{"id":2891,"date":"2026-04-05T18:18:16","date_gmt":"2026-04-05T16:18:16","guid":{"rendered":"https:\/\/sf2a.eu\/website2023\/?p=2891"},"modified":"2026-04-05T18:18:16","modified_gmt":"2026-04-05T16:18:16","slug":"message-sf2a-no-1179","status":"publish","type":"post","link":"https:\/\/sf2a.eu\/website2023\/message-sf2a-no-1179\/","title":{"rendered":"Message SF2A No 1179"},"content":{"rendered":"\n<h2 class=\"wp-block-heading\">Message SF2A No 1179 &#8211; 06\/04\/26<\/h2>\n\n\n\n<ol class=\"wp-block-list\">\n<li>OPTICON Call for Proposals 2026<\/li>\n\n\n\n<li>Call for NRT proposals &#8211; 2026B<\/li>\n\n\n\n<li>Journees SF2A, Atelier S15 \u00ab\u00a0Formation and Evolution of Large Moons Around Giant Planets\u00a0\u00bb, 24 juin, 2026, Grenoble (France) &#8211; Appel \u00e0 contributions<\/li>\n\n\n\n<li>Conf\u00e9rence Mercury 2026, 1-4 septembre, 2026, Leuven (Belgique)<\/li>\n\n\n\n<li>Ecole Th\u00e9matique Evry Schatzman : Magn\u00e9tisme stellaire, 4-9 octobre, 2026, Roscoff (France)<\/li>\n\n\n\n<li>NECO Workshop: \u00ab\u00a0Probing the Circumstellar and Interstellar Medium with Transients and Multi-Wavelength Observations\u00a0\u00bb, 26-29 Octobre, 2026, Tokyo (Japan)<\/li>\n\n\n\n<li>LATMOS Seminar April 14th &#8211; Jorge HERN\u00c1NDEZ BERNAL &#8211; Martian aerosols investigated with imagers and high resolution models<\/li>\n\n\n\n<li>Le num\u00e9ro d&rsquo;avril du magazine de la SAF l\u2019Astronomie est paru<\/li>\n\n\n\n<li>Annonce de parution Cahiers Clairaut 193<\/li>\n<\/ol>\n\n\n\n<h3 class=\"wp-block-heading\">1. OPTICON Call for Proposals 2026<\/h3>\n\n\n\n<p>The OPTICON Alliance -an alliance of small- to medium-aperture telescopes with historical roots in OPTICON (the Optical Infrared Coordination Network for Astronomy, formerly supported by the OPTICON RadioNet Pilot programme of the European Commission)- is pleased to announce its Call for Proposals.<\/p>\n\n\n\n<p>The OPTICON Alliance continues the legacy by providing open-access Trans-National Access to the facilities of its member institutions.<\/p>\n\n\n\n<p>Instructions for telescope time applications are available at:&nbsp;<a href=\"https:\/\/opticon-alliance.eu\/\">https:\/\/opticon-alliance.eu<\/a><\/p>\n\n\n\n<p>Deadline for submissions:&nbsp;<strong>April 17, 2026, at 23:59 UT<\/strong><\/p>\n\n\n\n<p>Transmis par Philippe Mathias<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">2. Call for NRT proposals &#8211; 2026B<\/h3>\n\n\n\n<p>This is the 2026B semester call for proposals to observe with the Nancay Radio Telescope. The submission deadline is:\u00a0<strong>1 May 2026<\/strong>.<\/p>\n\n\n\n<p>The Nancay Radio Telescope (NRT, France) is a high sensitivity (1.4 K\/Jy at 21cm) meridian telescope (the tracking duration is 1 hour, and varies approximately as 1\/cos(DEC) ) with full polarization capability in the frequency range from 1.1 GHz to 3.5 GHz. The declination limit is &gt; -39 deg. It is operated by the Observatoire de Paris, the Centre National de la Recherche Scientifique and also funded by the Region Centre-Val de Loire.&nbsp;<\/p>\n\n\n\n<p>The NRT proposal call is open to the international community.