying fundamental physics.  In this talk\,
  I will describe how SKA can deliver the next breakthroughs by discovering
  a large fraction of the Galactic pulsar population and thereby finding th
 e ultimate `pulsar laboratories' for testing gravitational theories\, prob
 ing the dense matter equation of state\, and studying neutron star magneto
 spheres.\n\nhttps://indico.ific.uv.es/event/3046/contributions/5303/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5303/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Dark Matter annihilation and the 21 cm signal
DTSTART;VALUE=DATE-TIME:20171107T110000Z
DTEND;VALUE=DATE-TIME:20171107T113000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5301@indico.ific.uv.es
DESCRIPTION:Speakers: Laura lopez Honorez (VUB)\nhttps://indico.ific.uv.es
 /event/3046/contributions/5301/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5301/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Weighing neutrinos with HI
DTSTART;VALUE=DATE-TIME:20171107T113000Z
DTEND;VALUE=DATE-TIME:20171107T120000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5300@indico.ific.uv.es
DESCRIPTION:Speakers: FRANCISCO VILLAESCUSA (Center for Computational Astr
 ophysics\, NY\, US)\nI will show the impact of neutrino masses on the abun
 dance and clustering properties of cosmic neutral hydrogen\, that we have 
 studied through high-resolution hydrodynamic simulations. I will point out
  that their effect can be understood taking into account the signatures ne
 utrinos leave of halo properties. I will also present some forecasts showi
 ng that 21cm data from SKA can be used to place very competitive bounds on
  the sum of the neutrino masses.\n\nhttps://indico.ific.uv.es/event/3046/c
 ontributions/5300/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5300/
END:VEVENT
BEGIN:VEVENT
SUMMARY:SKA and the Epoch of Reionization
DTSTART;VALUE=DATE-TIME:20171107T103000Z
DTEND;VALUE=DATE-TIME:20171107T110000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5298@indico.ific.uv.es
DESCRIPTION:Speakers: Jordi Miranda-Escudé (ICREA & IEC\, UB\, Spain)\nOb
 servations in the 21-cm line can probe different phases of\nreionization: 
 an initial one where the atomic medium is cold and is seen in\nabsorption 
 at the highest redshifts\, and the later signal of 21-cm emission\nfrom a 
 heated medium before it is ionized. The emission signal is the easier\none
  to observe in upcoming years\, and it can arise from low-density regions\
 nthat are less ionized than high-density ones\, but also from high-density
  clumps\nthat are more abundant in high-density regions\, associated with 
 sites of galaxy formation that can be observed also as damped Lyman alpha 
 absorbers.\nCross-correlation studies with other sources and emission line
 s will be\nessential to understand the origin of the 21-cm signal when it 
 is detected.\n\nhttps://indico.ific.uv.es/event/3046/contributions/5298/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5298/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The potential of SKA to  detect the thermal emission of distant So
 lar System objects
DTSTART;VALUE=DATE-TIME:20171107T090000Z
DTEND;VALUE=DATE-TIME:20171107T093000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5297@indico.ific.uv.es
DESCRIPTION:Speakers: Pablo Santos Sanz (IAA/CSIC\, Spain)\nThe feasibilit
 y of SKA to measure the thermal emission of distant and cold Solar System 
 objects\, such as Trans-Neptunian objects (TNOs) and Centaurs\, is investi
 gated in terms of the different wavelengths and expected sensitivities. Th
 ese thermal measurements would allow to obtain information\, via thermal o
 r thermophysical modeling\, of sizes\, albedos and thermal properties of T
 NOs and Centaurs. The results that can be obtained with SKA are complement
 ary and extend those obtained by the Herschel Space Observatory within its
  observing key programme called 'TNOs are Cool: a survey of the transneptu
 nian region' from which we derived sizes\, albedos and thermal properties 
 of 140 distant Solar System objects.\n\nhttps://indico.ific.uv.es/event/30
 46/contributions/5297/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5297/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Radio Continuum Surveys of Feedback in Galaxies
