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Telescopio MAGIC - Historial de revisiones
2026-05-03T16:49:00Z
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https://guanches.org/index.php?title=Telescopio_MAGIC&diff=198925&oldid=prev
Atamankad en 19:54 16 abr 2024
2024-04-16T19:54:53Z
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revisión del 19:54 16 abr 2024</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Telescopios|Magic]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Telescopios|Magic]]</div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Observatorio del Roque de <del style="font-weight: bold; text-decoration: none;">Los </del>Muchachos]]</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:<ins style="font-weight: bold; text-decoration: none;">Telescopios del </ins>Observatorio del Roque de <ins style="font-weight: bold; text-decoration: none;">los </ins>Muchachos]]</div></td></tr>
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Atamankad
https://guanches.org/index.php?title=Telescopio_MAGIC&diff=113839&oldid=prev
Atamankad en 17:58 1 abr 2013
2013-04-01T17:58:44Z
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<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>'''MAGIC''' significa '''''Major Atmospheric Gamma-ray Imaging Cherenkov Telescope''''', o sea "<del style="font-weight: bold; text-decoration: none;">Gran </del>Telescopio de <del style="font-weight: bold; text-decoration: none;">Rayos Gamma </del>de <del style="font-weight: bold; text-decoration: none;">Imagen </del>Cherenkov". Está localizado en el [[Observatorio del Roque de los Muchachos]] en [[La Palma]] ([[Islas Canarias]]). <del style="font-weight: bold; text-decoration: none;">Con </del>un espejo de 17 metros de diámetro y un área de 240 metros cuadrados, <del style="font-weight: bold; text-decoration: none;">es </del>capaz de detectar los destellos de luz producidos en la atmósfera por rayos cósmicos. <del style="font-weight: bold; text-decoration: none;">Su objetivo fundamental es la detección de </del>[[<del style="font-weight: bold; text-decoration: none;">rayos gamma</del>]] <del style="font-weight: bold; text-decoration: none;">de muy alta energía con los que tienen muchas dificultades los detectores a bordo de satélites</del>. </div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>'''MAGIC''' significa '''''Major Atmospheric Gamma-ray Imaging Cherenkov Telescope''''', o sea "Telescopio de <ins style="font-weight: bold; text-decoration: none;">rayos gamma por emisión </ins>de <ins style="font-weight: bold; text-decoration: none;">radiación </ins>Cherenkov <ins style="font-weight: bold; text-decoration: none;">en la atmósfera</ins>". Está localizado en el [[Observatorio del Roque de los Muchachos]] en [[La Palma]] ([[Islas Canarias]]). <ins style="font-weight: bold; text-decoration: none;">Tras su construcción en 2004, MAGIC era un solo [[telescopio Cherenkov]] con </ins>un espejo de 17 metros de diámetro y un área de 240 metros cuadrados, capaz de detectar los destellos de luz producidos en la atmósfera por rayos cósmicos. <ins style="font-weight: bold; text-decoration: none;">En 2008 se le unió un segundo telescopio, un clon del anterior, apodado MAGIC-II.<ref>"Technical status of the MAGIC telescopes", MAGIC collaboration, Proc. International Cosmic Rays Conference 2009, arXiv:0907.1211</ref> Operado junto al primero, mejora sustancialmente su </ins>[[<ins style="font-weight: bold; text-decoration: none;">resolución óptica|resolución angular</ins>]] <ins style="font-weight: bold; text-decoration: none;">y su sensibilidad</ins>.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Empezó a tomar datos en </del>[[<del style="font-weight: bold; text-decoration: none;">2004</del>]] <del style="font-weight: bold; text-decoration: none;">y es el sucesor del experimento </del>[[<del style="font-weight: bold; text-decoration: none;">HEGRA</del>]].</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Su objetivo fundamental es la detección de </ins>[[<ins style="font-weight: bold; text-decoration: none;">rayos gamma</ins>]] <ins style="font-weight: bold; text-decoration: none;">de muy alta energía. A estas energías, por encima de 10 </ins>[[<ins style="font-weight: bold; text-decoration: none;">electronvoltio|GeV</ins>]]<ins style="font-weight: bold; text-decoration: none;">, son muy difíciles de detectar con instrumentos situados a bordo de satélites porque su débil flujo hace necesarias áreas de detección muy grandes</ins>.</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">=== Institutos colaboradores ===</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">[[Archivo:Magic</ins>-<ins style="font-weight: bold; text-decoration: none;">Telescope.jpg|thumb</ins>|<ins style="font-weight: bold; text-decoration: none;">200px</ins>|<ins style="font-weight: bold; text-decoration: none;">Espejo principal del primer telescopio MAGIC</ins>.<ins style="font-weight: bold; text-decoration: none;">]]</ins></div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Institut de Física d'Altes Energies</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Los telescopios MAGIC sucedieron a unos telescopios de Cherenkov de la generación anterior que se llamaban [[HEGRA]] y estaban localizados en el mismo lugar.