&nbsp;<\/p>\n\n\n\n<p>Forms and explanations:&nbsp;<a href=\"https:\/\/www.obs-nancay.fr\/nrt-support-pages\/\">https:\/\/www.obs-nancay.fr\/nrt-support-pages\/<\/a><\/p>\n\n\n\n<p>Proposals are to be sent to:&nbsp;<a href=\"mailto:lucas.guillemot@cnrs-orleans.fr\">lucas.guillemot at cnrs-orleans.fr<\/a>&nbsp;.<\/p>\n\n\n\n<p>Transmis par Lucas Guillemot, on behalf of the NRT Programme Committee<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">3. Journees SF2A, Atelier S15 \u00ab\u00a0Formation and Evolution of Large Moons Around Giant Planets\u00a0\u00bb, 24 juin, 2026, Grenoble (France) &#8211; Appel \u00e0 contributions<\/h3>\n\n\n\n<p>La multiplicit\u00e9 des missions vers les lunes Galil\u00e9ennes soul\u00e8ve des questions majeures sur les conditions de formation et d\u2019\u00e9volution et diff\u00e9rentiation des satellites. Nous proposons un atelier visant \u00e0 rassembler la communaut\u00e9 fran\u00e7aise, fortement engag\u00e9e dans les missions JUNO, JUICE et Europa-Clipper ainsi que la future mission Tianwen-4. L&rsquo;objectif de cet atelier est d&rsquo;amener les personnes travaillant sur diff\u00e9rents mod\u00e8les (formation, dynamique, structure interne) afin de cr\u00e9er une communaut\u00e9 consciente des contraintes physico-chimiques issues des autres disciplines.<\/p>\n\n\n\n<p>La session rassemblera ainsi les communaut\u00e9s travaillant :<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>sur la formation des satellites dans les disques circumplan\u00e9taires et l\u2019origine du syst\u00e8me galil\u00e9en ;<\/li>\n\n\n\n<li>sur la dynamique orbitale, la stabilit\u00e9 et l\u2019entretien de la r\u00e9sonance de Laplace ;<\/li>\n\n\n\n<li>sur la mod\u00e9lisation des int\u00e9rieurs soumis aux mar\u00e9es (thermique, rh\u00e9ologie, oc\u00e9ans, couplage noyau\u2013manteau\u2013glace) ;<\/li>\n\n\n\n<li>et sur les observations (Juno, Galileo, Cassini, JUICE, Europa Clipper, observatoires au sol et spatiaux).<\/li>\n<\/ul>\n\n\n\n<p>Un parall\u00e8le sera esquiss\u00e9 avec des syst\u00e8mes exoplan\u00e9taires en cha\u00eene r\u00e9sonante tels que TRAPPIST-1, o\u00f9 des m\u00e9canismes analogues de dissipation de mar\u00e9e pourraient fa\u00e7onner l\u2019\u00e9tat interne et l\u2019\u00e9ventuelle habitabilit\u00e9, afin de mettre en perspective les enseignements du syst\u00e8me galil\u00e9en au-del\u00e0 du Syst\u00e8me solaire.<\/p>\n\n\n\n<p>Transmis par Antoine Schneeberger, Mathilde Kervazo, Sam Fayolle, Alexandre Revol, Kevin Bailli\u00e9<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">4. Conf\u00e9rence Mercury 2026, 1-4 septembre, 2026, Leuven (Belgique)<\/h3>\n\n\n\n<p>Nous avons le plaisir d\u2019annoncer la conf\u00e9rence internationale Mercury 2026, qui se tiendra du 1er au 4 septembre 2026 \u00e0 Leuven, en Belgique, sous l\u2019\u00e9gide du D\u00e9partement des sciences de la Terre et de l\u2019environnement de la KU Leuven. La conf\u00e9rence Mercury 2026 (KU Leuven\/ESA) r\u00e9unira la communaut\u00e9 internationale des sciences plan\u00e9taires afin de discuter des derni\u00e8res avanc\u00e9es en mati\u00e8re d\u2019exploration et de compr\u00e9hension de Mercure, notamment des nouvelles d\u00e9couvertes issues des missions MESSENGER et BepiColombo. La conf\u00e9rence se tiendra dans la ville historique de Louvain, en Belgique, et comprendra des pr\u00e9sentations d\u2019invit\u00e9s, des expos\u00e9s, des sessions de posters, ainsi que des occasions de discussion et de collaboration.