<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
<record>
  <controlfield tag="001">301594</controlfield>
  <controlfield tag="005">20240928181149.0</controlfield>
  <datafield tag="035" ind1=" " ind2=" ">
    <subfield code="a">G:(GEPRIS)399628650</subfield>
  </datafield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="a">G:(GEPRIS)399628650</subfield>
    <subfield code="d">399628650</subfield>
  </datafield>
  <datafield tag="040" ind1=" " ind2=" ">
    <subfield code="a">GEPRIS</subfield>
    <subfield code="c">http://gepris.its.kfa-juelich.de</subfield>
  </datafield>
  <datafield tag="150" ind1=" " ind2=" ">
    <subfield code="a">PAPAS: Bestimmung der tatsächlichen Sternentstehungsraten in roten, in Galaxienhaufen fallenden Spiralgalaxien</subfield>
    <subfield code="y">2017 - 2018</subfield>
  </datafield>
  <datafield tag="371" ind1=" " ind2=" ">
    <subfield code="a">Dr. Eduard Thommes</subfield>
  </datafield>
  <datafield tag="450" ind1=" " ind2=" ">
    <subfield code="a">DFG project G:(GEPRIS)399628650</subfield>
    <subfield code="w">d</subfield>
    <subfield code="y">2017 - 2018</subfield>
  </datafield>
  <datafield tag="510" ind1="1" ind2=" ">
    <subfield code="a">Deutsche Forschungsgemeinschaft</subfield>
    <subfield code="0">I:(DE-588b)2007744-0</subfield>
    <subfield code="b">DFG</subfield>
  </datafield>
  <datafield tag="680" ind1=" " ind2=" ">
    <subfield code="a">Not all red galaxies in clusters are red and dead. In unrelaxed clusters - like Virgo – also red spirals exist that show ongoing star formation, reddened by dust. We aim to find out whether the dusty red spirals are common field galaxies in the process of entering the cluster potential or whether their star formation is triggered by ram pressure from moving across the inter-cluster medium. In our best studied cluster, Abell 901/2 the determination of the SFR from H and the UV+FIR flux leads to conflicting results. The PAnic Paschen Alpha Survey (PAPAS) is proposed to check the H-based SFR in several intermediate redshift galaxy clusters by using the Paschen-line red-shifted into the K-band. The current proposal should complete the observations of A226/8 by repeating observations lost due to bad weather in H2016.</subfield>
  </datafield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="o">oai:juser.fz-juelich.de:968337</subfield>
    <subfield code="p">authority:GRANT</subfield>
    <subfield code="p">authority</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">G</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">AUTHORITY</subfield>
  </datafield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="o">oai:juser.fz-juelich.de:968337</subfield>
  </datafield>
</record>
</collection>