{"id":395,"date":"2025-12-17T11:00:19","date_gmt":"2025-12-17T11:00:19","guid":{"rendered":"https:\/\/microstars.eu\/?page_id=395"},"modified":"2026-07-15T15:04:50","modified_gmt":"2026-07-15T15:04:50","slug":"publications","status":"publish","type":"page","link":"https:\/\/microstars.eu\/index.php\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"\n<div class=\"wp-block-group animated fadeInUp has-global-padding is-layout-constrained wp-container-core-group-is-layout-ed3c30a0 wp-block-group-is-layout-constrained\">\n<div class=\"wp-block-group publications has-global-padding is-layout-constrained wp-container-core-group-is-layout-068f883d wp-block-group-is-layout-constrained\">\n<h2 class=\"wp-block-heading has-body-font-family\" style=\"padding-bottom:var(--wp--preset--spacing--10);font-size:clamp(27.894px, 1.743rem + ((1vw - 3.2px) * 2.094), 48px);font-style:normal;font-weight:700;letter-spacing:-1px\">Publications<\/h2>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"has-body-font-family wp-block-paragraph\" style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.625), 20px);letter-spacing:-1px\"><a href=\"https:\/\/academic.oup.com\/mnras\/article\/529\/4\/4387\/7625603?login=false\" data-type=\"link\" data-id=\"https:\/\/academic.oup.com\/mnras\/article\/529\/4\/4387\/7625603?login=false\" target=\"_blank\" rel=\"noreferrer noopener\">Performance and first measurements of the MAGIC stellar intensity interferometer<\/a> (MAGIC Collaboration, 2024)<\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-body-font-family wp-elements-1 wp-block-paragraph\" style=\"color:#69e3ba;font-size:14px;font-style:normal;font-weight:300\">S Abe, J Abhir, V A Acciari, A Aguasca-Cabot, I Agudo, T Aniello, S Ansoldi, L A Antonelli, A Arbet&nbsp;Engels, C Arcaro<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"has-body-font-family wp-block-paragraph\" style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.625), 20px);letter-spacing:-1px\"><a href=\"https:\/\/academic.oup.com\/mnras\/article\/491\/2\/1540\/5625079?login=false\" data-type=\"link\" data-id=\"https:\/\/academic.oup.com\/mnras\/article\/491\/2\/1540\/5625079?login=false\" target=\"_blank\" rel=\"noreferrer noopener\">Optical intensity interferometry observations using the MAGIC Imaging Atmospheric Cherenkov Telescopes<\/a> (MAGIC Collaboration, 2019)<\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-body-font-family wp-elements-2 wp-block-paragraph\" style=\"color:#69e3ba;font-size:14px;font-style:normal;font-weight:300\">V A Acciari, M I Bernardos, E Colombo, J L Contreras, J Cortina, A De&nbsp;Angelis, C Delgado, C D\u00edaz, D Fink, M Mariotti<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"has-body-font-family wp-block-paragraph\" style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.625), 20px);letter-spacing:-1px\"><a href=\"https:\/\/www.research-collection.ethz.ch\/entities\/publication\/abd4a2a5-6491-459f-8615-762cb44c78bb\" data-type=\"link\" data-id=\"https:\/\/academic.oup.com\/mnras\/article\/491\/2\/1540\/5625079?login=false\" target=\"_blank\" rel=\"noreferrer noopener\">Update on the performance of the MAGIC Intensity Interferometer<\/a><\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-body-font-family wp-elements-3 wp-block-paragraph\" style=\"color:#69e3ba;font-size:14px;font-style:normal;font-weight:300\">V A Acciari, M I Bernardos, E Colombo, J L Contreras, J Cortina, A De&nbsp;Angelis, C Delgado, C D\u00edaz, D Fink, M Mariotti<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"has-body-font-family wp-block-paragraph\" style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.625), 20px);letter-spacing:-1px\"><a href=\"https:\/\/academic.oup.com\/mnras\/article\/491\/2\/1540\/5625079?login=false\" data-type=\"link\" data-id=\"https:\/\/academic.oup.com\/mnras\/article\/491\/2\/1540\/5625079?login=false\" target=\"_blank\" rel=\"noreferrer noopener\">Performance of MAGIC stellar intensity interferometer and expansion to MAGIC + CTAO-LST1 stellar intensity interferometer<\/a><\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-body-font-family wp-elements-4 wp-block-paragraph\" style=\"color:#69e3ba;font-size:14px;font-style:normal;font-weight:300\">Alejo Cifuentes, V. A. Acciari, F. Barnes, G. Chon, E. Colombo, J. Cortina, C. Delgado, C. D\u00edaz, M. Fiori, D. Fink, T. Hassan, I. Jim\u00e9nez Mart\u00ednez, I. Jorge, D. Kerszberg, E. Lyard, G. Mart\u00ednez, R. Mirzoyan, M. Polo, N. Produit, J. J. Rodr\u00edguez-V\u00e1zquez, P. Saha, T. Schweizer, D. Strom, R. Walter, C. W. Wunderlich<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"has-body-font-family wp-block-paragraph\" style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.625), 20px);letter-spacing:-1px\"><a href=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1538-3873\/ae20c0\" data-type=\"link\" data-id=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1538-3873\/ae20c0\" target=\"_blank\" rel=\"noreferrer noopener\">A Butterfly\u2019s Eye Camera for Intensity Interferometry with Cherenkov