<\/p>\n\n\n\n<p>Les th\u00e8mes abord\u00e9s comprendront : Structure interne et composition, \u00c9volution de la surface et volcanisme, Tectonique et contraction plan\u00e9taire, Exosph\u00e8re et magn\u00e9tosph\u00e8re de Mercure, Formation et diff\u00e9renciation plan\u00e9taire, et nouveaux r\u00e9sultats des missions MESSENGER et BepiColombo<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Dates cl\u00e9s : Ouverture des inscriptions :&nbsp;<strong>1er avril 2026<\/strong><\/li>\n\n\n\n<li>Soumission des r\u00e9sum\u00e9s :&nbsp;<strong>1er avril \u2013 30 juin 2026<\/strong><\/li>\n\n\n\n<li>Dates de la conf\u00e9rence : 1er \u2013 4 septembre 2026<\/li>\n<\/ul>\n\n\n\n<p>De plus amples informations (notamment sur l&rsquo;h\u00e9bergement) sont disponibles sur le site web de la conf\u00e9rence :<\/p>\n\n\n\n<p><a href=\"https:\/\/ees.kuleuven.be\/en\/mercury2026\">https:\/\/ees.kuleuven.be\/en\/mercury2026<\/a><\/p>\n\n\n\n<p>Transmis par L\u00e9a Griton, pour le SOC<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">5. Ecole Th\u00e9matique Evry Schatzman : Magn\u00e9tisme stellaire, 4-9 octobre, 2026, Roscoff (France)<\/h3>\n\n\n\n<p>L\u2019\u00e9dition 2026 de l&rsquo;Ecole Th\u00e9matique \u00ab\u00a0Evry Schatzman 2026 : Magn\u00e9tisme stellaire\u00a0\u00bb aura lieu du 4 au 9 octobre 2026 \u00e0 Roscoff et \u00a0les inscriptions sont ouvertes :\u00a0<a href=\"https:\/\/ees2026.sciencesconf.org\/\">https:\/\/ees2026.sciencesconf.org\/<\/a>.<\/p>\n\n\n\n<p>Transmis par C\u00e9line Reyl\u00e9<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">6. NECO Workshop: \u00ab\u00a0Probing the Circumstellar and Interstellar Medium with Transients and Multi-Wavelength Observations\u00a0\u00bb, 26-29 Octobre, 2026, Tokyo (Japan)<\/h3>\n\n\n\n<p>We are pleased to announce the workshop:<\/p>\n\n\n\n<p>\u00ab\u00a0Probing the Circumstellar and Interstellar Medium with Transients and Multi-Wavelength Observations\u00a0\u00bb<\/p>\n\n\n\n<p><a href=\"https:\/\/collaborations.lam.fr\/neco\/workshops\/neco_2026.html\">https:\/\/collaborations.lam.fr\/neco\/workshops\/neco_2026.html<\/a><\/p>\n\n\n\n<p>Dates: 26-29 October 2026<\/p>\n\n\n\n<p>Location: Waseda University, Tokyo, Japan<\/p>\n\n\n\n<figure class=\"wp-block-embed is-type-wp-embed is-provider-waseda-university wp-block-embed-waseda-university\"><div class=\"wp-block-embed__wrapper\">\n<blockquote class=\"wp-embedded-content\" data-secret=\"XanbGxdyFA\"><a href=\"https:\/\/www.waseda.jp\/top\/en\/access\/nishiwaseda-campus\">Nishiwaseda Campus<\/a><\/blockquote><iframe loading=\"lazy\" class=\"wp-embedded-content\" sandbox=\"allow-scripts\" security=\"restricted\" style=\"position: absolute; visibility: hidden;\" title=\"&#8220;Nishiwaseda Campus&#8221; &#8212; Waseda