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  <controlfield tag="001">2494</controlfield>
  <controlfield tag="005">20160701171706.0</controlfield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-651</subfield>
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  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">de Cuyper, J.-P.</subfield>
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  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2002</subfield>
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  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Improving the Rectification of Echelle Spectra</subfield>
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  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">We discuss how to improve the rectification of echelle spectra, based on tests done with a stable, fiber-fed spectrograph. Minor differences in the light path induce changes of the blaze function. However, these changes are almost independent of the spectral order when expressed in the proper coordinate. Additionally, we show how to avoid signatures of bad columns, insofar they are due to changes in the light path. </subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Hensberge, H.</subfield>
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  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Astronomical Data Analysis Software and Systems XI</subfield>
    <subfield code="v">281</subfield>
    <subfield code="y">2002</subfield>
    <subfield code="c">324</subfield>
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  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">http://esoads.eso.org/abs/2002ASPC..281..324D</subfield>
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    <subfield code="a">published in</subfield>
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    <subfield code="a">NONREF</subfield>
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