{"id":3973,"date":"2025-05-26T16:10:14","date_gmt":"2025-05-26T16:10:14","guid":{"rendered":"http:\/\/astri.me.oa-brera.inaf.it\/?page_id=3973"},"modified":"2025-06-06T14:59:41","modified_gmt":"2025-06-06T14:59:41","slug":"new-the-astri-pillars","status":"publish","type":"page","link":"https:\/\/www.astri.inaf.it\/index.php\/prova\/new-the-astri-pillars\/","title":{"rendered":"La scienza dell&#8217;ASTRI Mini-Array"},"content":{"rendered":"\n<style type=\"text\/css\" data-created_by=\"avia_inline_auto\" id=\"style-css-av-mbj727ig-cf2671b24136ae1500965fe4c09ad3b1\">\n#top .av-special-heading.av-mbj727ig-cf2671b24136ae1500965fe4c09ad3b1{\npadding-bottom:10px;\n}\nbody .av-special-heading.av-mbj727ig-cf2671b24136ae1500965fe4c09ad3b1 .av-special-heading-tag .heading-char{\nfont-size:25px;\n}\n.av-special-heading.av-mbj727ig-cf2671b24136ae1500965fe4c09ad3b1 .av-subheading{\nfont-size:15px;\n}\n<\/style>\n<div  class='av-special-heading av-mbj727ig-cf2671b24136ae1500965fe4c09ad3b1 av-special-heading-h2 blockquote modern-quote  avia-builder-el-0  el_before_av_textblock  avia-builder-el-first '><h2 class='av-special-heading-tag '  itemprop=\"headline\"  >La scienza dell\u2019ASTRI Mini-Array<\/h2><div class=\"special-heading-border\"><div class=\"special-heading-inner-border\"><\/div><\/div><\/div>\n<section  class='av_textblock_section av-mbj72jtw-22a8287b5d2b889d6b62abd9bb368e55 '   itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/CreativeWork\" ><div class='avia_textblock'  itemprop=\"text\" ><h3><span style=\"font-weight: 400;\">I \u201cpilastri\u201d di ASTRI<\/span><\/h3>\n<p>Il programma scientifico dell&#8217;ASTRI Mini-Array si svilupper\u00e0 in due fasi. Durante i primi quattro anni di attivit\u00e0, l&#8217;ASTRI Mini-Array \u00ecoperer\u00e0 come esperimento; nei successivi quattro anni, evolver\u00e0 gradualmente in un osservatorio aperto alla comunit\u00e0 scientifica. Una rappresentazione grafica dei principali temi scientifici centrali che intendiamo affrontare nei primi quattro anni di attivit\u00e0 \u00e8 mostrata nella seguente figura.<\/p>\n<\/div><\/section>\n\n<style type=\"text\/css\" data-created_by=\"avia_inline_auto\" id=\"style-css-av-mbj74vxi-9d056aeec8834dffab7f1768979be31e\">\n.avia-image-container.av-mbj74vxi-9d056aeec8834dffab7f1768979be31e img.avia_image{\nbox-shadow:none;\n}\n.avia-image-container.av-mbj74vxi-9d056aeec8834dffab7f1768979be31e .av-image-caption-overlay-center{\ncolor:#ffffff;\n}\n<\/style>\n<div  class='avia-image-container av-mbj74vxi-9d056aeec8834dffab7f1768979be31e av-styling- avia-align-center  avia-builder-el-2  el_after_av_textblock  el_before_av_textblock '   itemprop=\"image\" itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/ImageObject\" ><div class=\"avia-image-container-inner\"><div class=\"avia-image-overlay-wrap\"><img decoding=\"async\" fetchpriority=\"high\" class='wp-image-4172 avia-img-lazy-loading-not-4172 avia_image ' src=\"https:\/\/www.astri.inaf.it\/wp-content\/uploads\/2025\/06\/ASTRI_Pillars.png\" alt='Figure