In order to make the most of the interaction with the members of the S-PLUS collaboration, we encourage the presentation of posters by the participants showing their work topics.<\/p>\n
Title and Abstract of Posters should be sent via email to ixlapis2020@gmail.com<\/a> with subject “Poster Abstract”.<\/p>\n Abstract submission deadline is January <\/strong>31st<\/strong>.<\/span><\/p>\n Posters maximum size should be A0.<\/p>\n Aidelman, Yael<\/strong> Baume, Gustavo<\/strong> Canossa Gosteinski, Marco Antonio<\/strong> Caso, Juan Pablo<\/strong> De Rossi, Mar\u00eda Emilia<\/strong> Donoso, Emilio<\/strong> Ennis, Ana<\/strong> Escudero, Carlos<\/strong> Feinstein, Carlos<\/strong> L\u00f3pez, Claudio<\/strong> L\u00f3pez, Iv\u00e1n<\/strong> Moreno, Jonathan<\/strong> Moyano, Facundo<\/strong> Parisi, Celeste<\/strong> Pichel, Ana<\/strong> Ponce, David<\/strong> Rodr\u00edguez, Facundo<\/strong> Rodr\u00edguez, Jimena<\/strong> Scalia, Mar\u00eda Cecilia<\/strong> Torres, Andrea<\/strong> Zenocratti, Lucas<\/strong> Posters of Participants In order to make the most of the interaction with the members of the S-PLUS collaboration, we encourage the presentation of posters by the participants showing their work topics. Title and Abstract of Posters should be sent via email to ixlapis2020@gmail.com with subject “Poster Abstract”. Abstract submission deadline is January 31st. Posters […]<\/p>\n","protected":false},"author":15,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"advgb_blocks_editor_width":"","advgb_blocks_columns_visual_guide":"","footnotes":""},"class_list":["post-1007","page","type-page","status-publish","hentry","post"],"aioseo_notices":[],"aioseo_head":"\n\t\t\n\t\n\t\n\t\n\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\tList of Posters (Author Alphabetic Order)<\/h1>\n
\nUsing Machine-Learning to obtain Be star candidates<\/a><\/p>\n
\nMining Study of Ionospheric Data<\/a><\/p>\n
\nSearching for Ultra Diffuse Galaxies in the Low-Density Environment around NGC 3115<\/a><\/p>\n
\nSiblings, Friends and Acquaintances: Testing Galaxy Association from Photometric Redshifts<\/a><\/p>\n
\nObservability of First Galaxies with a Generic FIR\/sub-mm Telescope<\/a><\/p>\n
\nGUNDAM: Blazing Fast Spatial Correlation Functions in Galaxy Surveys<\/a><\/p>\n
\nGlobular Cluster Systems as Tracers of Galactic Evolution<\/a><\/p>\n
\nPixel Colour-Magnitude Diagram Analysis of the Fornax Cluster using S-PLUS images (Part I)<\/a>
\nPixel Colour-Magnitude Diagram Analysis of the Fornax Cluster using S-PLUS images (Part II)<\/a><\/p>\n
\nStellar Formation in NGC 2366: Searching for Clusters and Associations using Unsupervised Algorithms<\/a><\/p>\n
\nThe Population of Neighborhood Galaxies around Radio AGNs<\/a><\/p>\n
\nThe SExOSS Project with S-PLUS: Search of Extended Objects in the Southern Sky<\/a>
\nSpectral-Cube Fitting Software for Spitzer and JWST Studies of Active Galaxies<\/a><\/p>\n
\nNew Light Curve of Massive Star Binary System HD 152590<\/a><\/p>\n
\nStar Formation within Bars of Nearby Galaxies<\/a><\/p>\n
\nChemical Properties of Bulge Globular Clusters from CaT Spectroscopy<\/a>
\nCaT Metallicities of SMC Star Clusters: Tracers of the Chemical Evolution<\/a><\/p>\n
\nLooking for blazars in the Galactic plane<\/a><\/p>\n
\nDichotomy in the Radio Galaxies Habitats in the Local Universe<\/a><\/p>\n
\nImproving Galaxy Group Finders<\/a><\/p>\n
\nThe YSG still preserve the same structure of the molecular clouds from which they form<\/a><\/p>\n
\nThe Color-Magnitude Relation of Early-Type Galaxies through the Analysis of Lick Indices<\/a><\/p>\n
\nGemini Near-Infrared Spectra of B[e] Star Candidates<\/a><\/p>\n
\nStudying the Color-Magnitud Relation of Simulated Early-Type Galaxies<\/a>
\nMass-Metallicity Relation as a Function of Morpho-Kinematics in EAGLE Simulations<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"