% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@ARTICLE{Hlsenbusch:604886,
      author       = {Hülsenbusch, Thomas and Winkelmann, Lutz and Eichner, Timo
                      and Lang, Tino and Palmer, Guido and Maier, Andreas},
      title        = {{R}educing wavelength jitter in white-light seeded
                      femtosecond optical parametric chirped-pulse amplifiers},
      journal      = {Optics express},
      volume       = {32},
      number       = {13},
      issn         = {1094-4087},
      address      = {Washington, DC},
      publisher    = {Optica},
      reportid     = {PUBDB-2024-01251},
      pages        = {23416},
      year         = {2024},
      abstract     = {White light generation (WLG) in bulk material can be used
                      as a versatile broadband seed source for optical parametric
                      chirped pulse amplification (OPCPA) stages. In this case, it
                      is beneficial to optimize the performance of the WLG seeder
                      in combination with the subsequent OPCPA stage. Here, we
                      characterize how small variations in the drive pulse energy
                      affect the white light seeder performance, in particular the
                      wavelength stability of the amplified OPCPA spectrum. To
                      isolate the influence of drive pulse energy on the OPCPA
                      central wavelength, we introduce a phase-sensitive amplitude
                      measurement and carefully optimize the drive pulse focus
                      position (at the bulk) to minimize the sensitivity to the
                      jitter of the drive pulse energy. With additional active
                      stabilization of the delay between pump and seed pulses in
                      the OPCPA, we achieve a central wavelength jitter of
                      2 × 10$^{−4}$. With this performance, our source is
                      an ideal front-end for applications in laser-plasma
                      acceleration or free-electron laser seeding.},
      cin          = {MLS / FS-LA},
      ddc          = {530},
      cid          = {I:(DE-H253)MLS-20210107 / I:(DE-H253)FS-LA-20130416},
      pnm          = {621 - Accelerator Research and Development (POF4-621)},
      pid          = {G:(DE-HGF)POF4-621},
      experiment   = {EXP:(DE-H253)KALDERA-20221201},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {39538805},
      UT           = {WOS:001253384100004},
      doi          = {10.1364/OE.527895},
      url          = {https://bib-pubdb1.desy.de/record/604886},
}