shows the ASTRI Mini-Array Pillars: 1 and 2, Time Domain, Non gamma-ray, Synergies' title='ASTRI_Pillars'  height=\"580\" width=\"1030\"  itemprop=\"thumbnailUrl\"  \/><\/div><\/div><\/div>\n<section  class='av_textblock_section av-mbj73frl-07831c45c00e8106cfd807ae216b0215 '   itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/CreativeWork\" ><div class='avia_textblock'  itemprop=\"text\" ><p>Il nostro programma scientifico si basa su alcuni \u201cpilasti principali\u201d: ambiti nei quali l&#8217;ASTRI Mini-Array offrir\u00e0 contributi decisivi per rispondere a domande scientifiche fondamentali.<\/p>\n<p>L&#8217;ASTRI Mini-Array studier\u00e0 sorgenti a energie molto elevate (VHE) e ultra-elevate (UHE), fornendo sia una precisa identificazione che informazioni cruciali sulla loro morfologia e spettro.<\/p>\n<h3><strong>Le risorse di ASTRI<\/strong><\/h3>\n<p><strong data-start=\"1027\" data-end=\"1061\">L\u2019ampio intervallo energetico.<\/strong><br data-start=\"1061\" data-end=\"1064\" \/>Per la prima volta estendiamo la sensibilit\u00e0 differenziale dei moderni IACT fino a decine di TeV e oltre. Questo permetter\u00e0 di indagare eventuali caratteristiche spettrali a VHE, come cut-off o emissioni previste fino a decine di TeV da sorgenti galattiche PeV.<\/p>\n<p><strong data-start=\"1327\" data-end=\"1356\">Il grande campo di vista.<\/strong><br data-start=\"1356\" data-end=\"1359\" \/>Il campo di vista di 10\u00b0 dell&#8217;ASTRI Mini-Array, combinato con un\u2019eccellente prestazione off-axis (solo un fattore 2 di sensibilit\u00e0 in meno al bordo rispetto al centro), permetter\u00e0 di osservare pi\u00f9 sorgenti in un\u2019unica puntata e favorir\u00e0 scoperte casuali.<\/p>\n<\/div><\/section>\n\n<style type=\"text\/css\" data-created_by=\"avia_inline_auto\" id=\"style-css-av-mbj78clz-a0a1ac8f0d4f2ff947ae40f49c16de0b\">\n.avia-image-container.av-mbj78clz-a0a1ac8f0d4f2ff947ae40f49c16de0b img.avia_image{\nbox-shadow:none;\n}\n.avia-image-container.av-mbj78clz-a0a1ac8f0d4f2ff947ae40f49c16de0b .av-image-caption-overlay-center{\ncolor:#ffffff;\n}\n<\/style>\n<div  class='avia-image-container av-mbj78clz-a0a1ac8f0d4f2ff947ae40f49c16de0b av-styling- avia-align-center  avia-builder-el-4  el_after_av_textblock  el_before_av_textblock  av-has-copyright av-copyright-always'   itemprop=\"image\" itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/ImageObject\" ><div class=\"avia-image-container-inner\"><div class=\"avia-image-overlay-wrap\"><img decoding=\"async\" fetchpriority=\"high\" class='wp-image-4174 avia-img-lazy-loading-not-4174 avia_image ' src=\"https:\/\/www.astri.inaf.it\/wp-content\/uploads\/2025\/06\/ASTRI_Cygnus.png\" alt='' title='ASTRI_Cygnus'  height=\"994\" width=\"1030\"  itemprop=\"thumbnailUrl\"  \/><\/div><small class=\"avia-copyright\">Credits: Vercellone S. et al., 2022, JHEAP, 35,1<\/small><\/div><\/div>\n<section  class='av_textblock_section av-mbj76v0s-6dc58a94b08cd474c0e52c64118f1896 '   itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/CreativeWork\" ><div class='avia_textblock'  itemprop=\"text\" ><p>Questa figura mostra quanto sia importante un ampio campo visivo per osservare regioni affollate. Il pannello riporta una simulazione di 200 ore verso la regione del Cigno. Diverse sorgenti del Terzo Catalogo HAWC di sorgenti gamma a energie molto elevate (3HWC) possono essere rilevate in una singola puntata dell&#8217;ASTRI Mini-Array. Le croci verdi indicano la posizione delle sorgenti 3HWC in un campo visivo di 10\u00b0\u00d710\u00b0. [<em>Crediti: <\/em><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S2214404822000222\" target=\"_blank\" rel=\"noopener\"><em>Vercellone S. et al., 2022, JHEAP, 35,1<\/em><\/a>]<\/p>\n<p><strong data-start=\"2193\" data-end=\"2227\">L\u2019ottima risoluzione angolare.<\/strong><br data-start=\"2227\" data-end=\"2230\" \/>L\u2019ASTRI Mini-Array raggiunge una risoluzione angolare di circa 3\u2019 nel range 3\u2013100 TeV.<\/p>\n<\/div><\/section>\n\n<style type=\"text\/css\" data-created_by=\"avia_inline_auto\" id=\"style-css-av-mbj7a7pk-c4abf49ee1d7e81850f869e331d2c164\">\n.avia-image-container.av-mbj7a7pk-c4abf49ee1d7e81850f869e331d2c164 img.avia_image{\nbox-shadow:none;\n}\n.avia-image-container.av-mbj7a7pk-c4abf49ee1d7e81850f869e331d2c164 .av-image-caption-overlay-center{\ncolor:#ffffff;\n}\n<\/style>\n<div  class='avia-image-container av-mbj7a7pk-c4abf49ee1d7e81850f869e331d2c164 av-styling- avia-align-center  avia-builder-el-6  el_after_av_textblock  el_before_av_textblock  av-has-copyright av-copyright-always'   itemprop=\"image\" itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/ImageObject\" ><div class=\"avia-image-container-inner\"><div class=\"avia-image-overlay-wrap\"><img decoding=\"async\" fetchpriority=\"high\" class='wp-image-4176 avia-img-lazy-loading-not-4176 avia_image ' src=\"https:\/\/www.astri.inaf.it\/wp-content\/uploads\/2025\/06\/ASTRI_Angular_Resolution.png\" alt='' title='ASTRI_Angular_Resolution'  height=\"988\" width=\"1030\"  itemprop=\"thumbnailUrl\"  \/><\/div><small class=\"avia-copyright\">Credits: Vercellone S. et al., 2022, JHEAP, 35,1<\/small><\/div><\/div>\n<section  class='av_textblock_section av-mbj793xs-291630c9a42c5495ae15ebad91e57236 '   itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/CreativeWork\" ><div class='avia_textblock'  itemprop=\"text\" ><p>Questa figura mostra l\u2019importanza della risoluzione angolare dell&#8217;ASTRI Mini-Array. L\u2019immagine presenta una simulazione di 200 ore (fino a 200 TeV) della regione intorno alla sorgente galattica eHWC 1907+063. Il cerchio verde chiaro rappresenta l\u2019errore HAWC di circa 0,52\u00b0 (per E > 56 TeV). Pur condividendo un simile range energetico, l\u2019ASTRI Mini-Array ha una risoluzione angolare nettamente superiore rispetto a HAWC, consentendo una precisa localizzazione delle sorgenti galattiche UHE.