Telescopes<\/a><\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-body-font-family wp-elements-5 wp-block-paragraph\" style=\"color:#69e3ba;font-size:14px;font-style:normal;font-weight:300\">J. Cortina, A. Cifuentes Santos, T. Hassan, and F. Fr\u00edas Garc\u00eda-Lago<\/p>\n<\/div>\n<\/div>\n\n\n\n<div style=\"height:118px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group publications has-global-padding is-layout-constrained wp-container-core-group-is-layout-068f883d wp-block-group-is-layout-constrained\">\n<h2 class=\"wp-block-heading has-body-font-family\" style=\"padding-bottom:var(--wp--preset--spacing--20);font-size:clamp(27.894px, 1.743rem + ((1vw - 3.2px) * 2.094), 48px);font-style:normal;font-weight:700;letter-spacing:-1px\">Useful references<\/h2>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"wp-block-paragraph\" style=\"font-style:normal;font-weight:600\"><a href=\"https:\/\/linkinghub.elsevier.com\/retrieve\/pii\/S1387647307000620\" data-type=\"link\" data-id=\"https:\/\/linkinghub.elsevier.com\/retrieve\/pii\/S1387647307000620\">An introduction to visibility modelling<\/a> (J. P. Berger &amp; D. Segransan, 2007)<\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-small-font-size wp-elements-6 wp-block-paragraph\" style=\"color:#69e3ba\">Jean Philippe Berger, Damien Segransan<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"wp-block-paragraph\" style=\"font-style:normal;font-weight:600\"><a href=\"https:\/\/arxiv.org\/abs\/2007.10295\" data-type=\"link\" data-id=\"https:\/\/arxiv.org\/abs\/2007.10295\">Demonstration of stellar intensity interferometry with the four VERITAS telescopes<\/a><a href=\"https:\/\/arxiv.org\/abs\/2007.10295\" target=\"_blank\" rel=\"noreferrer noopener\"> (VERITAS Collaboration, 2020)<\/a><\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-small-font-size wp-elements-7 wp-block-paragraph\" style=\"color:#69e3ba\">A. U. Abeysekara, W. Benbow, A. Brill, J.H. Buckley, J.L. Christiansen, A.J.Chromey, M. K. Daniel, J. Davis, A. Falcone, Q. Feng, J. P. Finley, L. Fortson, A. Furniss, A. Gent, C. Giuri, O. Gueta, D. Hanna, T. Hassan, O. Hervet, J. Holder, G. Hughes, T. B. Humensky, P. Kaaret, M. Kertzman, D. Kieda, F. Krennrich, S. Kumar, T. LeBohec, T. T. Y. Lin, M. Lundy, G. Maier, N. Matthews, P. Moriarty, R. Mukherjee M. Nievas-Rosillo, S. O&#8217;Brien, R. A. Ong, A. N. Otte, K. Pfrang, M. Pohl, R. R. Prado, E. Pueschel, J. Quinn, K. Ragan, P. T. Reynolds, D. Ribeiro, G. T. Richards, E. Roache, J. L. Ryan, M. Santander, G. H. Sembroski, S. P. Wakely, A. Weinstein, P. Wilcox, D. A. Williams, T. J Williamson<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"wp-block-paragraph\" style=\"font-style:normal;font-weight:600\"><a href=\"https:\/\/www.degruyterbrill.com\/document\/doi\/10.4159\/harvard.9780674366688.c4\/html\" data-type=\"link\" data-id=\"https:\/\/www.degruyterbrill.com\/document\/doi\/10.4159\/harvard.9780674366688.c4\/html\">A Test of a New Type of Stellar Interferometer on Sirius<\/a> (R. Hanbury-Brown and R. Q. Twiss, 1956)<\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-small-font-size wp-elements-8 wp-block-paragraph\" style=\"color:#69e3ba\">Robert Hanbury Brown and Richard Q. Twiss<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"wp-block-paragraph\" style=\"font-style:normal;font-weight:600\"><a href=\"https:\/\/articles.adsabs.harvard.edu\/\/full\/1974MNRAS.167..121H\/0000121.000.html\" data-type=\"link\" data-id=\"https:\/\/articles.adsabs.harvard.edu\/\/full\/1974MNRAS.167..121H\/0000121.000.html\">The Angular Diameters of 32 Stars<\/a> (R. Hanbury-Brown and R. Q. Twiss, 1974)<\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-small-font-size wp-elements-9 wp-block-paragraph\" style=\"color:#69e3ba\">Hanbury Brown, R., Davis, J., &amp; Allen, L. R.<\/p>\n<\/div>\n\n\n\n<div style=\"height:40px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-group is-layout-flow wp-block-group-is-layout-flow\">\n<p class=\"wp-block-paragraph\" style=\"font-style:normal;font-weight:600\"><a href=\"https:\/\/link.springer.com\/article\/10.1007\/s00159-012-0051-2\" data-type=\"link\" data-id=\"https:\/\/link.springer.com\/article\/10.1007\/s00159-012-0051-2\">Interferometric observations of rapidly rotating stars<\/a> (G T van Belle, 2012)<\/p>\n\n\n\n<p class=\"has-text-color has-link-color has-small-font-size wp-elements-10 wp-block-paragraph\" style=\"color:#69e3ba\">Gerard T. van Belle<\/p>\n<\/div>\n<\/div>\n\n\n\n<div style=\"height:132px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"publications","meta":{"footnotes":""},"class_list":["post-395","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/pages\/395","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/comments?post=395"}],"version-history":[{"count":13,"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/pages\/395\/revisions"}],"predecessor-version":[{"id":1523,"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/pages\/395\/revisions\/1523"}],"wp:attachment":[{"href":"https:\/\/microstars.eu\/index.php\/wp-json\/wp\/v2\/media?parent=395"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}