Subsections

• 1.3.1 References
• 1.3.2 Acknowledgements
• 1.3.3 Guidelines

1.3 How to Refer to the ISO Documentation

1.3.1 References

1. References for general ISO topics, including the mission, satellite, instrument payload, orbit and operations, project organisation, observations and ISO data products:
   • The ISO Handbook, Volumes I-V, T.G. Müller, J.A.D.L. Blommaert & P. García-Lario (Eds.), ESA SP-1262, 2003:
     • Volume I: ISO - Mission & Satellite Overview,
       Kessler M.F., Müller T.G., Leech K. et al., Version 2.0, July 2003
     • Volume II: CAM - The ISO Camera,
       Blommaert J., Siebenmorgen R., Coulais A. et al., Version 2.0, June 2003
     • Volume III: LWS - The Long Wavelength Spectrometer,
       Gry C., Swinyard B., Harwood A. et al., Version 2.1, June 2003
     • Volume IV: PHT - The Imaging Photo-Polarimeter,
       Laureijs R.J., Klaas U., Richards P.J. et al., Version 2.0.1, June 2003
     • Volume V: SWS - The Short Wavelength Spectrometer,
       Leech K., Kester D., Shipman R. et al., Version 2.0.1, June 2003
   • Kessler M.F., Steinz J.A., Anderegg M. et al. 1996, The Infrared Space Observatory (ISO) mission, A&A 315, L27
   • Kessler M.F. 1999, The ISO mission: past and future, in `The Universe as Seen by ISO'. Eds. P. Cox & M.F. Kessler, ESA SP-427, 23

2. References for the ISO instruments in A&A Special Issue, Volume 315, Number 2, pp. L27-L400, 1996:
   • Cesarsky C.J., Abergel A., Agnèse P. et al. 1996, ISOCAM in flight, A&A 315, L32
   • Clegg P.E., Ade P.A.R., Armand C. et al. 1996, The ISO Long-Wavelength spectrometer, A&A 315, L38
   • Lemke D., Klaas U., Abolins J. et al. 1996, ISOPHOT: Capabilities and performance, A&A 315, L64
   • De Graauw, Th., Haser, L.N., Beintema, D.A. et al. 1996, Observing with the ISO Short Wavelength Spectrometer, A&A 315, L49

   Further instrument specific publications in The Universe as Seen by ISO, 1999, ESA SP-427, P. Cox & M.F. Kessler (Eds.):

   • Cesarsky C.J. 1999, ISOCAM: first assessment after the end of the mission, in `The Universe as Seen by ISO'. Eds. P. Cox & M.F. Kessler, ESA SP-427, 45
   • Clegg P.E. 1999, The ISO Long-Wavelength Spectrometer: description, performance and highlights, in `The Universe as Seen by ISO'. Eds. P. Cox & M.F. Kessler, ESA SP-427, 39
   • Lemke D. & Klaas U. 1999, ISOPHOT - performance, results and outlook, in `The Universe as Seen by ISO'. Eds. P. Cox & M.F. Kessler, ESA SP-427, 51
   • De Graauw Th. 1999, Summary of ISO SWS performance and science highlights, in `The Universe as Seen by ISO'. Eds. P. Cox & M.F. Kessler, ESA SP-427, 31

3. References for technical notes in the ISO Explanatory Library:
   
   http://www.iso.vilspa.esa/ $\rightarrow$ ISO Explanatory Library

4. References for Interactive Analysis (IA) software and data reduction procedures:
   • CAM: ISOCAM Interactive Analysis User's Manual,
     Version 5.0, SAI/96-5226/Dc, M. Delaney & S. Ott (Eds.), 2002
     http://www.iso.vilspa.esa.es/ $\rightarrow$ ISO Data Analysis Software
     $\rightarrow$ ISOCAM Interactive Analysis (CIA)

   • LWS: http://www.iso.vilspa.esa.es/ $\rightarrow$ ISO Data Analysis Software
     $\rightarrow$ ISO Spectroscopic Analysis Package (ISAP)
     $\rightarrow$ LWS Interactive Analysis (LIA)

   • PHT: PHT Interactive Analysis User Manual,
     Version 9.0, C. Gabriel, 2000.
     http://www.iso.vilspa.esa.es/ $\rightarrow$ ISO Data Analysis Software
     $\rightarrow$ ISOPHOT Interactive Analysis (PIA)

   • SWS: http://www.iso.vilspa.esa.es/ $\rightarrow$ ISO Data Analysis Software
     $\rightarrow$ ISO Spectroscopic Analysis Package (ISAP)
     $\rightarrow$ Observers SWS Interactive Analysis Package (OSIA)

1.3.2 Acknowledgements

1. ISO
   
   Any article based on ISO data should contain the following text, as a footnote to the title:
   
   Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, the Netherlands and the United Kingdom) and with the participation of ISAS and NASA.
   
   Should the journal in question not permit footnotes to the title, the above text should appear as a footnote the first time ISO is mentioned.
   
