The European Hubble Space Telescope Legacy Archive Wolfram Freudling.
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Transcript of The European Hubble Space Telescope Legacy Archive Wolfram Freudling.
![Page 1: The European Hubble Space Telescope Legacy Archive Wolfram Freudling.](https://reader036.fdocuments.net/reader036/viewer/2022062410/5697bffb1a28abf838cc12b6/html5/thumbnails/1.jpg)
The European Hubble Space Telescope
Legacy Archive
Wolfram Freudling
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The Hubble Space Telescope
1 telescope - currently, 3instruments in operation
- repair and service mission SM4 in 2008
- expected lifetime > 201312 instrumentsFOC, FOS, GHRS, HSP, WF/PC1, ACS, FGS, NICMOS, STIS, WFPC2, COS, WFC3
3 archives
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• HST archives contain pipeline-reduced science-ready data
• often requires significant processing before use• “difficult” data require significant expertise to
process• new paradigm: Archive produces high-level
Data Products: Hubble Legacy Archive (HLA)• also include community contributions• collaboration STScI, ST-ECF, CADC
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HST DATAimaging (e.g. ACS, WFPC2)
single object spectroscopy (STIS)
slitless spectroscopy (e.g. ACS, NICMOS)
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Slitless Spectroscopy in Space
• slitless spectroscopy inefficient from ground
• but in space:– low background– surveys in regions of spectrum which are
not accessible from ground (UV, IR)– high angular resolution of HST
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Data Examples
ACS
NICMOS
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HST Slitless DataHST focal plane sky distribution of
HST slitless spectroscopic data
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HST Slitless Data
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4 May 2006 Hubble Legacy Archive 10
Mission Statement
“Extract science grade 1d spectra of all isolated objects visible in undispersed images of HST slitless spectrographs using the best possible
calibration.”
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4 May 2006 Hubble Legacy Archive 11
GoalsWe will try:
• extract 1d spectra (vs. F) of all easy (high s/n) spectra• produce 2d (x vs y ) cutouts of all spectra• produce 2d cutouts of corresponding objects on undispersed images• extract spectra which are barely visible or noise only as long as there is
an object visible on the undispersed image• extract spectra for both point sources and extended sources• extract spectra at the edge of detector• extract spectra affected by bad pixels• characterize extracted spectra (noise, continuum level, lines?, …)
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4 May 2006 Hubble Legacy Archive 12
Goals IIWe will not try:• extract spectra of objects without undispersed image• deblend overlapping spectra • produce validated 2d spectra ( vs y)• classify spectra (stellar, extragalactic, QSO, BD, …)
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Pipeline for HLA Grism Data: PHLAG
poster by Martin Kümmel et al.
pipeline extracts spectra from slitless HST spectra
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ST-ECF HLA User Interface
spectra displayed in VOspec
undispersed image displayed in Aladin
spectrum selector
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ConclusionsThe ST-ECF Hubble Legacy Archive will contain:• ~ 104near IR spectra 1.1 to 1.9 µm (NICMOS G141)
o unique wavelength coverageo deep unbiased survey
• ~ 105 optical spectra 6000 to 10000 Å (ACS WF)
o deep, wide-angle spectroscopic survey• quasi-randomly distributed over the sky• best quality at high galactic latitude