2022N35 - criteri di valutazione titoli e prove d'esame

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2022PA560 Lettera - SSD: L-FIL-LET/10 - SC: 10/F1 - dipartimento DISLL;

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Procedure valutative per professori di seconda fascia

Array ( [body] => Array ( [#theme] => field [#weight] => -4 [#title] => Body [#access] => 1 [#label_display] => hidden [#view_mode] => teaser [#language] => und [#field_name] => body [#field_type] => text_with_summary [#field_translatable] => 0 [#entity_type] => node [#bundle] => foglia_complessa [#object] => stdClass Object ( [vid] => 407335 [uid] => 32 [title] => Procedure valutative per professori di seconda fascia [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92080 [type] => foglia_complessa [language] => it [created] => 1661951219 [changed] => 1667382880 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382880 [revision_uid] => 4 [taxonomy_vocabulary_2] => Array ( ) [taxonomy_vocabulary_3] => Array ( ) [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[summary] => [format] => 2 [safe_value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[safe_summary] => ) ) ) [field_foglia_complessa_accordion] => Array ( [und] => Array ( [0] => Array ( [nid] => 92079 [access] => 1 [node] => stdClass Object ( [vid] => 407334 [uid] => 8831 [title] => 2022PA560 - Bando parte generale e allegati [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92079 [type] => accordion [language] => it [created] => 1661951216 [changed] => 1667382877 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382877 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 92078 [access] => 1 ) [1] => Array ( [nid] => 92081 [access] => 1 ) [2] => Array ( [nid] => 93295 [access] => 1 ) [3] => Array ( [nid] => 93615 [access] => 1 ) [4] => Array ( [nid] => 93977 [access] => 1 ) [5] => Array ( [nid] => 93978 [access] => 1 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 6 [current_revision_id] => 407334 [is_current] => 1 [is_pending] => [revision_moderation] => [entity_view_prepared] => 1 ) ) [1] => Array ( [nid] => 58783 [access] => 1 [node] => stdClass Object ( [vid] => 438805 [uid] => 8831 [title] => Concorsi docenti altre informazioni [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 58783 [type] => accordion [language] => it [created] => 1559112888 [changed] => 1697443786 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1697443786 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[summary] => [format] => 2 [safe_value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[safe_summary] => ) ) ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( [und] => Array ( [0] => Array ( [value] =>

Altre informazioni

[format] => 1 [safe_value] =>

Altre informazioni

) ) ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 58782 ) [1] => Array ( [nid] => 82541 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 18 [current_revision_id] => 438805 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) ) [field_foglia_complessa_allegato] => Array ( ) [field_image_fc] => Array ( ) [field_testo_opzionale_fc] => Array ( [und] => Array ( [0] => Array ( [nid] => 8456 [access] => 1 [node] => stdClass Object ( [vid] => 443433 [uid] => 4 [title] => Ufficio Personale docente - Settore Reclutamento [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 8456 [type] => testo_opzionale [language] => und [created] => 1341050862 [changed] => 1701255566 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1701255566 [revision_uid] => 4 [field_testo_opz] => Array ( [und] => Array ( [0] => Array ( [value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

[format] => 1 [safe_value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

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Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[summary] => [format] => 2 [safe_value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[safe_summary] => ) ) [#formatter] => text_summary_or_trimmed [0] => Array ( [#markup] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