</ins></div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Universitat Autònoma de Barcelona</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Reúne una larga serie de mejoras e innovaciones técnicas respecto a la primera generación de telescopios de Cherenkov</ins>. <ins style="font-weight: bold; text-decoration: none;">Las [[cámara]]s</ins>, <ins style="font-weight: bold; text-decoration: none;">o sea</ins>, <ins style="font-weight: bold; text-decoration: none;">los detectores donde enfocan la luz los espejos</ins>, <ins style="font-weight: bold; text-decoration: none;">son mucho más eficientes y rápidas</ins>. <ins style="font-weight: bold; text-decoration: none;">Las monturas son extremadamente ligeras (junto con los espejos</ins>, <ins style="font-weight: bold; text-decoration: none;">pesan menos de 20 toneladas)</ins>, <ins style="font-weight: bold; text-decoration: none;">para poder moverse con rapidez cuando se da la alerta de la explosión de algún objeto rápidamente variable. Los espejos están construidos en una aleación de [[aluminio]] y son altamente reflectantes pero también muy ligeros. Los cables que van de la cámara a la electrónica central están hechos</ins>, <ins style="font-weight: bold; text-decoration: none;">no de hilo de cobre</ins>, <ins style="font-weight: bold; text-decoration: none;">sino de fibra óptica para reducir el peso y mejorar el transporte de la señal. Las señales de los fotodetectores duran unos </ins>[[<ins style="font-weight: bold; text-decoration: none;">segundo|nanosegundos</ins>]] <ins style="font-weight: bold; text-decoration: none;">y requieren digitalizadores extremadamente rápidos: los actuales en operación muestrean a 2 GHz.</ins></div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Institut für Physik, Humboldt</del>-<del style="font-weight: bold; text-decoration: none;">University of Berlin</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Crimean Astrophysical Observatory</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*University of California, Davis, USA</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Universidad Complutense, Madrid</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Division of Experimental Physics, University of Lodz</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Max-Planck-Gesellschaft</del>|<del style="font-weight: bold; text-decoration: none;">Max-Planck-Institute for Physics, Munich</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Physics Department, University of Padua</del>|<del style="font-weight: bold; text-decoration: none;">Università di Padova and INFN sez</del>. <del style="font-weight: bold; text-decoration: none;">di Padova, Italy</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Space Research Unit, Potchefstroom University</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Dipartimento di Fisica, University of Siena|Università di Siena and INFN sez</del>. <del style="font-weight: bold; text-decoration: none;">di Pisa</del>, <del style="font-weight: bold; text-decoration: none;">Italy</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Institute for Nuclear Research and Nuclear Energy, Sofia</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Tuorla Observatory</del>, <del style="font-weight: bold; text-decoration: none;">Pikkiö</del>, <del style="font-weight: bold; text-decoration: none;">Finland</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Dipartimento di Fisica dell'University of Udine|Università di Udine and INFN sez</del>. <del style="font-weight: bold; text-decoration: none;">di Trieste</del>, <del style="font-weight: bold; text-decoration: none;">Italy</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*University of Würzburg</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Yerevan Physics Institute</del>, <del style="font-weight: bold; text-decoration: none;">Cosmic Ray Division</del>, <del style="font-weight: bold; text-decoration: none;">Jerewan</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*Institute for Particle Physics</del>, <del style="font-weight: bold; text-decoration: none;">Eidgenössische Technische Hochschule Zürich</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">*</del>[[<del style="font-weight: bold; text-decoration: none;">Instituto de Astrofísica de Canarias</del>]]<del style="font-weight: bold; text-decoration: none;">, Tenerife, España</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">A energías tan altas, los telescopios MAGIC observan sólo objetos del universo en los que los fotones no resultan de procesos de [[fusión nuclear]] como los que suceden normalmente en las [[estrellas]]. Ejemplos de procesos no-nucleares son la acreción de materia por un [[objeto compacto]] como una [[estrella de neutrones]] o un [[agujero negro]], la aceleración de partículas cargadas en un remanente de [[supernova]] o en ondas de choque en los chorros (jets) de una [[galaxia activa]]. Los rayos gamma de muy alta energía también pueden ser productos secundarios de las colisiones de [[rayos cósmicos]] con átomos del medio interestelar y, por tanto, sirven para estudiar la distribución de los rayos cósmicos en nuestra galaxia. Y podrían así mismo ser secundarios de la aniquilación de partículas de [[materia oscura]] con lo que podrían constituirse también en un medio muy útil para saber dónde se concentra la materia oscura. La investigación de rayos gamma de altas energías y rayos cósmicos forma parte de la llamada [[Física de Astropartículas]].