University\" src=\"https:\/\/www.waseda.jp\/top\/en\/access\/nishiwaseda-campus\/embed#?secret=Zr4aS8a9JU#?secret=XanbGxdyFA\" data-secret=\"XanbGxdyFA\" width=\"500\" height=\"282\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\"><\/iframe>\n<\/div><\/figure>\n\n\n\n<p>This workshop will bring together researchers working on transients (SNe, GRBs, FRBs) and galaxy evolution&nbsp;<\/p>\n\n\n\n<p>to explore the multi-scale structure of baryonic matter, from circumstellar environments to the intergalactic medium.<\/p>\n\n\n\n<p>Topics will include:<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Multi-wavelength observations (JWST, ALMA, NOEMA, PFS, SKA)<\/li>\n\n\n\n<li>CSM studies with early supernova observations<\/li>\n\n\n\n<li>ISM in GRB host galaxies<\/li>\n\n\n\n<li>FRB dispersion measures and CGM\/IGM<\/li>\n\n\n\n<li>Quasar spectroscopy and BAL regions<\/li>\n\n\n\n<li>Dust evolution and feedback<\/li>\n\n\n\n<li>Toward a unified multi-scale framework (CSM to CGM\/IGM)<\/li>\n<\/ul>\n\n\n\n<p>The workshop will include dedicated discussion sessions to foster collaboration, particularly between Japanese and French teams.<\/p>\n\n\n\n<p>Preliminary registration:&nbsp;<a href=\"https:\/\/docs.google.com\/forms\/d\/e\/1FAIpQLScdPOgW9C4vB6zLM9ryA8Gw7mYUcsbT0BErAdnzOCIiycGmug\/viewform?embedded=true\">https:\/\/docs.google.com\/forms\/d\/e\/1FAIpQLScdPOgW9C4vB6zLM9ryA8Gw7mYUcsbT0BErAdnzOCIiycGmug\/viewform?embedded=true<\/a><\/p>\n\n\n\n<p>Transmis par Akio Inoue and Denis Burgarella<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">7. LATMOS Seminar April 14th &#8211; Jorge HERN\u00c1NDEZ BERNAL &#8211; Martian aerosols investigated with imagers and high resolution models<\/h3>\n\n\n\n<p>On Tuesday April 14th, Jorge HERN\u00c1NDEZ BERNAL (LMD) will give a seminar on \u00ab\u00a0Martian aerosols investigated with imagers and high resolution models\u00a0\u00bb. The seminar will take place at\u00a0<strong>11:30am<\/strong>\u00a0in LATMOS Guyancourt in room 2202. It will be retransmitted on Webinaire.<\/p>\n\n\n\n<p><a href=\"https:\/\/webinaire.numerique.gouv.fr\/meeting\/signin\/invite\/74758\/creator\/43688\/hash\/ba23115e3882fabc45cfd8a4dfa7b8c53ea754cc\">https:\/\/webinaire.numerique.gouv.fr\/meeting\/signin\/invite\/74758\/creator\/43688\/hash\/ba23115e3882fabc45cfd8a4dfa7b8c53ea754cc<\/a><\/p>\n\n\n\n<p>The research of Martian aerosols is often based on global surveys by point-spectrometers that capture the global trends, and the reproduction of such trends with models. Imagers offer a different kind of coverage and enable a different approach to the research of Martian aerosols. They provide details on the morphology and dynamics of aerosol masses, enable analysis of sol-to-sol meteorological variations, provide context for other kinds of observations, and in some cases can provide information on aspects hardly accessible for retrievals by point-spectrometers. Imagers become particularly powerful when they are combined with high resolution models (whether mesoscale of high resolution GCMs), enabling new kinds of comparisons. In this seminar I will talk about my work and research ideas on this line.