) ) [field_foglia_complessa_accordion] => Array ( [#theme] => field [#weight] => -1 [#title] => accordion [#access] => 1 [#label_display] => above [#view_mode] => teaser [#language] => und [#field_name] => field_foglia_complessa_accordion [#field_type] => node_reference [#field_translatable] => 0 [#entity_type] => node [#bundle] => foglia_complessa [#object] => stdClass Object ( [vid] => 407335 [uid] => 32 [title] => Procedure valutative per professori di seconda fascia [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92080 [type] => foglia_complessa [language] => it [created] => 1661951219 [changed] => 1667382880 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382880 [revision_uid] => 4 [taxonomy_vocabulary_2] => Array ( ) [taxonomy_vocabulary_3] => Array ( ) [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[summary] => [format] => 2 [safe_value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[safe_summary] => ) ) ) [field_foglia_complessa_accordion] => Array ( [und] => Array ( [0] => Array ( [nid] => 92079 [access] => 1 [node] => stdClass Object ( [vid] => 407334 [uid] => 8831 [title] => 2022PA560 - Bando parte generale e allegati [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92079 [type] => accordion [language] => it [created] => 1661951216 [changed] => 1667382877 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382877 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 92078 [access] => 1 ) [1] => Array ( [nid] => 92081 [access] => 1 ) [2] => Array ( [nid] => 93295 [access] => 1 ) [3] => Array ( [nid] => 93615 [access] => 1 ) [4] => Array ( [nid] => 93977 [access] => 1 ) [5] => Array ( [nid] => 93978 [access] => 1 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 6 [current_revision_id] => 407334 [is_current] => 1 [is_pending] => [revision_moderation] => [entity_view_prepared] => 1 ) ) [1] => Array ( [nid] => 58783 [access] => 1 [node] => stdClass Object ( [vid] => 438805 [uid] => 8831 [title] => Concorsi docenti altre informazioni [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 58783 [type] => accordion [language] => it [created] => 1559112888 [changed] => 1697443786 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1697443786 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[summary] => [format] => 2 [safe_value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[safe_summary] => ) ) ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( [und] => Array ( [0] => Array ( [value] =>

Altre informazioni

[format] => 1 [safe_value] =>

Altre informazioni

) ) ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 58782 ) [1] => Array ( [nid] => 82541 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 18 [current_revision_id] => 438805 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) ) [field_foglia_complessa_allegato] => Array ( ) [field_image_fc] => Array ( ) [field_testo_opzionale_fc] => Array ( [und] => Array ( [0] => Array ( [nid] => 8456 [access] => 1 [node] => stdClass Object ( [vid] => 443433 [uid] => 4 [title] => Ufficio Personale docente - Settore Reclutamento [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 8456 [type] => testo_opzionale [language] => und [created] => 1341050862 [changed] => 1701255566 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1701255566 [revision_uid] => 4 [field_testo_opz] => Array ( [und] => Array ( [0] => Array ( [value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

