Ionized Outflows of Hot Stars     

F. Najarro  R.-P. Kudritzki  D.J. Hillier  H.J.G.L.M. Lamers  R.H.M. Voors  P.W. Morris  L.B.F.M. Waters 《Astrophysics and Space Science》1997,255(1-2):137-144

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The High-Resolution Solar Reference Spectrum between 250 and 550 nm and its Application to Measurements with the Ozone Monitoring Instrument     

Marcel Dobber  Robert Voors  Ruud Dirksen  Quintus Kleipool  Pieternel Levelt 《Solar physics》2008,249(2):281-291

We have constructed a new high resolution solar reference spectrum in the spectral range between 250 and 550 nm. The primary use of this spectrum is for the calibration of the Dutch – Finnish Ozone Monitoring Instrument (OMI), but other applications are mentioned. The incentive for deriving a new high resolution solar reference spectrum is that available spectra do not meet our requirements on radiometric accuracy or spectral resolution. In this paper we explain the steps involved in constructing the new spectrum, based on available low and high resolution spectra and discuss the main sources of uncertainty. We compare the result with solar measurements obtained with the OMI as well as with other UV-VIS space-borne spectrometers with a similar spectral resolution. We obtain excellent agreement with the OMI measurements, which indicates that both the newly derived solar reference spectrum and our characterization of the OMI instrument are well understood. We also find good agreement with previously published low resolution spectra. The absolute intensity scale, wavelength calibration and representation of the strength of the Fraunhofer lines have been investigated and optimized to obtain the resulting high resolution solar reference spectrum.  相似文献   

Dust in LBV Nebulae     

L.B.F.M. Waters  P.W. Morris  R.H.M. Voors  H.J.G.L.M. Lamers  N.R. Trams 《Astrophysics and Space Science》1997,255(1-2):179-185

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ISOCAM Imaging of LBVS     

N.R. Trams  R.H.M. Voors  L.B.F.M. Waters 《Astrophysics and Space Science》1997,255(1-2):195-196

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