www.stecf.org
Open in
urlscan Pro
134.171.42.94
Public Scan
Submitted URL: http://www.stecf.org/
Effective URL: https://www.stecf.org/
Submission: On October 15 via api from US — Scanned from CA
Effective URL: https://www.stecf.org/
Submission: On October 15 via api from US — Scanned from CA
Form analysis
1 forms found in the DOMName: gs — GET https://www.google.com/custom
<form name="gs" method="GET" action="https://www.google.com/custom"><input type="hidden" name="num" value="50"><input type="hidden" name="hl" value="en"><input type="hidden" name="client" value="google-coop-np"><input type="hidden" name="cof"
value="AH:left;CX:ST-ECF;L:http://www.stecf.org/img/topimage.jpg;LH:65;LP:1;GFNT:#666666;DIV:#cccccc;"><input type="hidden" name="adkw"
value="AELymgX8mc_CGGXbUefOofK9B7oR3eOEqrzFrJRqSJCNV_yjyK4uzOBIcPt3ZqHifctgkgKpNdgDB-h9DfzO2sCyvnKDzR166w8T25Dm662ZcHtL9irxkTAL5wka0rXJO0Jrqb5I26KkFpobqh5JhdPnFenxqG2gL1S30rmLlIkePcg85K52LmI"><input type="text" name="q" size="7" maxlength="2048"
value="" title="Search"> <input type="submit" name="btnG" value="Search"><input id="custom" type="hidden" name="cx" value="014384758416157151158:ot-tzeyu97y" checked=""></form>
Text Content
For press and public spacetelescope.org Observing with HST About HST HST Documentation Proposal Preparation Science Data Archive HST archive at ESO ESO archive Hubble Legacy Archive HLA slitless data portal Data retrieval form HLA ACS/WFC G800L data Data preparation Data Processing Quality control Data release content Calibration HLA NICMOS G141 data VO instructions HLA-FAQ WFC2/FOS/HUDF/GOODS Advanced data products GOODS/FORS2 survey UDF GOODS ACS images Instrument science WFC3 grism mode WFC3/UVIS G280 WFC3/IR G102 WFC3/IR G141 WFC3 grism data simulations WFC3 data reduction cookbook ACS grism mode WFC G800L HRC G800L HRC PR200L SBC PR130L SBC PR110L NICMOS grism mode Calibration Software STIS Calibration Enhancement Spectroscopy Charge Tranfer Efficiency Calibration lamps Documents FOS Final Calibration Upgrade Documents Slitless Spectr. Simulations Spectral Templates Tiny Tim Software tools IRAF tools Python tools Scisoft Selected astronomy software Slitless spectroscopy software Coordination Activities ESA-ESO working groups Opticon ST-ECF Documents Newsletters Instrument science reports Conferences List of conferences ESO conference page A tree for site navigation will open here if you enable JavaScript in your browser. HOME ABOUT ST-ECF CONTACT CLOSURE OF THE ST-ECF Following decisions made by both ESA and ESO during the last few years, the ST-ECF has closed and ceased operations on 31 December 2010. Established as a joint venture between these two organisations in 1984, the ST-ECF has worked in close collaboration with the STScI in Baltimore to support European users of Hubble and to provide significant contributions to the operation of the observatory and its instruments. The European HST Archive has been moved to ESA's European Space Astronomy Centre (ESAC), Spain, where most of ESA's Space Science Archives are located and operated from. The new URL to the European HST archive is: http://hst.esac.esa.int Information resulting from the group's instrument science activities has been transferred to STScI and is available from their website. Re-links from the previous locations on the ST-ECF web site to the corresponding location on the STScI site have been established and should work for the remainder of the lifetime of the ST-ECF web site. More... Hubble with ACS/G800L spectra released by the ST-ECF as part of the Hubble Legacy Archive project. OTHER NEWS HST III Conference in Venice The Hubble Space Telescope (HST) is a joint project between the US National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA). The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory (ESO) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope.