{"id":{"repo_id":"radboud","oai_identifier":"oai:repository.ubn.ru.nl:2066/115711"},"canonical_url":"https://search.dev.ndltd.org/etd/radboud/oai:repository.ubn.ru.nl:2066/115711","repository":{"repo_id":"radboud","name":"Radboud University Nijmegen","base_url":"https://repository.ubn.ru.nl/oai/request"},"display":{"title":"Evolved stars in galactic plane surveys","abstract":"Contains fulltext : 115711.pdf (Publisher’s version ) (Open Access)","abstract_html":"Contains fulltext : 115711.pdf (Publisher’s version ) (Open Access)","abstract_has_math":false,"creators":["Verbeek, K."],"institution":"[S.l.] : [S.n.]","degree_name":null,"degree_level":null,"degree_discipline":null,"degree_department":null,"school":null,"contributors":["Groot, P.J."],"advisors":[],"committee_chairs":[],"committee_members":[],"year":2013,"date_issued":"2013","date_published":"2013","updated_at":"2026-07-24T04:00:43Z","subjects":["Astronomy"],"languages":[],"rights":[],"rights_urls":[],"identifier_entries":[{"key":"dc:identifier","label":"Identifier","values":["9789461918000"],"render_values":[{"text":"9789461918000","href":null,"code":true}]}]},"links":{"outbound_url":"http://hdl.handle.net/2066/115711","outbound_label":"Handle","outbound_source":"dc:identifier"},"metadata_groups":[{"id":"people","label":"People","entries":[{"key":"dc:contributor","label":"Contributor","values":["Groot, P.J."]},{"key":"dc:creator","label":"Author","values":["Verbeek, K."]}]},{"id":"academic_context","label":"Academic Context","entries":[{"key":"dc:date","label":"Dc Date","values":["2013"]},{"key":"dc:publisher","label":"Institution","values":["[S.l.] : [S.n.]"]},{"key":"dc:type","label":"Dc Type","values":["Doctoral thesis"]}]},{"id":"subjects_keywords","label":"Subjects and Keywords","entries":[{"key":"dc:subject","label":"Dc Subject","values":["Astronomy"]}]},{"id":"identifiers","label":"Identifiers","entries":[{"key":"dc:identifier","label":"Identifier","values":["https://repository.ubn.ru.nl//bitstream/handle/2066/115711/115711.pdf","http://hdl.handle.net/2066/115711","9789461918000"]}]},{"id":"additional","label":"Additional Metadata","entries":[{"key":"dc:description","label":"Description","values":["Contains fulltext : 115711.pdf (Publisher’s version ) (Open Access)","For the first time in history the entire Galactic Plane is digitally mapped from La Palma and Chile by the European Galactic Plane surveys EGAPS (UVEX, IPHAS and VPHAS+, see http://www.uvexsurvey.org http://www.iphas.org and http://www.vphasplus.org). The complete Galactic plane (3600 square degrees) is imaged in optical colours (U,g,r,i,Halpha and HeI5875) down to 21st magnitude using the INT and VST telescopes. This will eventually result into a multi-colour mosaic and a catalogue with more than a billion of stars. In this thesis the populations of evolved stars (white dwarfs, compact binaries and other UV-excess sources) in the data of the \"UV-Excess Survey of the Northern Galactic Plane (UVEX)\" are studied. From the first 211 square degrees of UVEX data, the bluest stars are automatically selected as UV-excess sources, spectroscopic follow-up of UV-excess objects is obtained, a DA white dwarfs space number density and birth rate is derived, and UV-excess sources with an infrared-excess are investigated. (see also Verbeek et al., 2012; Verbeek et al., 2013; Groot et al., 2009)","Radboud Universiteit Nijmegen, 11 september 2013","Promotor : Groot, P.J.","254 p."]},{"key":"dc:title","label":"Title","values":["Evolved stars in galactic plane surveys"]}]}],"canonical_facts":{"dc:contributor":["Groot, P.J."],"dc:creator":["Verbeek, K."],"dc:date":["2013"],"dc:description":["Contains fulltext : 115711.pdf (Publisher’s version ) (Open Access)","For the first time in history the entire Galactic Plane is digitally mapped from La Palma and Chile by the European Galactic Plane surveys EGAPS (UVEX, IPHAS and VPHAS+, see http://www.uvexsurvey.org http://www.iphas.org and http://www.vphasplus.org). The complete Galactic plane (3600 square degrees) is imaged in optical colours (U,g,r,i,Halpha and HeI5875) down to 21st magnitude using the INT and VST telescopes. This will eventually result into a multi-colour mosaic and a catalogue with more than a billion of stars. In this thesis the populations of evolved stars (white dwarfs, compact binaries and other UV-excess sources) in the data of the \"UV-Excess Survey of the Northern Galactic Plane (UVEX)\" are studied. From the first 211 square degrees of UVEX data, the bluest stars are automatically selected as UV-excess sources, spectroscopic follow-up of UV-excess objects is obtained, a DA white dwarfs space number density and birth rate is derived, and UV-excess sources with an infrared-excess are investigated. (see also Verbeek et al., 2012; Verbeek et al., 2013; Groot et al., 2009)","Radboud Universiteit Nijmegen, 11 september 2013","Promotor : Groot, P.J.","254 p."],"dc:identifier":["https://repository.ubn.ru.nl//bitstream/handle/2066/115711/115711.pdf","http://hdl.handle.net/2066/115711","9789461918000"],"dc:publisher":["[S.l.] : [S.n.]"],"dc:subject":["Astronomy"],"dc:title":["Evolved stars in galactic plane surveys"],"dc:type":["Doctoral thesis"]},"updated_at":"2026-07-24T04:00:43Z"}