<\/p>\n\n\n\n<p>Transmis par Audrey Chatain<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">8. Le num\u00e9ro d&rsquo;avril du magazine de la SAF l\u2019Astronomie est paru<\/h3>\n\n\n\n<p>Le num\u00e9ro d&rsquo;avril (n\u00b0203) du magazine de la SAF l\u2019Astronomie est paru.<\/p>\n\n\n\n<p>Dans les Actualit\u00e9s T. Encrenaz (OP), S.Collin-Zahn (OP) et F. Deschamps (IESA,Taiwan) pr\u00e9sentent l&rsquo;observation d&rsquo;une exoplan\u00e8te autour d&rsquo;une \u00e9toile double, une barre de fer inexpliqu\u00e9e au sein d&rsquo;une n\u00e9buleuse plan\u00e9taire, une nouvelle hypoth\u00e8se expliquant l&rsquo;origine du champ magn\u00e9tique terrestre, l&rsquo;apport de Gaia \u00e0 l&rsquo;histoire des ast\u00e9ro\u00efdes.<\/p>\n\n\n\n<p>Dans la rubrique \u00ab\u00a0Spatial\u00a0\u00bb S. S\u00e9bille (SAF) raconte les d\u00e9buts de Sophie Adenot, dans la station spatiale internationale et la vie \u00e0 bord. F Mottez (OP) nous renseigne la mission IMAP charg\u00e9e de l&rsquo;\u00e9tude de l&rsquo;h\u00e9liosph\u00e8re. W. Huan et C. Bao (Acad\u00e9mie chinoise des Sciences) pr\u00e9sentent la mission chinoise \u00ab\u00a0Einstein Probe\u00a0\u00bb \u00e9tudiant les ph\u00e9nom\u00e8nes transitoires en rayons X. Dans le Zoom, L. Amard et S. Brun (Cea-Saclay) pr\u00e9voient le champ magn\u00e9tique du Soleil alors qu&rsquo;il sera devenu une g\u00e9ante rouge. Dans la rubrique Histoire, J.-M. Faidit (SAF) explique l&rsquo;ing\u00e9nieuse invention de F. Ouvi\u00e8re, le Cosmographe, permettant la pr\u00e9sentation p\u00e9dagogique des mouvements de la Terre.<\/p>\n\n\n\n<p>Observations &amp; Travaux pr\u00e9sente la d\u00e9couverte de la com\u00e8te C\/2026 A1 (MAPS) par un groupe d&rsquo;astronomes amateurs, G. Attard, A. Maury, F. Signoret, D. Huber.<\/p>\n\n\n\n<p>Du c\u00f4t\u00e9 Observations, G. Sautot et E. Evrard (SAF) nous invitent \u00e0 observer la galaxie M83. K. Antier (SAF) s&rsquo;inqui\u00e8te du projet \u00ab\u00a0Reflect Orbital\u00a0\u00bb qui \u00e9claire le ciel nocturne comme un phare c\u00e9leste.<\/p>\n\n\n\n<p>Pour vous informer sur le num\u00e9ro en cours et les num\u00e9ros pr\u00e9c\u00e9dents, vous abonner, ou abonner votre laboratoire, voir&nbsp;<a href=\"https:\/\/lastronomie.fr\/\">https:\/\/lastronomie.fr.<\/a><\/p>\n\n\n\n<p>Transmis par Nicole Mein<\/p>\n\n\n\n<h3 class=\"wp-block-heading\">9. Annonce de parution Cahiers Clairaut 193<\/h3>\n\n\n\n<p>Le n\u00b0 193 (mars 2026) du trimestriel \u00ab\u00a0Les Cahiers Clairaut\u00a0\u00bb, la revue du Comit\u00e9 de liaison enseignants et astronomes (Clea), est paru.<\/p>\n\n\n\n<p>Actualit\u00e9 de l&rsquo;ann\u00e9e oblige, le dossier th\u00e9matique de ce num\u00e9ro est consacr\u00e9 aux \u00e9clipses solaires. Au sommaire : Pascal Descamps (Obs. de Paris) explique les r\u00e9currences des \u00e9clipse solaires, B\u00e9atrice Sandr\u00e9 d\u00e9taille le mouvement de l&rsquo;ombre de la Lune \u00e0 la surface terrestre et David Alberto nous d\u00e9voile le fonctionnement de l&rsquo;Astronomical rotula, une maquette du XVIIIe si\u00e8cle qui permet de pr\u00e9voir les \u00e9clipses. Hors th\u00e8me du dossier, Th\u00e9r\u00e8ze Encrenaz (Obs. de Paris) nous emm\u00e8ne explorer les exoplan\u00e8tes.