[format] => 1 [safe_value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

) ) ) [name] => simonetta.capparotto [picture] => 0 [data] => a:2:{s:13:"form_build_id";s:37:"form-fe5ebd9e5e240c4294455b6b42fa6a76";s:14:"wysiwyg_status";a:1:{i:1;i:1;}} [num_revisions] => 21 [current_revision_id] => 443433 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) ) [field_immagine_top] => Array ( ) [field_immagine_bottom] => Array ( ) [field_immagine_decorativa_latera] => Array ( [und] => Array ( [0] => Array ( [fid] => 72106 [uid] => 4 [filename] => selezioni.png [uri] => public://selezioni.png [filemime] => image/png [filesize] => 67347 [status] => 1 [timestamp] => 1634297584 [type] => image [field_file_image_alt_text] => Array ( [und] => Array ( [0] => Array ( [value] => Immagine decorativa [format] => [safe_value] => Immagine decorativa ) ) ) [field_file_image_title_text] => Array ( ) [field_folder] => Array ( [und] => Array ( [0] => Array ( [tid] => 2048 ) ) ) [metatags] => Array ( [und] => Array ( [title] => Array ( [value] => [current-page:title] | [current-page:pager][site:name] [default] => [current-page:title] | [current-page:pager][site:name] ) [description] => Array ( [value] => ) [abstract] => Array ( [value] => ) [keywords] => Array ( [value] => ) [robots] => Array ( [value] => Array ( [index] => 0 [follow] => 0 [noindex] => 0 [nofollow] => 0 [noarchive] => 0 [nosnippet] => 0 [noodp] => 0 [noydir] => 0 [noimageindex] => 0 [notranslate] => 0 ) ) [news_keywords] => Array ( [value] => ) [standout] => Array ( [value] => ) [rating] => Array ( [value] => ) [referrer] => Array ( [value] => ) [rights] => Array ( [value] => ) [image_src] => Array ( [value] => ) [canonical] => Array ( [value] => [current-page:url:absolute] [default] => [current-page:url:absolute] ) [set_cookie] => Array ( [value] => ) [shortlink] => Array ( [value] => [current-page:url:unaliased] [default] => [current-page:url:unaliased] ) [original-source] => Array ( [value] => ) [prev] => Array ( [value] => ) [next] => Array ( [value] => ) [content-language] => Array ( [value] => ) [geo.position] => Array ( [value] => ) [geo.placename] => Array ( [value] => ) [geo.region] => Array ( [value] => ) [icbm] => Array ( [value] => ) [refresh] => Array ( [value] => ) [revisit-after] => Array ( [value] => [period] => ) [pragma] => Array ( [value] => ) [cache-control] => Array ( [value] => ) [expires] => Array ( [value] => ) [og:type] => Array ( [value] => article [default] => article ) [og:url] => Array ( [value] => [current-page:url:absolute] [default] => [current-page:url:absolute] ) [og:title] => Array ( [value] => [current-page:title] [default] => [current-page:title] ) [og:determiner] => Array ( [value] => ) [og:description] => Array ( [value] => ) [og:updated_time] => Array ( [value] => ) [og:see_also] => Array ( [value] => ) [og:image] => Array ( [value] => ) [og:image:url] => Array ( [value] => ) [og:image:secure_url] => Array ( [value] => ) [og:image:type] => Array ( [value] => ) [og:image:width] => Array ( [value] => ) [og:image:height] => Array ( [value] => ) [og:latitude] => Array ( [value] => ) [og:longitude] => Array ( [value] => ) [og:street_address] => Array ( [value] => ) [og:locality] => Array ( [value] => ) [og:region] => Array ( [value] => ) [og:postal_code] => Array ( [value] => ) [og:country_name] => Array ( [value] => ) [og:email] => Array ( [value] => ) [og:phone_number] => Array ( [value] => ) [og:fax_number] => Array ( [value] => ) [og:locale] => Array ( [value] => ) [og:locale:alternate] => Array ( [value] => ) [article:author] => Array ( [value] => ) [article:publisher] => Array ( [value] => ) [article:section] => Array ( [value] => ) [article:tag] => Array ( [value] => ) [article:published_time] => Array ( [value] => ) [article:modified_time] => Array ( [value] => ) [article:expiration_time] => Array ( [value] => ) [profile:first_name] => Array ( [value] => ) [profile:last_name] => Array ( [value] => ) [profile:username] => Array ( [value] => ) [profile:gender] => Array ( [value] => ) [og:audio] => Array ( [value] => ) [og:audio:secure_url] => Array ( [value] => ) [og:audio:type] => Array ( [value] => ) [book:author] => Array ( [value] => ) [book:isbn] => Array ( [value] => ) [book:release_date] => Array ( [value] => ) [book:tag] => Array ( [value] => ) [og:video:url] => Array ( [value] => ) [og:video:secure_url] => Array ( [value] => ) [og:video:width] => Array ( [value] => ) [og:video:height] => Array ( [value] => ) [og:video:type] => Array ( [value] => ) [video:actor] => Array ( [value] => ) [video:actor:role] => Array ( [value] => ) [video:director] => Array ( [value] => ) [video:writer] => Array ( [value] => ) [video:duration] => Array ( [value] => ) [video:release_date] => Array ( [value] => ) [video:tag] => Array ( [value] => ) [video:series] => Array ( [value] => ) ) ) [alt] => Immagine decorativa [metadata] => Array ( [height] => 1363 [width] => 550 ) [height] => 1363 [width] => 550 [title] => ) ) ) [field_link_in_evidenza] => Array ( ) [field_usa_layout_pagina_link] => Array ( [und] => Array ( [0] => Array ( [value] => 0 ) ) ) [field_etichetta_link_in_evidenza] => Array ( ) [field_tabs] => Array ( ) [field_condividi_social] => Array ( [und] => Array ( [0] => Array ( [value] => 1 ) ) ) [field_formato_immagine] => Array ( ) [field_video_link] => Array ( ) [field_nosidebar] => Array ( [und] => Array ( [0] => Array ( [value] => 0 ) ) ) [field_chatbot] => Array ( [und] => Array ( [0] => Array ( [value] => 0 ) ) ) [field_chatbot_codice_chat] => Array ( ) [field_header_custom] => Array ( [und] => Array ( [0] => Array ( [value] => 0 ) ) ) [field_header_custom_ref] => Array ( ) [field_accessiway] => Array ( [und] => Array ( [0] => Array ( [value] => 0 ) ) ) [field_footer_custom] => Array ( ) [field_footer_custom_ref] => Array ( ) [field_usa_layout_hero] => Array ( ) [field_note_interne] => Array ( ) [field_url_en_page] => Array ( ) [field_crawler_ai] => Array ( ) [path] => Array ( [pathauto] => 0 ) [name] => stefano.zampieri [picture] => 0 [data] => a:2:{s:13:"form_build_id";s:48:"form-WsCySmos4vAVlyFhG6gU5T7knfAyqco8LxlocSU_yIA";s:14:"wysiwyg_status";a:1:{i:1;i:1;}} [num_revisions] => 4 [current_revision_id] => 407335 [is_current] => 1 [is_pending] => [revision_moderation] => [entity_view_prepared] => 1 ) [#items] => Array ( [0] => Array ( [nid] => 92079 [access] => 1 [node] => stdClass Object ( [vid] => 407334 [uid] => 8831 [title] => 2022PA560 - Bando parte generale e allegati [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92079 [type] => accordion [language] => it [created] => 1661951216 [changed] => 1667382877 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382877 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 92078 [access] => 1 ) [1] => Array ( [nid] => 92081 [access] => 1 ) [2] => Array ( [nid] => 93295 [access] => 1 ) [3] => Array ( [nid] => 93615 [access] => 1 ) [4] => Array ( [nid] => 93977 [access] => 1 ) [5] => Array ( [nid] => 93978 [access] => 1 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 6 [current_revision_id] => 407334 [is_current] => 1 [is_pending] => [revision_moderation] => [entity_view_prepared] => 1 ) ) [1] => Array ( [nid] => 58783 [access] => 1 [node] => stdClass Object ( [vid] => 438805 [uid] => 8831 [title] => Concorsi docenti altre informazioni [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 58783 [type] => accordion [language] => it [created] => 1559112888 [changed] => 1697443786 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1697443786 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[summary] => [format] => 2 [safe_value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[safe_summary] => ) ) ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( [und] => Array ( [0] => Array ( [value] =>

Altre informazioni

[format] => 1 [safe_value] =>

Altre informazioni

) ) ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 58782 ) [1] => Array ( [nid] => 82541 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 18 [current_revision_id] => 438805 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) [#formatter] => node_reference_default [0] => Array ( [#type] => link [#title] => 2022PA560 - Bando parte generale e allegati [#href] => node/92079 [#options] => Array ( [entity_type] => node [entity] => stdClass Object ( [vid] => 407334 [uid] => 8831 [title] => 2022PA560 - Bando parte generale e allegati [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92079 [type] => accordion [language] => it [created] => 1661951216 [changed] => 1667382877 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382877 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 92078 [access] => 1 ) [1] => Array ( [nid] => 92081 [access] => 1 ) [2] => Array ( [nid] => 93295 [access] => 1 ) [3] => Array ( [nid] => 93615 [access] => 1 ) [4] => Array ( [nid] => 93977 [access] => 1 ) [5] => Array ( [nid] => 93978 [access] => 1 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 6 [current_revision_id] => 407334 [is_current] => 1 [is_pending] => [revision_moderation] => [entity_view_prepared] => 1 ) ) ) [1] => Array ( [#type] => link [#title] => Concorsi docenti altre informazioni [#href] => node/58783 [#options] => Array ( [entity_type] => node [entity] => stdClass Object ( [vid] => 438805 [uid] => 8831 [title] => Concorsi docenti altre informazioni [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 58783 [type] => accordion [language] => it [created] => 1559112888 [changed] => 1697443786 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1697443786 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[summary] => [format] => 2 [safe_value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[safe_summary] => ) ) ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( [und] => Array ( [0] => Array ( [value] =>

