This HTML5 document contains 42 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
n18http://linked.opendata.cz/ontology/domain/vavai/riv/typAkce/
dctermshttp://purl.org/dc/terms/
n9http://localhost/temp/predkladatel/
n8http://purl.org/net/nknouf/ns/bibtex#
n14http://linked.opendata.cz/resource/domain/vavai/projekt/
n12http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n17http://linked.opendata.cz/ontology/domain/vavai/
shttp://schema.org/
rdfshttp://www.w3.org/2000/01/rdf-schema#
skoshttp://www.w3.org/2004/02/skos/core#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n21http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F68407700%3A21230%2F14%3A00224057%21RIV15-MSM-21230___/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n15http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n7http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n16http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n13http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n20http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n19http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n10http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F68407700%3A21230%2F14%3A00224057%21RIV15-MSM-21230___
rdf:type
skos:Concept n17:Vysledek
rdfs:seeAlso
http://www.astroscu.unam.mx/rmaa/RMxAC..45/PDF/RMxAC..45_file7-02.pdf
dcterms:description
We present and discuss the role of robotic telescopes including GLORIA network in high–energy astrophysics, as well as related strategies. Numerous satellite projects focus on high energy astrophysics from X-rays to gamma-rays, however, a large fraction of objects of high-energy astrophysics emits also optical light, which is, in many cases, variable. The observation of these sources at optical wavelengths can provide valuable inputs for multispectral analysis of various categories of celestial high-energy (HE) sources. The magnitudes of numerous objects are bright and can be hence accessed by robotic ground-based observatories, hence these observations can contribute to investigations and analyses of HE sources. In addition to direct imaging, the Low dispersive spectroscopy (LDS) represent important optional strategy for RTs, taking into account the results from past extended LDS surveys with photographic telescopes/plates. We present and discuss the role of robotic telescopes including GLORIA network in high–energy astrophysics, as well as related strategies. Numerous satellite projects focus on high energy astrophysics from X-rays to gamma-rays, however, a large fraction of objects of high-energy astrophysics emits also optical light, which is, in many cases, variable. The observation of these sources at optical wavelengths can provide valuable inputs for multispectral analysis of various categories of celestial high-energy (HE) sources. The magnitudes of numerous objects are bright and can be hence accessed by robotic ground-based observatories, hence these observations can contribute to investigations and analyses of HE sources. In addition to direct imaging, the Low dispersive spectroscopy (LDS) represent important optional strategy for RTs, taking into account the results from past extended LDS surveys with photographic telescopes/plates.
dcterms:title
The Role of Robotic Telescopes and GLORIA in High Energy Astrophysics: Imaging And LDS Spectroscopy The Role of Robotic Telescopes and GLORIA in High Energy Astrophysics: Imaging And LDS Spectroscopy
skos:prefLabel
The Role of Robotic Telescopes and GLORIA in High Energy Astrophysics: Imaging And LDS Spectroscopy The Role of Robotic Telescopes and GLORIA in High Energy Astrophysics: Imaging And LDS Spectroscopy
skos:notation
RIV/68407700:21230/14:00224057!RIV15-MSM-21230___
n3:aktivita
n13:P
n3:aktivity
P(7E12074), P(GA13-33324S), P(GC13-39464J)
n3:dodaniDat
n10:2015
n3:domaciTvurceVysledku
n12:8998558
n3:druhVysledku
n19:D
n3:duvernostUdaju
n7:S
n3:entitaPredkladatele
n21:predkladatel
n3:idSjednocenehoVysledku
43180
n3:idVysledku
RIV/68407700:21230/14:00224057
n3:jazykVysledku
n16:eng
n3:klicovaSlova
telescopes; spectroscopy; surveys
n3:klicoveSlovo
n15:telescopes n15:surveys n15:spectroscopy
n3:kontrolniKodProRIV
[740DE7FAC872]
n3:mistoKonaniAkce
Torremolinos
n3:mistoVydani
México
n3:nazevZdroje
III Workshop on Robotic Autonomous Observatories
n3:obor
n20:JA
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
1
n3:projekt
n14:7E12074 n14:GC13-39464J n14:GA13-33324S
n3:rokUplatneniVysledku
n10:2014
n3:tvurceVysledku
Hudec, René
n3:typAkce
n18:WRD
n3:zahajeniAkce
2013-10-07+02:00
s:issn
1405-2059
s:numberOfPages
4
n8:hasPublisher
Universidad Nacional Autónoma de México
n9:organizacniJednotka
21230