   The preferred reference article for the ISO mission is:
   
   Kessler M.F., Steinz J.A., Anderegg M. et al. 1996, The Infrared Space Observatory (ISO) mission, A&A 315, L27.

2. Scientific Instruments
   
   You should acknowledge the instrument(s) you use with a reference to one (or more) of the following articles:
   • Cesarsky C.J., Abergel A., Agnèse P. et al. 1996, ISOCAM in flight, A&A 315, L32
   • Clegg P.E., Ade P.A.R., Armand C. et al. 1996, The ISO Long-Wavelength Spectrometer, A&A 315, L38
   • Lemke D., Klaas U., Abolins J. et al. 1996, ISOPHOT: Capabilities and performance, A&A 315, L64
   • De Graauw Th., Haser L.N., Beintema D.A. et al. 1996, Observing with the ISO Short Wavelength Spectrometer, A&A 315, L49

3. CIA (ISOCAM Interactive Analysis)
   
   If you use CIA to reduce your CAM data please write in the acknowledgments:
   
   The ISOCAM data presented in this paper were analysed using `CIA', a joint development by the ESA Astrophysics Division and the ISOCAM Consortium. The ISOCAM Consortium is led by the ISOCAM PI, C. Cesarsky.
   
   The preferred reference to CIA is:
   
   Ott S., Abergel A., Altieri B. et al. 1997, Design and Implementation of CIA, the ISOCAM Interactive Analysis System, in ASP Conf. Ser. Vol. 125, Astronomical Data Analysis Software and Systems (ADASS) VI, G. Hunt & H.E. Payne (Eds.), San Francisco: ASP, 34

4. ISAP (ISO Spectroscopic Analysis Package)
   
   If you use ISAP to reduce your SWS or LWS data please write in the acknowledgments:
   
   The ISO Spectral Analysis Package (ISAP) is a joint development by the LWS and SWS Instrument Teams and Data Centers. Contributing institutes are CESR, IAS, IPAC, MPE, RAL and SRON.

5. PIA (ISOPHOT Interactive Analysis)
   
   If you use PIA to reduce your ISOPHOT data please write in the acknowledgments:
   
   The ISOPHOT data presented in this paper were reduced using PIA, which is a joint development by the ESA Astrophysics Division and the ISOPHOT Consortium with the collaboration of the Infrared Processing and Analysis Center (IPAC). Contributing ISOPHOT Consortium institutes are DIAS, RAL, AIP, MPIK, and MPIA.
   
   The preferred reference to PIA is:
   
   Gabriel C., Acosta-Pulido J., Heinrichsen I. et al. 1997, The ISOPHOT Interactive Analysis PIA, a calibration and scientific analysis tool, in ASP Conf. Ser. Vol. 125, Astronomical Data Analysis Software and Systems (ADASS) VI, G. Hunt & H.E. Payne (Eds.), San Francisco: ASP, 108

6. OSIA (Observers SWS Interactive Analysis Package)
   
   If you use OSIA to reduce your SWS data please write in the acknowledgements:
   
   OSIA is a joint development of the SWS consortium. Contributing institutes are SRON, MPE, KUL and the ESA Astrophysics Division.
   
   If you use IA3 to reduce your SWS data please write in the acknowledgements:
   
   IA3 is a joint development of the SWS consortium. Contributing institutes are SRON, MPE, KUL and the ESA Astrophysics Division.

1.3.3 Guidelines

• Identifying ISO observations in a publication:
  
  The `Observations' section (or equivalent) of a paper using ISO data should clearly identify the observations on which the results presented in the publication are based. This is done uniquely by listing the TDT and AOT for each individual observation used. The TDT is an 8 digit number which you can see in the query results in the ISO Data Archive or in the filename of the retrieved observation. The AOT is a combination of a three letter code: CAM, LWS, PHT or SWS indicating the instrument (Camera, Long Wavelength Spectrometer, Imaging Photo-Polarimeter and Short Wavelength Spectrometer, respectively) and a two digit number indicating the instrument mode. The AOT can be found from query results in the archive or from the retrieved file headers of the data sets related to an observation. The authors should also include all additional information of the observations which has astronomical relevance in the studied case (e.g. the time the observations were made), but the TDT and AOT should never be omitted in order to give the possibility for future readers to find the original data in the ISO Data Archive.

• Inventory of ISO publications
  
  In order to offer a complete bibliographic information to the ISO Data Archive users, we try to keep track of all publications involving ISO data, and of all observations used for these publications. The ISO Data Archive provides the references of the publications involving any selected observation and a link to their Astrophysics Data System (ADS) entry^1.2. Your contribution in this matter can greatly help keeping an information as comprehensive as possible and we therefore ask you to kindly provide the following information for each of your publications:
  • complete reference of the article (or preprint)
  • list of TDT numbers and instrument modes of the observations that you have exploited for the publication

  You can send the information either by e-mail to:
  

  helpdesk@iso.vilspa.esa.es

  or by normal mail to:
  

  ISO Project Scientist
  (ISO Preprints)
  ESA Satellite Tracking Station
  Villafranca del Castillo
  P.O. Box 50727
  28080 Madrid, Spain