Altre informazioni

[format] => 1 [safe_value] =>

Altre informazioni

) ) ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 58782 ) [1] => Array ( [nid] => 82541 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 18 [current_revision_id] => 438805 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) ) [links] => Array ( [#theme] => links__node [#pre_render] => Array ( [0] => drupal_pre_render_links ) [#attributes] => Array ( [class] => Array ( [0] => links [1] => inline ) ) [node] => Array ( [#theme] => links__node__node [#links] => Array ( [node-readmore] => Array ( [title] => Read more about Procedure valutative per professori di seconda fascia [href] => node/92080 [html] => 1 [attributes] => Array ( [rel] => tag [title] => Procedure valutative per professori di seconda fascia ) ) ) [#attributes] => Array ( [class] => Array ( [0] => links [1] => inline ) ) ) ) [field_testo_opzionale_fc] => Array ( [#theme] => field [#weight] => 1 [#title] => Testo Opzionale [#access] => 1 [#label_display] => above [#view_mode] => teaser [#language] => und [#field_name] => field_testo_opzionale_fc [#field_type] => node_reference [#field_translatable] => 0 [#entity_type] => node [#bundle] => foglia_complessa [#object] => stdClass Object ( [vid] => 407335 [uid] => 32 [title] => Procedure valutative per professori di seconda fascia [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92080 [type] => foglia_complessa [language] => it [created] => 1661951219 [changed] => 1667382880 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382880 [revision_uid] => 4 [taxonomy_vocabulary_2] => Array ( ) [taxonomy_vocabulary_3] => Array ( ) [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[summary] => [format] => 2 [safe_value] =>

Il documento ufficiale è reperibile all’Albo on line di Ateneo

Procedura valutativa per la chiamata di un Professore di seconda fascia, ai sensi dell’art. 24, comma 5, Legge 30 dicembre 2010, n. 240, riservata a ricercatori a tempo determinato di cui all’art. 24 comma 3 lett. b) della Legge 30 dicembre 2010, n.240 nel terzo anno del contratto triennale di lavoro subordinato, a tempo determinato, stipulato con la medesima Università ed in possesso dell’Abilitazione Scientifica Nazionale ai sensi dell’art. 16 della Legge 30 dicembre 2010, n. 240 – 2022PA560

Scadenza: 22 settembre 2022, ore 13

Domanda telematica

[safe_summary] => ) ) ) [field_foglia_complessa_accordion] => Array ( [und] => Array ( [0] => Array ( [nid] => 92079 [access] => 1 [node] => stdClass Object ( [vid] => 407334 [uid] => 8831 [title] => 2022PA560 - Bando parte generale e allegati [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 92079 [type] => accordion [language] => it [created] => 1661951216 [changed] => 1667382877 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1667382877 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 92078 [access] => 1 ) [1] => Array ( [nid] => 92081 [access] => 1 ) [2] => Array ( [nid] => 93295 [access] => 1 ) [3] => Array ( [nid] => 93615 [access] => 1 ) [4] => Array ( [nid] => 93977 [access] => 1 ) [5] => Array ( [nid] => 93978 [access] => 1 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 6 [current_revision_id] => 407334 [is_current] => 1 [is_pending] => [revision_moderation] => [entity_view_prepared] => 1 ) ) [1] => Array ( [nid] => 58783 [access] => 1 [node] => stdClass Object ( [vid] => 438805 [uid] => 8831 [title] => Concorsi docenti altre informazioni [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 58783 [type] => accordion [language] => it [created] => 1559112888 [changed] => 1697443786 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1697443786 [revision_uid] => 4 [taxonomy_vocabulary_8] => Array ( ) [body] => Array ( [und] => Array ( [0] => Array ( [value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[summary] => [format] => 2 [safe_value] =>

