{"id":54,"date":"2014-03-13T21:23:02","date_gmt":"2014-03-13T21:23:02","guid":{"rendered":"http:\/\/antonios-antoniou.gr\/en\/?page_id=54"},"modified":"2014-11-06T11:21:51","modified_gmt":"2014-11-06T11:21:51","slug":"citations","status":"publish","type":"page","link":"https:\/\/www.antonios-antoniou.gr\/en\/citations","title":{"rendered":"Citations"},"content":{"rendered":"<p align=\"center\"><b style=\"line-height: 1.5;\"><span style=\"text-decoration: underline;\">According to<\/span>:\u00a0 <\/b><a style=\"line-height: 1.5;\" href=\"http:\/\/adsabs.harvard.edu\/cgi-bin\/nph-abs_connect\" target=\"_blank\">Smithsonian\/NASA Astrophysics Data System (ADS)<\/a><\/p>\n<p align=\"center\"><b>Until December <\/b><b>2013<\/b><\/p>\n<p style=\"text-align: left;\" align=\"center\"><b><\/b>1. To the paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>Danezis, E. Lyratzi, E. Popovi<\/b><b>\u0107, L. \u010c., Dimitrijevi\u0107, M. S., <span style=\"text-decoration: underline;\">Antoniou, A.<\/span><span style=\"text-decoration: underline;\">,<\/span><\/b> <i>\u201c<\/i><i>Interpreting the complex line profiles in the stellar spectra\u201d,<\/i> 2009, <b><span style=\"text-decoration: underline;\">NewAR 53<\/span><\/b>, <b><span style=\"text-decoration: underline;\">21<\/span><\/b><b><span style=\"text-decoration: underline;\">4 <\/span><\/b><\/p>\n<p style=\"text-align: justify;\">referred:<b><\/b><\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>O. Chesneau, L. Dessart, D. \u00a0Mourard, Ph. B\u00e9rio, Ch. Buil, D. Bonneau, M. Borges Fernandes, J. M. Clausse, O. Delaa, A. Marcotto, A. Meilland, F. Millour, N. Nardetto, K. Perraut, A. Roussel, A. Spang, P. Stee,I. Tallon-Bosc, H. McAlister, T. ten Brummelaar, J. Sturmann, L. Sturmann, N. Turner,C. Farrington, and P. J. Gold\ufb01nger<\/b><\/p>\n<p style=\"text-align: justify;\">in their paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><i>\u201cTime, spatial, and spectral resolution of the H<\/i><i>\u03b1<\/i><i> line-formation region of Deneb and Rigel with the VEGA\/CHARA interferometer\u201d, <\/i><b><span style=\"text-decoration: underline;\">Astronomy &amp; Astrophysics , 521, A5, 2010.<\/span><\/b><\/p>\n<p style=\"text-align: justify;\">2.\u00a0To the paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>Danezis<\/b><b>, <\/b><b>E<\/b><b>., <\/b><b><span style=\"text-decoration: underline;\">Antoniou<\/span><\/b><b><span style=\"text-decoration: underline;\">, <\/span><\/b><b><span style=\"text-decoration: underline;\">A<\/span><\/b><b><span style=\"text-decoration: underline;\">.,<\/span><\/b><b><\/b><b>Lyratzi<\/b><b>, <\/b><b>E<\/b><b>., <\/b><b>Theodossiou<\/b><b>, <\/b><b>E<\/b><b>., <\/b><b>Stathopoulou<\/b><b>, <\/b><b>M<\/b><b>., <\/b><b>Nikolaidis<\/b><b>, D., <\/b><b>Drakopoulos<\/b><b>, <\/b><b>C<\/b><b>., <\/b><b>Soulikias<\/b><b>, <\/b><b>A<\/b><b>. &amp; <\/b><b>Koutroumanou<\/b><b>, <\/b><b>M<\/b><b>.: \u201c<\/b><i>The complex <\/i><i>coronal<\/i><i> structure of the Oe star HD 175754\u201d<\/i>, IV Serbian Conference on Spectral Lines Shapes (IV SCSLS), 2003, \u039f\u03ba\u03c4\u03ce\u03b2\u03c1\u03b9\u03bf\u03c2 10-15, Arandjelovac, \u03a3\u03b5\u03c1\u03b2\u03af\u03b1, <a href=\"http:\/\/adsabs.harvard.edu\/cgi-bin\/nph-data_query?bibcode=2003POBeo..76..175D&amp;db_key=AST&amp;link_type=ABSTRACT&amp;high=4999bacd2e19293\"><b>2003,<\/b><b>\u00a0POBeo<\/b><b>,<\/b><b>\u00a0<\/b><b>76,<\/b><b>\u00a0<\/b><b>175<\/b><\/a><\/p>\n<p style=\"text-align: justify;\">Referred:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>M<\/b><b>. <\/b><b>Avlonitis<\/b><b> <\/b><b>and<\/b><b> <\/b><b>A<\/b><b>. <\/b><b>Pappa<\/b><b> <\/b><b><\/b><\/p>\n<p style=\"text-align: justify;\">in their paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><i>\u201cTowards a probabilistic approach for DAC and SAC exact reconstruction in hot emission stars<\/i>,\u201d <b><span style=\"text-decoration: underline;\">Mem. S.A.It. Suppl. Vol. 15, 64<\/span><\/b><\/p>\n<p style=\"text-align: justify;\">3.\u00a0To the paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>Lyratzi, E., Danezis, E., Nikolaidis, D., Popovi\u0107, L. \u010c, Dimitrijevi\u0107, M. S. &amp; <span style=\"text-decoration: underline;\">Antoniou, A.