</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">La mayor parte de la colaboración MAGIC está actualmente implicada en el proyecto [[Cherenkov Telescope Array]], que se propone la construcción de una matriz de decenas de telescopios de rayos gamma con una sensibilidad diez veces mayor que MAGIC.</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">== Resultados relevantes ==</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Descubrimiento<ref>"Variable Very-High-Energy Gamma-Ray Emission from the Microquasar LS I +61 303", MAGIC collaboration, Science, 312, no. 5781 (2006) 1771</ref> en rayos gamma de la emisión periódica de la binaria [[LS I +61 303]].</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Descubrimiento en rayos gamma del [[núcleo activo de galaxia]] prototípico BL Lac.<ref>"Discovery of Very High Energy Gamma-Ray Emission from the Low-Frequency-peaked BL Lacertae Object BL Lacertae",</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">MAGIC collaboration, ApJ Lett. 666 (2007) L17</ref></ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Evidencia de emisión gamma<ref>"Very High Energy Gamma-ray Radiation from the Stellar-mass Black Hole Cygnus X-1", MAGIC collaboration, Ap. J. 665 (2007) L51</ref> en la [[binaria de Rayos X]] con [[agujero negro]] [[Cygnus X-1]].</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Descubrimiento<ref>"Very-High-Energy gamma rays from a Distant Quasar: How Transparent Is the Universe?", MAGIC collaboration, Science 320 (2008) 1752</ref> de emisión de altas energías del quásar [[3C279]].</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Primer descubrimiento<ref>"Observation of Pulsed Gamma-Rays Above 25 GeV from the Crab Pulsar with MAGIC", MAGIC collaboration, Science 322 (2008) 1221.</ref> de emisión pulsada de un [[púlsar]] en altas energías ([[pulsar del Cangrejo]]).</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Primera medida de gran precisión del lugar de origen de los rayos gamma de la [[radiogalaxia]] [[M87]].<ref>"Radio Imaging of the Very-High-Energy Gamma-Ray Emission Region in the Central Engine of a Radio Galaxy", MAGIC collaboration, Science 325 (2009) 169.</ref></ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">== Institutos colaboradores ==</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Instituto de Física de Altas Energías]]</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Universidad Autónoma de Barcelona]]</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Universidad de Barcelona]]</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Universidad Complutense]], [[Madrid]]</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Division of Experimental Physics, University of Lodz</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Instituto Max Planck de Física]], [[Múnich]]</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Physics Department, University of Padua|Università di Padova and INFN sez. di Padova, Italy</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Dipartimento di Fisica, University of Siena|Università di Siena and INFN sez. di Pisa, Italy</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Institute for Nuclear Research and Nuclear Energy, Sofia</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Tuorla Observatory, Pikkiö, Finland</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Dipartimento di Fisica dell'University of Udine|Università di Udine and INFN sez. di Trieste, Italy</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* University of Würzburg</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Institute for Particle Physics, Eidgenössische Technische Hochschule Zürich</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[DESY]] Zeuthen Berlín.</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Instituto de Astrofísica de Andalucía]], Granada, España.</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[Instituto de Astrofísica de Canarias]], Tenerife, España.</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* Consorcio de institutos [[croatas]].</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr>
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<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"><references /></ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>=== Enlaces externos ===</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>=== Enlaces externos ===</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://magic.mppmu.mpg.de/ Página del telescopio MAGIC (en inglés)]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://magic.mppmu.mpg.de/ Página del telescopio MAGIC (en inglés)]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://magic.ifae.es/ Página del telescopio MAGIC (en español)]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://magic.ifae.es/ Página del telescopio MAGIC (en español)]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
