Science, ISSN 0036-8075, 07/2018, Volume 361, Issue 6398, p. eaat1378
Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of...
ORIGIN | TELESCOPE | SPECTROGRAPH | PERFORMANCE | MULTIDISCIPLINARY SCIENCES | Sky | Red shift | Atmospheric models | Gravitational waves | Spatial discrimination | Luminosity | Emission | Activation | Cosmic radiation | Cosmic rays | Energy | Radio sources (astronomy) | Cooperation | Neutrinos | Gravity | Fluctuations | Statistical analysis | Electromagnetic radiation | Blazars | Universe | Photons | Line of sight | Relativistic effects | Emissions | Gamma rays | Observatories | X rays | Wavelengths | Collaboration | Telescopes | Relativism | Acceleration | Astronomy | Tracers | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
ORIGIN | TELESCOPE | SPECTROGRAPH | PERFORMANCE | MULTIDISCIPLINARY SCIENCES | Sky | Red shift | Atmospheric models | Gravitational waves | Spatial discrimination | Luminosity | Emission | Activation | Cosmic radiation | Cosmic rays | Energy | Radio sources (astronomy) | Cooperation | Neutrinos | Gravity | Fluctuations | Statistical analysis | Electromagnetic radiation | Blazars | Universe | Photons | Line of sight | Relativistic effects | Emissions | Gamma rays | Observatories | X rays | Wavelengths | Collaboration | Telescopes | Relativism | Acceleration | Astronomy | Tracers | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Astroparticle Physics, ISSN 0927-6505, 03/2013, Volume 43, Issue SI, pp. 3 - 18
The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to...
Cherenkov Telescopes | TeV gamma-ray astronomy | Air showers | TELESCOPE | ASTRONOMY | MISSION | ASTRONOMY & ASTROPHYSICS | EMISSION | HESS | SUPERNOVA REMNANT W44 | PHYSICS, PARTICLES & FIELDS | Gamma rays | Sciences of the Universe | Astrophysics | Physics | Instrumentation and Methods for Astrophysic | High Energy Astrophysical Phenomena | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Cherenkov Telescopes | TeV gamma-ray astronomy | Air showers | TELESCOPE | ASTRONOMY | MISSION | ASTRONOMY & ASTROPHYSICS | EMISSION | HESS | SUPERNOVA REMNANT W44 | PHYSICS, PARTICLES & FIELDS | Gamma rays | Sciences of the Universe | Astrophysics | Physics | Instrumentation and Methods for Astrophysic | High Energy Astrophysical Phenomena | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 10/2017, Volume 848, Issue 2, p. L12
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational...
OPTICAL AFTERGLOWS | NEARBY SUPERNOVA RATES | GRAVITATIONAL-WAVES | PULSAR PSR-1913+16 | COMPACT OBJECTS | gravitational waves | RADIO TELESCOPE | CLOSE BINARIES | GAMMA-RAY BURSTS | stars: neutron | RELATIVISTIC GRAVITY | BLACK-HOLES | Stars: neutron | Gravitational waves | GAMMA-RAY BURST | AFTERGLOW | PULSAR | EVOLUTION | ASTRONOMY & ASTROPHYSICS | REDSHIFT | IMAGER | NUCLEOSYNTHESIS | HOST GALAXY | Astrofísica | Astrophysics | Ones gravitacionals | Astronomia i astrofísica | Astronomia | Raigs gamma | Astronomy | Àrees temàtiques de la UPC | Física | Gamma ray astronomy | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
OPTICAL AFTERGLOWS | NEARBY SUPERNOVA RATES | GRAVITATIONAL-WAVES | PULSAR PSR-1913+16 | COMPACT OBJECTS | gravitational waves | RADIO TELESCOPE | CLOSE BINARIES | GAMMA-RAY BURSTS | stars: neutron | RELATIVISTIC GRAVITY | BLACK-HOLES | Stars: neutron | Gravitational waves | GAMMA-RAY BURST | AFTERGLOW | PULSAR | EVOLUTION | ASTRONOMY & ASTROPHYSICS | REDSHIFT | IMAGER | NUCLEOSYNTHESIS | HOST GALAXY | Astrofísica | Astrophysics | Ones gravitacionals | Astronomia i astrofísica | Astronomia | Raigs gamma | Astronomy | Àrees temàtiques de la UPC | Física | Gamma ray astronomy | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 06/2015, Volume 578, p. A22
Context. Because of its proximity, Mrk 421 is one of the best sources on which to study the nature of BL Lac objects. Its proximity allows us to characterize...
