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Invitation to Tender for Satellite Laser Ranging Telescope System

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high sensitivity digital camera(s) which is used as an aid <strong>for</strong> tracking<br />

and calibration purposes.<br />

The tenderer offering a bistatic system shall include as a minimum<br />

requirement in the receiving telescope design the possibility of a<br />

payload of 30 kg <strong>to</strong> be located in a place where the focus is located. At<br />

least a volume of 20cm(H)*35cm(W)*45cm(L) occupied by the box<br />

should be also accounted <strong>for</strong> in the design. If the detec<strong>to</strong>r box can't be<br />

fitted directly <strong>to</strong> the back of the telescope, the beam path shall be<br />

extended and the focus directed <strong>to</strong> the place where the detec<strong>to</strong>r box<br />

can be installed.<br />

While not a minimum requirement <strong>to</strong> participate in the tender, the<br />

tenderer may also provide the designing, manufacturing, and<br />

installation of a detec<strong>to</strong>r box in the tender (cf. Template D). In this<br />

case, the box shall include an optical bench where all the necessary<br />

elements <strong>for</strong> kHz SLR operation are installed, these include (e.g.): the<br />

C- SPAD detec<strong>to</strong>r (provided by FGI); a camera; an iris; a narrow<br />

bandwidth filter; an ND filter; all the optical elements needed <strong>for</strong><br />

relaying the beam <strong>to</strong> the detec<strong>to</strong>r; an digital camera; and the<br />

collimating optics needed <strong>for</strong> the detec<strong>to</strong>r. The detec<strong>to</strong>r box design<br />

should allow remote alignment of the elements without using any<br />

wireless transmitters (cf. Appendix 2), including all the necessary<br />

software.<br />

This Call <strong>for</strong> Offers is open <strong>to</strong> all optical solutions <strong>for</strong> kHz satellite<br />

laser ranging. It is strongly advised that the tenderers provide<br />

sufficient supplementary documentation <strong>to</strong> demonstrate the<br />

suitability of their solution <strong>for</strong> kHz SLR operations.<br />

References:<br />

The International <strong>Laser</strong> <strong>Ranging</strong> Service<br />

http://iIrs.gsfc.nasa gov/<br />

Bistatic kHz systems:<br />

Austrian Academy of Sciences Observa<strong>to</strong>ry of Lustbühel, Austria<br />

http://www.iwf.oeaw.ac.at/en/research/solid-earth/slrtechnology/slr-station-graz-lustbuehel/<br />

Natural Environment Research Council Space Geodesy Facility at<br />

Herstmonceaux, UK<br />

http://sgf.rgo.ac.uk/sysspec/slr.html<br />

A monostatic 100Hz system:<br />

University of Bern, Zimmerwald Observa<strong>to</strong>ry, Switzerland<br />

http://cmslive3.unibe.ch/unibe/philnat/aiub/content/e14/e358/index<br />

_eng.html<br />

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