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<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">{{coord|28|45|43|N|17|53|24|W|region:ES-CN_type:landmark|display=title}} </ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Telescopios|Magic]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Telescopios|Magic]]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Observatorio del Roque de Los Muchachos]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Observatorio del Roque de Los Muchachos]]</div></td></tr>
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Atamankad
https://guanches.org/index.php?title=Telescopio_MAGIC&diff=113837&oldid=prev
Atamankad en 17:56 1 abr 2013
2013-04-01T17:56:35Z
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Atamankad
https://guanches.org/index.php?title=Telescopio_MAGIC&diff=3897&oldid=prev
Atamankad en 12:40 2 oct 2006
2006-10-02T12:40:01Z
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<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Telescopios|<del style="font-weight: bold; text-decoration: none;">Telescopio magic</del>]]</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>[[Categoría:Telescopios|<ins style="font-weight: bold; text-decoration: none;">Magic</ins>]]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[categoría:La Palma]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[categoría:La Palma]]</div></td></tr>
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Atamankad
https://guanches.org/index.php?title=Telescopio_MAGIC&diff=3737&oldid=prev
Mencey en 13:39 30 sep 2006
2006-09-30T13:39:17Z
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Revisión anterior</td>
<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revisión del 13:39 30 sep 2006</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*University of California, Davis, USA</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*University of California, Davis, USA</div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*<del style="font-weight: bold; text-decoration: none;">[[</del>Universidad Complutense<del style="font-weight: bold; text-decoration: none;">]]</del>, <del style="font-weight: bold; text-decoration: none;">[[</del>Madrid<del style="font-weight: bold; text-decoration: none;">]]</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*Universidad Complutense, Madrid</div></td></tr>
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Mencey
https://guanches.org/index.php?title=Telescopio_MAGIC&diff=1814&oldid=prev
Atamankad en 20:14 27 ago 2006
2006-08-27T20:14:16Z
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<p><b>Página nueva</b></p><div>'''MAGIC''' significa '''''Major Atmospheric Gamma-ray Imaging Cherenkov Telescope''''', o sea "Gran Telescopio de Rayos Gamma de Imagen Cherenkov". Está localizado en el [[Observatorio del Roque de los Muchachos]] en [[La Palma]] ([[Islas Canarias]]). Con un espejo de 17 metros de diámetro y un área de 240 metros cuadrados, es capaz de detectar los destellos de luz producidos en la atmósfera por rayos cósmicos. Su objetivo fundamental es la detección de [[rayos gamma]] de muy alta energía con los que tienen muchas dificultades los detectores a bordo de satélites. <br />
<br />
Empezó a tomar datos en [[2004]] y es el sucesor del experimento [[HEGRA]].<br />
<br />
=== Institutos colaboradores ===<br />
*Institut de Física d'Altes Energies<br />
*Universitat Autònoma de Barcelona<br />
*Institut für Physik, Humboldt-University of Berlin<br />
*Crimean Astrophysical Observatory<br />
*University of California, Davis, USA<br />
*[[Universidad Complutense]], [[Madrid]]<br />
*Division of Experimental Physics, University of Lodz<br />
*Max-Planck-Gesellschaft|Max-Planck-Institute for Physics, [[Munich]]<br />
*Physics Department, University of Padua|Università di Padova and INFN sez. di Padova, Italy<br />
*Space Research Unit, Potchefstroom University<br />
*Dipartimento di Fisica, University of Siena|Università di Siena and INFN sez. di Pisa, Italy<br />
*Institute for Nuclear Research and Nuclear Energy, Sofia<br />
*Tuorla Observatory, Pikkiö, Finland<br />
*Dipartimento di Fisica dell'University of Udine|Università di Udine and INFN sez. di Trieste, Italy<br />
*University of Würzburg<br />
*Yerevan Physics Institute, Cosmic Ray Division, Jerewan<br />
*Institute for Particle Physics, Eidgenössische Technische Hochschule Zürich<br />
*[[Instituto de Astrofísica de Canarias]], Tenerife, España<br />
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=== Enlaces externos ===<br />
*[http://magic.mppmu.mpg.de/ Página del telescopio MAGIC (en inglés)]<br />
*[http://magic.ifae.es/ Página del telescopio MAGIC (en español)]<br />
<br />
[[Categoría:Telescopios|Telescopio magic]]<br />
[[categoría:La Palma]]</div>
Atamankad