Radiation mechanisms: non-thermal | Galaxies: active | Gamma rays: galaxies | BL Lacertae objects: individual: Mrk 421 | radiation mechanisms: non-thermal | SELF-COMPTON MODEL | ENERGY-SPECTRUM | TEV BLAZARS | LARGE-AREA TELESCOPE | EXTRAGALACTIC BACKGROUND LIGHT | SPECTRAL VARIABILITY | SIMULTANEOUS MULTIWAVELENGTH OBSERVATIONS | ELECTRON ACCELERATION | galaxies: active | ASTRONOMY & ASTROPHYSICS | X-RAY | LAC OBJECTS | gamma rays: galaxies | Proximity | Broadband | Synchrotrons | Spectral energy distribution | Evolution | Mathematical models | Physical properties | Astronomy | Physics - High Energy Astrophysical Phenomena | Active galaxies | Gamma rays | Galàxies actives | Raigs gamma | ASTRONOMY AND ASTROPHYSICS
Radiation mechanisms: non-thermal | Galaxies: active | Gamma rays: galaxies | BL Lacertae objects: individual: Mrk 421 | radiation mechanisms: non-thermal | SELF-COMPTON MODEL | ENERGY-SPECTRUM | TEV BLAZARS | LARGE-AREA TELESCOPE | EXTRAGALACTIC BACKGROUND LIGHT | SPECTRAL VARIABILITY | SIMULTANEOUS MULTIWAVELENGTH OBSERVATIONS | ELECTRON ACCELERATION | galaxies: active | ASTRONOMY & ASTROPHYSICS | X-RAY | LAC OBJECTS | gamma rays: galaxies | Proximity | Broadband | Synchrotrons | Spectral energy distribution | Evolution | Mathematical models | Physical properties | Astronomy | Physics - High Energy Astrophysical Phenomena | Active galaxies | Gamma rays | Galàxies actives | Raigs gamma | ASTRONOMY AND ASTROPHYSICS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A31
Aims. We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15...
BL Lacertae objects: individual: Markarian 501 | Methods: data analysis | BL-LACERTAE | methods: data analysis | TEV BLAZARS | EMITTING ELECTRONS | EXTRAGALACTIC BACKGROUND LIGHT | STOCHASTIC ACCELERATION | GAMMA-RAY EMISSION | ASTRONOMY & ASTROPHYSICS | X-RAY | MULTIWAVELENGTH OBSERVATIONS | SPECTRAL ENERGY-DISTRIBUTION | TELESCOPE OBSERVATIONS | Polarization | Correlation | Parameters | Broadband | Computer simulation | Data acquisition | Emission analysis | Variability | X-ray emissions | Electron energy distribution | Blazars | Rotation | Emissions | Optical polarization | Observatories | X rays | Wavelengths | Energy bands | Correlation analysis | Correlation function | Mathematical models | Electron energy | Physics - High Energy Astrophysical Phenomena
BL Lacertae objects: individual: Markarian 501 | Methods: data analysis | BL-LACERTAE | methods: data analysis | TEV BLAZARS | EMITTING ELECTRONS | EXTRAGALACTIC BACKGROUND LIGHT | STOCHASTIC ACCELERATION | GAMMA-RAY EMISSION | ASTRONOMY & ASTROPHYSICS | X-RAY | MULTIWAVELENGTH OBSERVATIONS | SPECTRAL ENERGY-DISTRIBUTION | TELESCOPE OBSERVATIONS | Polarization | Correlation | Parameters | Broadband | Computer simulation | Data acquisition | Emission analysis | Variability | X-ray emissions | Electron energy distribution | Blazars | Rotation | Emissions | Optical polarization | Observatories | X rays | Wavelengths | Energy bands | Correlation analysis | Correlation function | Mathematical models | Electron energy | Physics - High Energy Astrophysical Phenomena
Journal Article