Per il rimborso spese di missione consultare la pagina dedicata

[safe_summary] => ) ) ) [field_accordion_element] => Array ( ) [field_accordion_sottotitolo] => Array ( ) [field_accordion_titolo_fro] => Array ( [und] => Array ( [0] => Array ( [value] =>

Altre informazioni

[format] => 1 [safe_value] =>

Altre informazioni

) ) ) [field_allegato_element] => Array ( [und] => Array ( [0] => Array ( [nid] => 58782 ) [1] => Array ( [nid] => 82541 ) ) ) [name] => carriere.docenti [picture] => 0 [data] => [num_revisions] => 18 [current_revision_id] => 438805 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) ) [field_foglia_complessa_allegato] => Array ( ) [field_image_fc] => Array ( ) [field_testo_opzionale_fc] => Array ( [und] => Array ( [0] => Array ( [nid] => 8456 [access] => 1 [node] => stdClass Object ( [vid] => 443433 [uid] => 4 [title] => Ufficio Personale docente - Settore Reclutamento [log] => [status] => 1 [comment] => 0 [promote] => 1 [sticky] => 0 [nid] => 8456 [type] => testo_opzionale [language] => und [created] => 1341050862 [changed] => 1701255566 [tnid] => 0 [translate] => 0 [revision_timestamp] => 1701255566 [revision_uid] => 4 [field_testo_opz] => Array ( [und] => Array ( [0] => Array ( [value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

[format] => 1 [safe_value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

) ) ) [name] => simonetta.capparotto [picture] => 0 [data] => a:2:{s:13:"form_build_id";s:37:"form-fe5ebd9e5e240c4294455b6b42fa6a76";s:14:"wysiwyg_status";a:1:{i:1;i:1;}} [num_revisions] => 21 [current_revision_id] => 443433 [is_current] => 1 [is_pending] => [revision_moderation] => ) ) ) ) [field_immagine_top] => Array ( ) [field_immagine_bottom] => Array ( ) [field_immagine_decorativa_latera] => Array ( [und] => Array ( [0] => Array ( [fid] => 72106 [uid] => 4 [filename] => selezioni.png [uri] => public://selezioni.png [filemime] => image/png [filesize] => 67347 [status] => 1 [timestamp] => 1634297584 [type] => image [field_file_image_alt_text] => Array ( [und] => Array ( [0] => Array ( [value] => Immagine decorativa [format] => [safe_value] => Immagine decorativa ) ) ) [field_file_image_title_text] => Array ( ) [field_folder] => Array ( [und] => Array ( [0] => Array ( [tid] => 2048 ) ) ) [metatags] => Array ( [und] => Array ( [title] => Array ( [value] => [current-page:title] | 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Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

[format] => 1 [safe_value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

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Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

[format] => 1 [safe_value] =>

Ufficio Personale docente - Settore Reclutamento

Palazzo Storione
Riviera Tito Livio 6, 35123 Padova
tel. 049 827 3936/ 3170/ 3172/ 3173/ 3176/ 3162/ 3178/ 1934/ 3035/ 1937/ 1929/ 3994/ 3288
email: reclutamento.docenti@unipd.it

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2022PA560 - Bando parte generale e allegati

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2022PA560 - Lettera pubblicazione avviso

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Calendario orali e link zoom - Dottorato nazionale in Scientific, Technological and Social Methods Enabling Circular Economy

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2022N24 - Comunicazione data e sede prova suppletiva

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Unipd-INAF Research: Measuring the "Fuel" of Galaxies from 4 billion Years Ago