\u00a0[<em>Crediti: <\/em><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S2214404822000222\" target=\"_blank\" rel=\"noopener\"><em>Vercellone S. et al., 2022, JHEAP, 35,1<\/em><\/a>]<\/p>\n<h3><strong>ASTRI Mini-Array e gli Osservatori UHE<\/strong><\/h3>\n<p>Prevediamo importanti sinergie con le attuali strutture UHE come LHAASO, HAWC e Tibet AS-\ud835\udfac. Un esempio \u00e8 mostrato nella figura seguente, dove si evidenziano le regioni obiettivo dei Pilastri 1 e 2 (cerchi rossi e blu, \u224810\u00b0 di diametro) e le sorgenti del catalogo 1LHAASO (punti arancioni, <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4365\/acfd29\" target=\"_blank\" rel=\"noopener\">Cao et al, 2024, ApJS, 271, 25<\/a>), in coordinate galattiche (proiezione di Aitoff). La linea nera continua mostra il limite in declinazione per le osservazioni dell\u2019ASTRI Mini-Array.<\/p>\n<\/div><\/section>\n\n<style type=\"text\/css\" data-created_by=\"avia_inline_auto\" id=\"style-css-av-mbj7deo5-885d1e2e5fa3a0a92356fd909ead2f4f\">\n.avia-image-container.av-mbj7deo5-885d1e2e5fa3a0a92356fd909ead2f4f img.avia_image{\nbox-shadow:none;\n}\n.avia-image-container.av-mbj7deo5-885d1e2e5fa3a0a92356fd909ead2f4f .av-image-caption-overlay-center{\ncolor:#ffffff;\n}\n<\/style>\n<div  class='avia-image-container av-mbj7deo5-885d1e2e5fa3a0a92356fd909ead2f4f av-styling- avia-align-center  avia-builder-el-8  el_after_av_textblock  el_before_av_textblock '   itemprop=\"image\" itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/ImageObject\" ><div class=\"avia-image-container-inner\"><div class=\"avia-image-overlay-wrap\"><img decoding=\"async\" fetchpriority=\"high\" class='wp-image-4178 avia-img-lazy-loading-not-4178 avia_image ' src=\"https:\/\/www.astri.inaf.it\/wp-content\/uploads\/2025\/06\/ASTRI_Pillars_1LHAASO.png\" alt='' title='ASTRI_Pillars_1LHAASO'  height=\"726\" width=\"1030\"  itemprop=\"thumbnailUrl\"  \/><\/div><\/div><\/div>\n<section  class='av_textblock_section av-mbj7b8pk-bc49e67c7436cdadaca7d020577c8c4e '   itemscope=\"itemscope\" itemtype=\"https:\/\/schema.org\/CreativeWork\" ><div class='avia_textblock'  itemprop=\"text\" ><p>Alcune sorgenti del catalogo 1LHAASO coincidono gi\u00e0 con le regioni selezionate dai Pilastri dell\u2019ASTRI Mini-Array, in particolare lungo il piano galattico. Mrk 501 e Mrk 421 sono inoltre candidati ideali per studi comuni di variabilit\u00e0.<\/p>\n<h3>Strumenti di Simulazione dell\u2019ASTRI Mini-Array<\/h3>\n<p>Le simulazioni scientifiche dell&#8217;ASTRI Mini-Array si basano sulle attuali funzioni di risposta strumentale (IRF, Prod2, v1.0), disponibili su <a href=\"https:\/\/zenodo.org\/records\/6827882\" target=\"_blank\" rel=\"noopener\">Zenodo<\/a>.