<\/span><\/b> <i>\u201c<\/i><i>The complex structure of the MgII <\/i><i>\u03bb\u03bb<\/i><i> 2795.523, 2802.698 <\/i><i>\u0391<\/i><i> <\/i><i>regions of 64 Be stars\u201d<\/i> <b>2007, <\/b><b><span style=\"text-decoration: underline;\">PASJ, <\/span><\/b><b><span style=\"text-decoration: underline;\">59, 357.<\/span><\/b><\/p>\n<p style=\"text-align: justify;\">referred:<\/p>\n<p style=\"text-align: justify;\"><b>M<\/b><b>. <\/b><b>Avlonitis<\/b><b> <\/b><b>and<\/b><b> <\/b><b>A<\/b><b>. <\/b><b>Pappa<\/b><b> <\/b><b><\/b><\/p>\n<p style=\"text-align: justify;\">in their paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><i>\u201cTowards a probabilistic approach for DAC and SAC exact reconstruction in hot emission stars<\/i>,\u201d <b><span style=\"text-decoration: underline;\">Mem. S.A.It. Suppl. Vol. 15, 64<\/span><\/b><\/p>\n<p style=\"text-align: justify;\"><b><\/b>4. To the paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>Danezis, E. Lyratzi, E. Popovi<\/b><b>\u0107, L. \u010c., Dimitrijevi\u0107, M. S., <span style=\"text-decoration: underline;\">Antoniou, A.<\/span><span style=\"text-decoration: underline;\">,<\/span><\/b> <i>\u201c<\/i><i>Interpreting the complex line profiles in the stellar spectra\u201d,<\/i> 2009, <b><span style=\"text-decoration: underline;\">NewAR 53<\/span><\/b>, <b><span style=\"text-decoration: underline;\">21<\/span><\/b><b><span style=\"text-decoration: underline;\">4 <\/span><\/b><\/p>\n<p style=\"text-align: justify;\">referred:<b><\/b><\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>L. C. Popocic and P. Jovanovic <\/b><\/p>\n<p style=\"text-align: justify;\">in their paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><i>\u201cSpectral line shapes as a tool for investigation of kinematics and physics of plasma in quasars\u201d <\/i>\u00a0<b><span style=\"text-decoration: underline;\">Mem. S.A.It. Suppl. Vol. 15, 44<\/span><\/b><\/p>\n<p style=\"text-align: justify;\">5.\u00a0To the paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>Lyratzi, E.<\/b><b>, <\/b><b>Popovi<\/b><b>\u0107, L. \u010c.,Danezis,\u00a0\u00a0 E., Dimitrijevi\u0107, M. S., <span style=\"text-decoration: underline;\">Antoniou, A.,<\/span> <i>\u201c<\/i><\/b><i>Kinematics of the broad absorption line region in QSOs: Rotation and random motion\u201d<\/i>, 2009<b>, <span style=\"text-decoration: underline;\">NewAR, 53, 179<\/span><\/b><\/p>\n<p style=\"text-align: justify;\">referred:<b><\/b><\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><b>L<\/b><b>. <\/b><b>C<\/b><b>. <\/b><b>Popocic<\/b><b> <\/b><b>and<\/b><b> <\/b><b>P<\/b><b>. <\/b><b>Jovanovic<\/b><b> <\/b><b><\/b><\/p>\n<p style=\"text-align: justify;\">in their paper:<\/p>\n<p style=\"text-align: justify; padding-left: 30px;\"><i>\u201cSpectral line shapes as a tool for investigation of kinematics and physics of plasma in quasars\u201d <\/i>\u00a0<b><span style=\"text-decoration: underline;\">Mem. S.A.It. Suppl. Vol. 15, 44<\/span><\/b><\/p>\n","protected":false},"excerpt":{"rendered":"<p>According to:\u00a0 Smithsonian\/NASA Astrophysics Data System (ADS) Until December 2013 1. To the paper: Danezis, E. Lyratzi, E. Popovi\u0107, L. \u010c., Dimitrijevi\u0107, M. S., Antoniou, A., \u201cInterpreting the complex line profiles in the stellar spectra\u201d, 2009, NewAR 53, 214 referred: O. Chesneau, L. Dessart, D. \u00a0Mourard, Ph. B\u00e9rio, Ch. Buil, D. Bonneau, M. Borges Fernandes, &hellip; <a href=\"https:\/\/www.antonios-antoniou.gr\/en\/citations\" class=\"more-link\">Continue reading <span class=\"screen-reader-text\">Citations<\/span> <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"open","template":"","meta":{"footnotes":""},"class_list":["post-54","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/pages\/54","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/comments?post=54"}],"version-history":[{"count":7,"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/pages\/54\/revisions"}],"predecessor-version":[{"id":61,"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/pages\/54\/revisions\/61"}],"wp:attachment":[{"href":"https:\/\/www.antonios-antoniou.gr\/en\/wp-json\/wp\/v2\/media?parent=54"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}