DTSTART;VALUE=DATE-TIME:20171106T150000Z
DTEND;VALUE=DATE-TIME:20171106T153000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5295@indico.ific.uv.es
DESCRIPTION:Speakers: Fatemeh Tabatabaei (IAC/CSIC\, Spain)\nhttps://indic
 o.ific.uv.es/event/3046/contributions/5295/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5295/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Transient Universe with the Square Kilometer Array
DTSTART;VALUE=DATE-TIME:20171107T083000Z
DTEND;VALUE=DATE-TIME:20171107T090000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5294@indico.ific.uv.es
DESCRIPTION:Speakers: Miguel Angel Pérez-Torres (IAA/CSIC\, Spain)\nThe S
 KA as currently designed will be a ground-breaking facility for \nradio tr
 ansient studies.  I will give an overview of the possibilities for transie
 nt and variable-source astrophysics with the Square Kilometre Array.  I wi
 ll focus on a few scientific topics that will highlight to aspects that ma
 y result in a dramatic increase of the scientific return: the addition of 
 near-real-time commensal searches of data streams for events\, and (ii) ra
 pid robotic response to Target-of-Opprtunity like triggers\n\nhttps://indi
 co.ific.uv.es/event/3046/contributions/5294/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5294/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Cosmic magnetism
DTSTART;VALUE=DATE-TIME:20171106T140000Z
DTEND;VALUE=DATE-TIME:20171106T143000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5293@indico.ific.uv.es
DESCRIPTION:Speakers: KUNZE KERSTIN (Universidad de Salamanca\, Spain)\nMa
 gnetic fields are observed on nearly all scales in the universe\, from sta
 rs and galaxies upto galaxy clusters and even beyond. The origin of cosmic
  magnetic fields is still an open question\, however a large class of mode
 ls puts its origin in the very early universe. Observations of the CMB\, L
 SS and 21 cm line can be used to constrain the magnetic field parameters.\
 n\nhttps://indico.ific.uv.es/event/3046/contributions/5293/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5293/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Extragalactic continuum
DTSTART;VALUE=DATE-TIME:20171106T143000Z
DTEND;VALUE=DATE-TIME:20171106T150000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5292@indico.ific.uv.es
DESCRIPTION:Speakers: Antxon Alberdi (IAA/CSIC\, Spain)\nhttps://indico.if
 ic.uv.es/event/3046/contributions/5292/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5292/
END:VEVENT
BEGIN:VEVENT
SUMMARY:HI and Galaxy evolution Science
DTSTART;VALUE=DATE-TIME:20171106T113000Z
DTEND;VALUE=DATE-TIME:20171106T120000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5291@indico.ific.uv.es
DESCRIPTION:Speakers: Lourdes VERDES-MONTENEGRO (IAA/CSIC\, Spain)\nhttps:
 //indico.ific.uv.es/event/3046/contributions/5291/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5291/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Science Synergies between SKA\, CTA and Athena
DTSTART;VALUE=DATE-TIME:20171106T133000Z
DTEND;VALUE=DATE-TIME:20171106T140000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5290@indico.ific.uv.es
DESCRIPTION:Speakers: Ivan Agudo (IAA/CSIC\, Spain)\nhttps://indico.ific.u
 v.es/event/3046/contributions/5290/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5290/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Using SKA to decipher the chemical and granulometric distribution 
 of dust in protoplanetary disks\, to be compared with the chondrite eviden
 ce
DTSTART;VALUE=DATE-TIME:20171106T103000Z
DTEND;VALUE=DATE-TIME:20171106T110000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5289@indico.ific.uv.es
DESCRIPTION:Speakers: Josep TRIGO-RODRIGUEZ (IEEC/CSIC\, Spain)\nhttps://i
 ndico.ific.uv.es/event/3046/contributions/5289/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5289/
END:VEVENT
BEGIN:VEVENT
SUMMARY:SKA and the Cradle of Life
DTSTART;VALUE=DATE-TIME:20171106T110000Z
DTEND;VALUE=DATE-TIME:20171106T113000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5288@indico.ific.uv.es
DESCRIPTION:Speakers: Izaskun Jimenez Serra (Queen Mary University of Lond
 on\, UK)\nIn this talk I will provide a review of the current activities a
