{"id":2980,"global_id":"uwm.edu\/physics?id=2980","global_id_lineage":["uwm.edu\/physics?id=2980"],"author":"63","status":"publish","date":"2015-11-04 12:57:03","date_utc":"2015-11-04 18:57:03","modified":"2023-01-18 10:22:02","modified_utc":"2023-01-18 16:22:02","url":"https:\/\/uwm.edu\/physics\/event\/cgca-seminar-angela-van-sistine\/","rest_url":"https:\/\/uwm.edu\/physics\/wp-json\/tribe\/events\/v1\/events\/2980","title":"CGCA Seminar: Angela Van Sistine","description":"<p>The CGCA (The Leonard E. Parker Center for Gravitation, Cosmology and Astrophysics) seminars are scheduled for Fridays at 1:00 pm in in the Kenwood Interdisciplinary Research Complex (KIRC) Room KEN 2175. A &#8220;brown bag lunch&#8221; group will assemble in KEN 4118 (fourth floor kitchenette located next to the elevators) at 12:00 NOON.<\/p>\n<p><strong>The ALFALFA Halpha Survey: Measuring the Local Star-Formation Rate Density<\/strong><br \/>\n<strong>Angela Van Sistine<\/strong>, University of Wisconsin-Milwaukee<\/p>\n<p>The ALFALFA Halpha survey uses a volume-limited sample of HI-selected galaxies from the ALFALFA survey to study star formation in the local universe. We have obtained sensitive narrow-band Halpha images of 1555 galaxies between 20 and 100 Mpc. Our large, complete sample of galaxies gives us robust statistics and allows us to cover a wide range of galaxian environments. A primary goal of our survey is to produce a precise measurement of the local star-formation rate density (SFRD). 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