<\/p>\n<p>Le IRF sono memorizzate in file FITS contenenti le seguenti quantit\u00e0 (FITS tables): area efficace di raccolta (&#8220;EFFECTIVE AREA&#8221;), funzione di dispersione angolare (&#8220;POINT SPREAD FUNCTION&#8221;), risoluzione energetica (&#8220;ENERGY DISPERSION&#8221;), tasso di fondo residuo (&#8220;BACKGROUND&#8221;). Queste grandezze sono fornite in funzione dell\u2019energia e dell\u2019angolo off-axis. I bin energetici sono logaritmici e compresi tra 10<sup>-0.7<\/sup> ~ 0.2 TeV e 10<sup>2.5<\/sup> ~ 316 TeV. Si usano 5 bin per decade per risoluzione angolare e fondo, 10 bin per decade per area efficace, e una binned matrix molto fine per la risoluzione energetica. L\u2019angolo off-axis \u00e8 suddiviso linearmente da 0\u00b0 a 6\u00b0, con bin di 1\u00b0. Per il fondo residuo, si usa un binning spaziale quadrato bidimensionale (da 0\u00b0 a 6\u00b0, bin di 0.2\u00b0).<\/p>\n<p>Le IRF posso essere usate come input negli strumenti di analisi e, in particolare, sono compatibili con il formato dati input\/output (I\/O) richiesti dagli strumenti di analisi <a href=\"https:\/\/gammapy.org\/\" target=\"_blank\" rel=\"noopener\">Gammapy<\/a> [<a href=\"https:\/\/www.aanda.org\/component\/article?access=doi&#038;doi=10.1051\/0004-6361\/202346488\" target=\"_blank\" rel=\"noopener\"><em>Donath A., et al., 2023, A&#038;A, 678, A157<\/em><\/a>] and <a href=\"http:\/\/cta.irap.omp.eu\/ctools\/\" target=\"_blank\" rel=\"noopener\">ctools<\/a> [<a href=\"https:\/\/www.aanda.org\/articles\/aa\/pdf\/2016\/09\/aa28822-16.pdf\" target=\"_blank\" rel=\"noopener\"><em>Kn\u00f6dlseder J., et al., 2016, A&#038;A 593, A1<\/em><\/a>].<\/p>\n<p>Una sintesi delle prestazioni principali dell&#8217;ASTRI Mini-Array \u00e8 disponibile in <em>Performance of the ASTRI Mini-Array at the Observatorio del Teide<\/em> \u2013 <a href=\"https:\/\/pos.sissa.it\/395\/884\/pdf\" target=\"_blank\" rel=\"noopener\">Lombardi S, et al., 2022, PoS(ICRC2021), 884<\/a><\/p>\n<h3 data-start=\"5033\" data-end=\"5092\"><strong data-start=\"5037\" data-end=\"5092\">Articoli Scientifici Generali sull\u2019ASTRI Mini-Array<\/strong><\/h3>\n<p data-start=\"5094\" data-end=\"5178\">Gli articoli pi\u00f9 recenti <em data-start=\"5119\" data-end=\"5134\">peer-reviewed<\/em> sui temi scientifici dell\u2019ASTRI Mini-Array:<\/p>\n<ul>\n<li><em>Science with the ASTRI Mini-Array: From Experiment to Open Observatory<\/em> \u2013 <a href=\"https:\/\/www.mdpi.com\/2218-1997\/10\/2\/94\" target=\"_blank\" rel=\"noopener\">Vercellone S., for the ASTRI Project, 2024, Universe, 10, 94<\/a><\/li>\n<li><em>ASTRI Mini-Array core science at the Observatorio del Teide<\/em> \u2013 <a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S2214404822000222?via%3Dihub\" target=\"_blank\" rel=\"noopener\">Vercellone S., et al., 2022, JHEAP, 35, 1<\/a><\/li>\n<li><em>Extragalactic observatory science with the ASTRI mini-array at the Observatorio del Teide<\/em> \u2013 <a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S2214404822000337?via%3Dihub\" target=\"_blank\" rel=\"noopener\">Saturni F.G., et al., 2022, JHEAP, 35, 91<\/a><\/li>\n<li><em>Galactic observatory science with the ASTRI Mini-Array at the Observatorio del Teide<\/em> \u2013 <a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S2214404822000350?via%3Dihub\" target=\"_blank\" rel=\"noopener\">D\u2019A\u00ec A., et al., 2022, JHEAP, 35, 139<\/a><\/li>\n<\/ul>\n<h3 