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Welcome to the HST Spectroscopic Legacy Archive (HSLA).

On this page: Introduction Data Release Notes Data Access
Acknowledgment Important Notes Documents Feedback
Co-add FUV spectrum of NGC 5548, composed of 764 co-added exposures.
Time-series spectra of NGC 5548 showing variability.
Co-add spectrum of HS 1700+6416.
Co-add FUV spectrum of SN 1987A.
Co-add spectrum of WD 2218+706.
Co-add FUV spectrum of FAIRALL 9.
Co-add spectrum of MRK-54.
Co-add FUV spectrum of TW Hya.
Co-add spectrum of V4046 SGR.
Time-series FUV spectra of WD 0308-565.

Introduction

With no space ultraviolet instruments currently planned for the near future, the data from the UV spectrographs aboard the Hubble Space Telescope (HST) possess a legacy value beyond their initial science goals. Since early 2016, the Hubble Spectroscopic Legacy Archive (HSLA) provides the community with all raw and associated combined spectra forĀ COS far-ultraviolet data publicly available in the Mikulski Archive for Space Telescopes ("MAST"). These data are packaged into "smart archives" according to target type and scientific themes to facilitate the construction of archival samples for common science uses.

With every release the HSLA contents are also augmented with all COS datasets entered in the public domain since the previous release. These releases also capture significant calibration enhancements of the spectroscopic data they hold. In particular, this release of the HSLA was timed to inform proposers in preparation for the HST Cycle 26 call for proposals.

STIS UV spectra will be made available in future releases.

Data Release: July 2018

What's new?

  • 1074 newly released COS FUV data and associated co-added products added since April 2017
  • FUV Blue Modes now included (G130M/1055/1096/1222)
  • FUV co-adds now include LP3 and LP4 in addition to LP1 and LP2, with updated dispersion solutions
  • 248 newly released COS NUV data products added since April 2017
  • NUV co-added products now available; updated dispersion solution zero points are used
  • Redesigned target product page with FUV and NUV co-add "Quick Looks"
  • FUV and NUV failed visits now excluded from co-adds for enhanced data product quality

Data Access

Access to the COS FUV and NUV exposures and associated co-adds, all the diagnostic plots, and cross-matched information from Simbad or NED can be found here:

Pre-Sorted Target Tables

The targets are sorted by type and broad science categories.

The entire database can be downloaded as a tar file here (~42 GB).

Acknowledgment

If the contents of the HSLA were helpful to your research work, the following acknowledgment would be appreciated: "This research has made use of the HSLA database, developed and maintained at STScI, Baltimore, USA." Please also cite this ISR.

Important Notes

  • The content and format of the data are designed to enable users to assess the quantity and quality of data that already exist in the archive to support their science goals.
  • The science-readiness of the HSLA products depends on the intrinsic nature of the targets considered (e.g., variable or non-variable) and their extent (point sources or extended sources). In all cases, the HSLA utilizes the individual *x1d* files produced by the standard COS pipeline to generate the co-adds included in the database.

Documents

For more information on the latest COS FUV calibration updates included in this release, see:
http://www.stsci.edu/hst/cos/documents/newsletters/cos_newsletters/full_stories/2018_04/lp3_deliveries
http://www.stsci.edu/hst/cos/documents/newsletters/cos_newsletters/full_stories/2018_04/lp4_deliveries

For more information on the latest COS NUV calibration updates included in this release, see:
http://www.stsci.edu/hst/cos/documents/newsletters/cos_newsletters/stan1702.html#article1
http://www.stsci.edu/hst/cos/documents/isrs/ISR2017_02.pdf
http://www.stsci.edu/hst/cos/documents/isrs/ISR2017_03.pdf

Descriptions of the original release (Feb. 2016) and of the overall structure of the database can be found here: Peeples et al. (2017).

Feedback

We invite questions and comments about the database to hst_spec_legacy@stsci.edu.