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@ARTICLE{Westphal:207270,
      author       = {Westphal, Andrew J. and Bechtel, Hans A. and Brenker, Frank
                      E. and Butterworth, Anna L. and Flynn, George and Frank,
                      David R. and Gainsforth, Zack and Hillier, Jon K. and
                      Postberg, Frank and Simionovici, Alexandre S. and Sterken,
                      Veerle J. and Stroud, Rhonda M. and Allen, Carlton and
                      Anderson, David and Ansari, Asna and Bajt, Saša and
                      Bastien, Ron K. and Bassim, Nabil and Borg, Janet and
                      Bridges, John and Brownlee, Donald E. and Burchell, Mark and
                      Burghammer, Manfred and Changela, Hitesh and Cloetens, Peter
                      and Davis, Andrew M. and Doll, Ryan and Floss, Christine and
                      Grün, Eberhard and Heck, Philipp R. and Hoppe, Peter and
                      Hudson, Bruce and Huth, Joachim and Hvide, Brit and
                      Kearsley, Anton and King, Ashley J. and Lai, Barry and
                      Leitner, Jan and Lemelle, Laurence and Leroux, Hugues and
                      Leonard, Ariel and Lettieri, Robert and Marchant, William
                      and Nittler, Larry R. and Ogliore, Ryan and Ong, Wei Ja and
                      Price, Mark C. and Sandford, Scott A. and Tresseras,
                      Juan-Angel Sans and Schmitz, Sylvia and Schoonjans, Tom and
                      Silversmit, Geert and Solé, Vicente A. and Srama, Ralf and
                      Stadermann, Frank and Stephan, Thomas and Stodolna, Julien
                      and Sutton, Steven and Trieloff, Mario and Tsou, Peter and
                      Tsuchiyama, Akira and Tyliszczak, Tolek and Vekemans, Bart
                      and Vincze, Laszlo and Von Korff, Joshua and Wordsworth,
                      Naomi and Zevin, Daniel and Zolensky, Michael E.},
      title        = {{F}inal {R}eports of the {S}tardust {I}nterstellar
                      {P}reliminary {E}xamination},
      journal      = {Meteoritics $\&$ planetary science},
      volume       = {49},
      number       = {9},
      issn         = {1086-9379},
      address      = {Hoboken, NJ},
      publisher    = {Wiley-Blackwell},
      reportid     = {PUBDB-2015-01253},
      pages        = {1720 - 1733},
      year         = {2014},
      note         = {(c) The Meteoritical Society. Post referee full text in
                      progress. Embargo for full text 1 year from 22 AUG 2014},
      abstract     = {With the discovery of bona fide extraterrestrial materials
                      in the Stardust Interstellar Dust Collector, NASA now has a
                      fundamentally new returned sample collection, after the
                      Apollo, Antarctic meteorite, Cosmic Dust, Genesis, Stardust
                      Cometary, Hayabusa, and Exposed Space Hardware samples.
                      Here, and in companion papers in this volume, we present the
                      results from the Preliminary Examination of this collection,
                      the Stardust Interstellar Preliminary Examination (ISPE). We
                      found extraterrestrial materials in two tracks in aerogel
                      whose trajectories and morphology are consistent with an
                      origin in the interstellar dust stream, and in residues in
                      four impacts in the aluminum foil collectors. While the
                      preponderance of evidence, described in detail in companion
                      papers in this volume, points toward an interstellar origin
                      for some of these particles, alternative origins have not
                      yet been eliminated, and definitive tests through isotopic
                      analyses were not allowed under the terms of the ISPE. In
                      this summary, we answer the central questions of the ISPE:
                      How many tracks in the collector are consistent in their
                      morphology and trajectory with interstellar particles? How
                      many of these potential tracks are consistent with real
                      interstellar particles, based on chemical analysis?
                      Conversely, what fraction of candidates are consistent with
                      either a secondary or interplanetary origin? What is the
                      mass distribution of these particles, and what is their
                      state? Are they particulate or diffuse? Is there any
                      crystalline material? How many detectable impact craters
                      (>100 nm) are there in the foils, and what is their size
                      distribution? How many of these craters have analyzable
                      residue that is consistent with extraterrestrial material?
                      And finally, can craters from secondaries be recognized
                      through crater morphology (e.g., ellipticity)?},
      cin          = {FS-ML / DOOR},
      ddc          = {520},
      cid          = {I:(DE-H253)FS-ML-20120731 / I:(DE-H253)HAS-User-20120731},
      pnm          = {FS In-house research / external facilities (POF2-544)},
      pid          = {G:(DE-H253)POF2-Other-Beam-20130405},
      experiment   = {EXP:(DE-MLZ)External-20140101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000342912100012},
      doi          = {10.1111/maps.12221},
      url          = {https://bib-pubdb1.desy.de/record/207270},
}