{"id":948,"date":"2024-04-22T11:08:18","date_gmt":"2024-04-22T11:08:18","guid":{"rendered":"http:\/\/147.96.46.35:10065\/?page_id=948"},"modified":"2025-11-03T13:11:54","modified_gmt":"2025-11-03T12:11:54","slug":"uv-catalogues","status":"publish","type":"page","link":"https:\/\/jcuva.ucm.es\/?page_id=948","title":{"rendered":"UV Catalogues"},"content":{"rendered":"\t\t
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\n\t\t\t\n\t\t\t\t \n\t\t\t\t\t\tUV CATALOGUES\t\t\t\t\t<\/span>\n\t\t\t\t\t\n\t\t\t\t\t\t\t<\/h2> <\/span>\n\n\t\t\t\n <\/div>\n\n\t\t\n\t\t<\/div>\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t
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The Joint Center for Ultraviolet Astronomy (JCUVA) shares the management of the Spektr-UF \/ WSO-UV Science Program. The WSO-UV SCC will also host the\u00a0Mission Data archive (MDA) .\u00a0<\/p>

As part of these activities, we will list below catalogues of UV sources, provided either by UV missions or by the community.<\/p>

Click on each catalogue for display<\/strong><\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t

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\n\t\t\t\n\t\t\t\t \n\t\t\t\t\t\tSTAR FORMATION CATALOGUES\t\t\t\t\t<\/span>\n\t\t\t\t\t\n\t\t\t\t\t\t\t<\/h2> <\/span>\n\n\t\t\t\n <\/div>\n\n\t\t\n\t\t<\/div>\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t
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\n \n \n <\/i> <\/a>\n <\/span>\n <\/div>\n STAR FORMATION CATALOGUE<\/span>\n
\n T Tauri Stars observed with I.U.E. Catalogue<\/span>\n <\/div>\n
T Tauri Stars (TTS) are low mass (M\u2264 1M\u2299) pre-main sequence (PMS) stars. They are often classified into two main sub-classes: classical TTS (cTTS) and weak line TTS (wTTS). This classification is based on the strength of the H\u03b1 line (W(H\u03b1 ) \u2265 10 \u00c5 for cTTS and W(H\u03b1 ) \u2264 10 \u00c5 for wTTS) that was taken primitively as a good tracer of their magnetic activity (and youth).<\/div> <\/div>\n <\/div>\n <\/div>\n
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\n \n \n <\/i> <\/a>\n <\/span>\n <\/div>\n STAR FORMATION CATALOGUE<\/span>\n
\n Herbig-Haro Objects Observed with I.U.E Catalogue<\/span>\n <\/div>\n
Herbig-Haro Objects (HHOs) are shock-excited nebulosities observed in star forming regions. They are powered by the energy released in the shocks between outflows from pre-main-sequence stars and interstellar gas (or previous ejecta)<\/div> <\/div>\n <\/div>\n <\/div>\n <\/div>\n <\/div>\n <\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t
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\n\t\t\t\n\t\t\t\t \n\t\t\t\t\t\tINTERSTELLAR MEDIUM IN THE UV\t\t\t\t\t<\/span>\n\t\t\t\t\t\n\t\t\t\t\t\t\t<\/h2> <\/span>\n\n\t\t\t\n <\/div>\n\n\t\t\n\t\t<\/div>\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t
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\n INTERSTELLAR MEDIUM IN THE UV<\/span>\n
\n UV Background Fluctuation Index from GalEX<\/span>\n <\/div>\n
Catalog containing the Ultraviolet Background Fluctuations Index from the all sky survey run by the Galaxy Evolution Explorer in the far ultraviolet (FUV) band (-intbgsub files).<\/div> <\/div>\n <\/div>\n <\/div>\n <\/div>\n <\/div>\n <\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t
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\n\t\t\t\n\t\t\t\t \n\t\t\t\t\t\tUV CATALOGUES\t\t\t\t\t<\/span>\n\t\t\t\t\t\n\t\t\t\t\t\t\t<\/h2> <\/span>\n\n\t\t\t\n <\/div>\n\n\t\t\n\t\t<\/div>\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t
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\n \n \n <\/i> <\/a>\n <\/span>\n <\/div>\n UV CATALOGUE<\/span>\n
\n GalEX Catalogues of UV sources produced by Luciana Bianchi<\/span>\n <\/div>\n
GALEX, the GALaxy Evolution eXplorer, performed the first extensive sky surveys at Ultraviolet wavelengths, filling the last gap so that our view of the sky is complete across the electromagnetic spectrum. The imaging surveys resulted in almost 600 million source measurements in two UV bands, far-UV and near-UV.<\/div> <\/div>\n <\/div>\n <\/div>\n
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\n \n \n <\/i> <\/a>\n <\/span>\n <\/div>\n UV CATALOGUE<\/span>\n
\n Synthetic photometry in the GalEX bands of stellar sources observed with I.U.E.<\/span>\n <\/div>\n
The Galaxy Evolution Explorer (GALEX) has produced the largest photometric catalogue of ultraviolet (UV) sources. As such, it has defined the new standard bands for UV photometry: the near UV band (NUV) and the far UV band (FUV). However, due to brightness limits, the GALEX mission has avoided the Galactic plane which is crucial for astrophysical research and future space missions.<\/div> <\/div>\n <\/div>\n <\/div>\n <\/div>\n <\/div>\n <\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t","protected":false},"excerpt":{"rendered":"

UV CATALOGUES The Joint Center for Ultraviolet Astronomy (JCUVA) shares the management of the Spektr-UF \/ WSO-UV Science Program. The WSO-UV SCC will also host the\u00a0Mission Data archive (MDA) .\u00a0 As part of these activities, we will list below catalogues of UV sources, provided either by UV missions or by the community. Click on each … <\/p>\n

Continue reading “UV Catalogues”<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":4,"comment_status":"closed","ping_status":"closed","template":"elementor_header_footer","meta":{"footnotes":""},"class_list":["post-948","page","type-page","status-publish","hentry"],"rttpg_featured_image_url":null,"rttpg_author":{"display_name":"Sonia P\u00e9rez","author_link":"https:\/\/jcuva.ucm.es\/?author=2"},"rttpg_comment":0,"rttpg_category":null,"rttpg_excerpt":"UV CATALOGUES The Joint Center for Ultraviolet Astronomy (JCUVA) shares the management of the Spektr-UF \/ WSO-UV Science Program. The WSO-UV SCC will also host the\u00a0Mission Data archive (MDA) .\u00a0 As part of these activities, we will list below catalogues of UV sources, provided either by UV missions or by the community. Click on each…","_links":{"self":[{"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=\/wp\/v2\/pages\/948","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=948"}],"version-history":[{"count":151,"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=\/wp\/v2\/pages\/948\/revisions"}],"predecessor-version":[{"id":4114,"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=\/wp\/v2\/pages\/948\/revisions\/4114"}],"wp:attachment":[{"href":"https:\/\/jcuva.ucm.es\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=948"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}