<\/p>\n\n\n\n<p>Le sommaire est \u00e0 d\u00e9couvrir l\u00e0 :&nbsp;<a href=\"http:\/\/clea-astro.eu\/vieclea\/productions-recentes\/cc\/cc193\/les-cahiers-clairaut-nb0-193-printemps-2026\">http:\/\/clea-astro.eu\/vieclea\/productions-recentes\/cc\/cc193\/les-cahiers-clairaut-nb0-193-printemps-2026<\/a><\/p>\n\n\n\n<p>Soutenez nos actions en nous rejoignant et\/ou en abonnant votre institution. Et bien entendu, vous pouvez toujours nous proposer articles et activit\u00e9s p\u00e9dagogiques pour publication.<\/p>\n\n\n\n<p>Transmis par Fr\u00e9d\u00e9ric Pitout<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\"\/>\n\n\n\n<p>Pour faire passer vos messages, envoyez un mail au secr\u00e9tariat SF2A (<a href=\"mailto:secretariat@sf2a.eu\">secretariat@sf2a.eu<\/a>) avant le vendredi 18h pour une diffusion le lundi apr\u00e8s-midi suivant.<\/p>\n\n\n\n<p>Pour se d\u00e9sabonner de la newsletter, rendez-vous dans votre espace MaSF2A (<a href=\"http:\/\/www.ma.sf2a.eu\/\">www.ma.sf2a.eu<\/a>)&gt;Annuaire&gt;G\u00e9rer votre fiche.<\/p>\n","protected":false},"excerpt":{"rendered":"<h4>Message SF2A No 1179 &#8211; 06\/04\/26<\/h4>\n<p>\n1. OPTICON Call for Proposals 2026<br \/>\n2. Call for NRT proposals &#8211; 2026B<br \/>\n3. Journees SF2A, Atelier S15 \u00ab\u00a0Formation and Evolution of Large Moons Around Giant Planets\u00a0\u00bb, 24 juin, 2026, Grenoble (France) &#8211; Appel \u00e0 contributions<br \/>\n4. Conf\u00e9rence Mercury 2026, 1-4 septembre, 2026, Leuven (Belgique)<br \/>\n5. Ecole Th\u00e9matique Evry Schatzman : Magn\u00e9tisme stellaire, 4-9 octobre, 2026, Roscoff (France)<br \/>\n6. NECO Workshop: \u00ab\u00a0Probing the Circumstellar and Interstellar Medium with Transients and Multi-Wavelength Observations\u00a0\u00bb, 26-29 Octobre, 2026, Tokyo (Japan)<br \/>\n7. LATMOS Seminar April 14th &#8211; Jorge HERN\u00c1NDEZ BERNAL &#8211; Martian aerosols investigated with imagers and high resolution models<br \/>\n8. Le num\u00e9ro d&rsquo;avril du magazine de la SAF l\u2019Astronomie est paru<br \/>\n9. Annonce de parution Cahiers Clairaut 193<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"saved_in_kubio":false,"footnotes":""},"categories":[1],"tags":[],"class_list":["post-2891","post","type-post","status-publish","format-standard","hentry","category-uncategorized"],"_links":{"self":[{"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/posts\/2891","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/comments?post=2891"}],"version-history":[{"count":1,"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/posts\/2891\/revisions"}],"predecessor-version":[{"id":2892,"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/posts\/2891\/revisions\/2892"}],"wp:attachment":[{"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/media?parent=2891"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/categories?post=2891"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/sf2a.eu\/website2023\/wp-json\/wp\/v2\/tags?post=2891"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}