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

[safe_summary] => ) ) ) [field_date_box_lancio_news] => Array ( [und] => Array ( [0] => Array ( [value] => 2022-08-31T00:00:00 [timezone] => Europe/Paris [timezone_db] => Europe/Paris [date_type] => date ) ) ) [field_etichetta_box_lancio_news] => Array ( ) [field_img_box_lancio_news] => Array ( [und] => Array ( [0] => Array ( [fid] => 110014 [uid] => 2032 [filename] => picture_PR.png [uri] => public://picture_PR_0.png [filemime] => image/png [filesize] => 165629 [status] => 1 [timestamp] => 1661948809 [type] => image [field_file_image_alt_text] => Array ( ) [field_file_image_title_text] => Array ( ) [field_folder] => Array ( [und] => Array ( [0] => Array ( [tid] => 2048 ) ) ) [metadata] => Array ( [height] => 227 [width] => 677 ) [height] => 227 [width] => 677 [alt] => space [title] => ) ) ) [field_link_alla_news] => Array ( ) [field_link_esterno_news] => Array ( ) [field_pagina_associata] => Array ( ) [field_link_etichetta] => Array ( ) [field_abstract_news] => Array ( [und] => Array ( [0] => Array ( [value] => A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua in association with the National Institute of Astrophysics, published a work wich measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time [format] => [safe_value] => A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua in association with the National Institute of Astrophysics, published a work wich measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time ) ) ) [field_allegato_news] => Array ( ) [field_categorie_news] => Array ( [und] => Array ( [0] => Array ( [tid] => 2296 ) ) ) [field_pub_date] => Array ( [und] => Array ( [0] => Array ( [value] => 2022-08-31T00:00:00 [value2] => 2023-08-31T00:00:00 [timezone] => Europe/Paris [timezone_db] => Europe/Paris [date_type] => date ) ) ) [field_layout_news] => Array ( [und] => Array ( [0] => Array ( [value] => single ) ) ) [field_testo_opzionale_news] => Array ( ) [field_url_en_page] => Array ( ) [field_url_en_page_label] => Array ( ) [path] => Array ( [pathauto] => 1 ) [name] => francesca.forzan [picture] => 0 [data] => b:0; 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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Star formation occurs with the collapse of dense molecular hydrogen clouds when neutral hydrogen atoms bond together. A galaxy "consumes" neutral hydrogen and transforms it into molecular hydrogen that subsequently forms stars. To keep the active formation of new stars, a galaxy must have a continuous supply of atomic hydrogen.
But how is new neutral hydrogen generated within galaxies? The scientific literature suggests two options: the intergalactic medium diffuses an accretion of gas (cosmological accretion) or by the fusion of galaxies (galaxy merger). The only place where the relationships binding neutral hydrogen to other observable properties of galaxies have been observed are in the nearby Universe, corresponding to the last billion years

A team of researchers led by the PhD student, Francesco Sinigaglia, of the University of Padua Galileo Galilei Department of Physics and Astronomy in association with the National Institute of Astrophysics, published the article MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5 in The Astrophysical Journal Letters. Together with researchers from MIGHTEE (MeerKAT International GHz Tiered Extragalactic Exploration), the work measured the relationships that link the mass of atomic hydrogen to stellar mass and the rate of star formation in galaxies at a distance corresponding to 4 billion years ago for the first time.

Francesco Sinigaglia, first author of the study, explains, "At a distance never before reached, we have observed how the variation of atomic hydrogen changes as a function of the number of stars and the rate of star formation found in distant active galaxies (star-forming). Our results indicate that galaxies found at a distance of 4-5 billion years hold reserves of atomic hydrogen comparable to those of current galaxies, especially in the case of massive galaxies. Knowing that the formation of stars rapidly consumes atomic hydrogen, this data can be explained by hypothesizing that there is a mechanism that efficiently supplies galaxies with atomic hydrogen from outside. Using theoretical models, we aim to study which predominant hydrogen supply mechanism can explain the results obtained from these observations".

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Calendario orali e link zoom - Borse di dottorato DM 351/2022 e 352/2022

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ALLERGIE: COME CURARLE E COME FORMARE SPECIALISTI. Tre giorni in Fiera a Padova con il congresso sulle allergie e intolleranze alimentari coordinato dalla professoressa Antonella Muraro dell’Università di Padova

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