 nd future\nplans of the Cradle of Life working group. The deployment of th
 e high\nfrequency Band 5 receivers of the SKA will enable key science in t
 he field\nof planet formation and Astrobiology. While the unprecedented hi
 gh-angular\nresolution of SKA1-Mid will allow to image the thermal emissio
 n of\ncentimetre-sized dust particles across the water snow line in nearby
 \nsystems\, its improved sensitivity with respect to current instrumentati
 on\nwill allow us to search for pre-biotic species such as formamide in\np
 roto-planetary disks and planet-sized fragments. On the other hand\, the\n
 low frequency capabilities of SKA-Low can be used to study the magnetic\nf
 ields of exolanets via their auroral synchrotron emission\, which can\npro
 vide information about their internal structure. These low frequency\nobse
 rvations will also enable commensal SETI searches of technologically\nadva
 nced signals down to levels of typical airport radars.\n\nhttps://indico.i
 fic.uv.es/event/3046/contributions/5288/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5288/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Overview of the Square Kilometre Array
DTSTART;VALUE=DATE-TIME:20171106T090000Z
DTEND;VALUE=DATE-TIME:20171106T093000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5287@indico.ific.uv.es
DESCRIPTION:Speakers: Philip J. Diamond (SKA Director General (University 
 of Manchester))\nhttps://indico.ific.uv.es/event/3046/contributions/5287/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5287/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Spanish participation in the SKA
DTSTART;VALUE=DATE-TIME:20171106T093000Z
DTEND;VALUE=DATE-TIME:20171106T100000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5286@indico.ific.uv.es
DESCRIPTION:Speakers: LOURDES VERDES-MONTENEGRO (IAA/CSIC\, Spain)\nhttps:
 //indico.ific.uv.es/event/3046/contributions/5286/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5286/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Unveiling the reionization epoch using CMB Stage IV multifrequency
  data
DTSTART;VALUE=DATE-TIME:20171106T132000Z
DTEND;VALUE=DATE-TIME:20171106T133000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5285@indico.ific.uv.es
DESCRIPTION:Speakers: Carlos Hernández-Monteagudo (CEFCA)\nhttps://indico
 .ific.uv.es/event/3046/contributions/5285/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5285/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Radio synchtrotron spectra of star forming galaxies
DTSTART;VALUE=DATE-TIME:20171106T131000Z
DTEND;VALUE=DATE-TIME:20171106T132000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5284@indico.ific.uv.es
DESCRIPTION:Speakers: Ute Lisenfeld (University of Granada)\nhttps://indic
 o.ific.uv.es/event/3046/contributions/5284/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5284/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Probing the neutral gas reservoir with current and future HI galax
 y surveys
DTSTART;VALUE=DATE-TIME:20171106T130500Z
DTEND;VALUE=DATE-TIME:20171106T131000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5283@indico.ific.uv.es
DESCRIPTION:Speakers: Michael Jones (IAA - CSIC)\nhttps://indico.ific.uv.e
 s/event/3046/contributions/5283/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5283/
END:VEVENT
BEGIN:VEVENT
SUMMARY:WDM and the Ionization History of the Universe
DTSTART;VALUE=DATE-TIME:20171106T130000Z
DTEND;VALUE=DATE-TIME:20171106T130500Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5282@indico.ific.uv.es
DESCRIPTION:Speakers: Pablo Villanueva Domingo (IFIC/CSIC-UV)\nhttps://ind
 ico.ific.uv.es/event/3046/contributions/5282/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5282/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Cosmology with radio continuum and HI galaxy surveys\, and synergi
 es with CMB probes
DTSTART;VALUE=DATE-TIME:20171107T093000Z
DTEND;VALUE=DATE-TIME:20171107T100000Z
DTSTAMP;VALUE=DATE-TIME:20261012T162104Z
UID:indico-contribution-3046-5281@indico.ific.uv.es
DESCRIPTION:Speakers: Diego Herranz (Instituto de Física de Cantabria)\nh
 ttps://indico.ific.uv.es/event/3046/contributions/5281/
LOCATION:Universe Salon Actos
URL:https://indico.ific.uv.es/event/3046/contributions/5281/
END:VEVENT
END:VCALENDAR