data-start=\"5718\" data-end=\"5780\"><strong data-start=\"5722\" data-end=\"5780\">Alcuni link utili a osservatori MWL attuali [e futuri]<\/strong><\/h3>\n<ul>\n<li><strong>Radio: <\/strong><a href=\"https:\/\/www.eso.org\/public\/teles-instr\/alma\/\" target=\"_blank\" rel=\"noopener\">ALMA<\/a>, <a href=\"https:\/\/www.csiro.au\/en\/about\/facilities-collections\/ATNF\/ASKAP-radio-telescope\" target=\"_blank\" rel=\"noopener\">ASCAP<\/a>, <a href=\"https:\/\/chime-experiment.ca\/en\" target=\"_blank\" rel=\"noopener\">Chime<\/a>, <a href=\"https:\/\/fast.bao.ac.cn\/\" target=\"_blank\" rel=\"noopener\">FAST<\/a>, <a href=\"https:\/\/www.radiotelescopes.inaf.it\/\" target=\"_blank\" rel=\"noopener\">INAF Radio Telescopes<\/a>, <a href=\"https:\/\/science.astron.nl\/telescopes\/lofar\/\" target=\"_blank\" rel=\"noopener\">LOFAR<\/a>, <a href=\"https:\/\/www.sarao.ac.za\/science\/meerkat\/about-meerkat\/\" target=\"_blank\" rel=\"noopener\">MeerKAT<\/a>, [<a href=\"https:\/\/www.skao.int\/en\" target=\"_blank\" rel=\"noopener\">SKAO<\/a>]<\/li>\n<li><strong>Optical:<\/strong> [<a href=\"https:\/\/elt.eso.org\/\" target=\"_blank\" rel=\"noopener\">ELT<\/a>], <a href=\"https:\/\/www.gtc.iac.es\/\" target=\"_blank\" rel=\"noopener\">GTC<\/a>, <a href=\"https:\/\/telescope.livjm.ac.uk\/\" target=\"_blank\" rel=\"noopener\">Liverpool Robotic Telescope<\/a>, <a href=\"https:\/\/www.eso.org\/public\/teles-instr\/lasilla\/ntt\/\" target=\"_blank\" rel=\"noopener\">NTT<\/a>, <a href=\"http:\/\/www.rem.inaf.it\/\" target=\"_blank\" rel=\"noopener\">REM<\/a>, <a href=\"https:\/\/www.tng.iac.es\/\" target=\"_blank\" rel=\"noopener\">TNG<\/a>, <a href=\"https:\/\/rubinobservatory.org\/\" target=\"_blank\" rel=\"noopener\">Vera C. Rubin Observatory<\/a>, <a href=\"https:\/\/www.eso.org\/public\/teles-instr\/paranal-observatory\/vlt\/\" target=\"_blank\" rel=\"noopener\">VLT<\/a>, <a href=\"https:\/\/www.oato.inaf.it\/blazars\/webt\/\" target=\"_blank\" rel=\"noopener\">WEBT<\/a><\/li>\n<li><strong>X-Ray: <\/strong><a href=\"https:\/\/www.nasa.gov\/mission\/chandra-x-ray-observatory\/\" target=\"_blank\" rel=\"noopener\">Chandra<\/a>, <a href=\"https:\/\/ep.bao.ac.cn\/ep\/\" target=\"_blank\" rel=\"noopener\">Einstein Probe<\/a>, <a href=\"https:\/\/www.mpe.mpg.de\/eROSITA\" target=\"_blank\" rel=\"noopener\">eROSITA\/SRG<\/a>, <a href=\"https:\/\/www.hermes-sp.eu\/\" target=\"_blank\" rel=\"noopener\">HERMES<\/a>, <a href=\"https:\/\/hxmt.nssdc.ac.cn\/\" target=\"_blank\" rel=\"noopener\"><em>Insight<\/em>-HXMT<\/a>, <a href=\"https:\/\/ixpe.msfc.nasa.gov\/index.html\" target=\"_blank\" rel=\"noopener\">IXPE<\/a>, <a href=\"https:\/\/www.nustar.caltech.edu\/\" target=\"_blank\" rel=\"noopener\">NuSTAR<\/a>, <a href=\"https:\/\/www.esa.int\/Science_Exploration\/Space_Science\/XMM-Newton\" target=\"_blank\" rel=\"noopener\">XMM-Newton<\/a><strong>, <\/strong><a href=\"https:\/\/www.svom.eu\/en\/home\/\" target=\"_blank\" rel=\"noopener\">SVOM<\/a><strong>, <\/strong><a href=\"https:\/\/swift.gsfc.nasa.gov\/\" target=\"_blank\" rel=\"noopener\"><em>Swift<\/em><\/a><strong>, <\/strong><a href=\"https:\/\/science.nasa.gov\/mission\/xrism\/\" target=\"_blank\" rel=\"noopener\">XRISM<\/a><\/li>\n<li><strong>HE: <\/strong>[<a href=\"https:\/\/science.nasa.gov\/mission\/cosi\/\" target=\"_blank\" rel=\"noopener\">COSI]<\/a>, <a href=\"https:\/\/fermi.gsfc.nasa.gov\/\" target=\"_blank\" rel=\"noopener\">Fermi<\/a><\/li>\n<li><strong>VHE: <\/strong>[<a href=\"https:\/\/www.ctao.org\/\" target=\"_blank\" rel=\"noopener\">CTAO<\/a>], <a href=\"https:\/\/www.mpi-hd.mpg.de\/HESS\/\" target=\"_blank\" rel=\"noopener\">H.E.S.S<\/a>., <a href=\"https:\/\/www.lst1.iac.es\/\" target=\"_blank\" rel=\"noopener\">LST-1<\/a>, <a href=\"https:\/\/magic.mppmu.mpg.de\/\" target=\"_blank\" rel=\"noopener\">MAGIC<\/a>, <a href=\"https:\/\/veritas.sao.arizona.edu\/\" target=\"_blank\" rel=\"noopener\">VERITAS<\/a><\/li>\n<li><strong>UHE: <\/strong><a href=\"https:\/\/www.hawc-observatory.org\/\" target=\"_blank\" rel=\"noopener\">HAWC<\/a>, <a href=\"http:\/\/english.ihep.cas.cn\/lhaaso\/\" target=\"_blank\" rel=\"noopener\">LHAASO<\/a>, <a href=\"https:\/\/www.swgo.org\/SWGOWiki\/doku.php?id=start\" target=\"_blank\" rel=\"noopener\">[SWGO]<\/a>, <a href=\"https:\/\/www.icrr.u-tokyo.ac.jp\/em\/index.html\" target=\"_blank\" rel=\"noopener\">Tibet AS-\ud835\udfac<\/a><\/li>\n<li><strong>Cosmic Rays:<\/strong> <a href=\"https:\/\/www.auger.org\/\" target=\"_blank\" rel=\"noopener\">Pierre Auger Observatory<\/a><\/li>\n<li><strong>Neutrino: <\/strong><a href=\"https:\/\/antares.in2p3.fr\/\" target=\"_blank\" rel=\"noopener\">ANTARES<\/a>, <a href=\"https:\/\/icecube.wisc.edu\/\" target=\"_blank\" rel=\"noopener\">IceCube<\/a>, <a href=\"https:\/\/www.km3net.org\/\" target=\"_blank\" rel=\"noopener\">KM3NeT<\/a><\/li>\n<li><strong>Gravitational Waves:<\/strong> <a href=\"https:\/\/www.ligo.caltech.edu\/\" target=\"_blank\" rel=\"noopener\">LIGO<\/a>, <a href=\"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/\" target=\"_blank\" rel=\"noopener\">KAGRA<\/a>, <a href=\"https:\/\/www.virgo-gw.eu\/\" target=\"_blank\" rel=\"noopener\">VIRGO<\/a><\/li>\n<\/ul>\n<\/div><\/section>\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":4,"featured_media":0,"parent":3930,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-3973","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/3973","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/users\/4"}],"replies":[{"embeddable":true,"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/comments?post=3973"}],"version-history":[{"count":12,"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/3973\/revisions"}],"predecessor-version":[{"id":4420,"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/3973\/revisions\/4420"}],"up":[{"embeddable":true,"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/3930"}],"wp:attachment":[{"href":"https:\/\/www.astri.inaf.it\/index.php\/wp-json\/wp\/v2\/media?parent=3973"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}