{"id":498,"date":"2018-01-01T01:18:52","date_gmt":"2018-01-01T00:18:52","guid":{"rendered":"http:\/\/obas-matlas.u-strasbg.fr\/WP\/?p=498"},"modified":"2019-09-04T01:27:00","modified_gmt":"2019-09-03T23:27:00","slug":"image-release-stephans-quintet","status":"publish","type":"post","link":"https:\/\/matlas.astro.unistra.fr\/WP\/?p=498","title":{"rendered":"Image release: Stephan&#8217;s Quintet"},"content":{"rendered":"\n<figure class=\"wp-block-image\"><img loading=\"lazy\" width=\"1024\" height=\"880\" src=\"http:\/\/obas-matlas.u-strasbg.fr\/WP\/wp-content\/uploads\/2019\/09\/NGC7331_ugr-1024x880.jpg\" alt=\"\" class=\"wp-image-497\" srcset=\"https:\/\/matlas.astro.unistra.fr\/WP\/wp-content\/uploads\/2019\/09\/NGC7331_ugr-1024x880.jpg 1024w, https:\/\/matlas.astro.unistra.fr\/WP\/wp-content\/uploads\/2019\/09\/NGC7331_ugr-300x258.jpg 300w, https:\/\/matlas.astro.unistra.fr\/WP\/wp-content\/uploads\/2019\/09\/NGC7331_ugr-768x660.jpg 768w, https:\/\/matlas.astro.unistra.fr\/WP\/wp-content\/uploads\/2019\/09\/NGC7331_ugr.jpg 1460w\" sizes=\"(max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><figcaption>@ CFHT\/Duc\/Cuillandre<\/figcaption><\/figure>\n\n\n\n<p>The field around NGC 7331 and the Stephan&#8217;s Quintet, as seen by MegaCam. The true color composite image reveals multiple foreground and background structures, such as Milky-Way cirrus emission, extended stellar halos around the galaxies and tidal debris of past collisions.<br>The image was obtained with the same procedure as for the MATALS survey; it was originally aimed at being published in the CFHT yearly calendar.<br>Published in <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2018MNRAS.475L..40D\">Duc et al 2018<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The field around NGC 7331 and the Stephan&#8217;s Quintet, as seen by MegaCam. The true color composite image reveals multiple foreground and background structures, such as Milky-Way cirrus emission, extended stellar halos around the galaxies and tidal debris of past collisions.The image was obtained with the same procedure as for the MATALS survey; it was &hellip; <\/p>\n<p class=\"link-more\"><a href=\"https:\/\/matlas.astro.unistra.fr\/WP\/?p=498\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;Image release: Stephan&#8217;s Quintet&#8221;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":[],"categories":[6],"tags":[],"_links":{"self":[{"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=\/wp\/v2\/posts\/498"}],"collection":[{"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=498"}],"version-history":[{"count":1,"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=\/wp\/v2\/posts\/498\/revisions"}],"predecessor-version":[{"id":499,"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=\/wp\/v2\/posts\/498\/revisions\/499"}],"wp:attachment":[{"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=498"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=498"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/matlas.astro.unistra.fr\/WP\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=498"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}