SDSS DR7 - Sloan Digital Sky Survey Data Release 7
Short Name:
SDSS DR7
Date:
04 Dec 2019 13:36:17
Publisher:
WFAU, Institute for Astronomy, University of Edinburgh
Description:
This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR7 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
SDSS DR5 - Sloan Digital Sky Survey Data Release 5
Short Name:
SDSS DR5
Date:
04 Dec 2019 13:36:06
Publisher:
WFAU, Institute for Astronomy, University of Edinburgh
Description:
This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR5 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
Catalogues of solar observations held at MSSL/UCL. Datasets available are SOHO CDS, SOHO EIT, Yohkoh SXT. URL links to data files are provided (EIT data files provided by SDAC, NASA). Reference: http://www.mssl.ucl.ac.uk/www_solar/surfindex.html
An archive of optical and near-infrared spectra of strongly lensed
quasars and the lensing galaxies. The spectra are resolved to about a
few Ångstroms and are flux-calibrated. The spectra resulted from
deblending the lensed images in bidimensional spectra available from
the SSAP service for `ivo://org.gavo.dc/mlqso/q/s
<http://dc.zah.uni-heidelberg.de/mlqso/q/s/info>`_.
WFAU, Institute for Astronomy, University of Edinburgh
Description:
The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
TheoSSA provides spectral energy distributions based on model
atmosphere calculations. Currently, we serve results obtained using
the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact
stars.
TheoSSA provides spectral energy distributions based on model
atmosphere calculations. Currently, we serve results obtained using
the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact
stars.
The Panchromatic High-Resolution Spectroscopic Survey of Local Group
Star Clusters PCSLG
Short Name:
PCSLG SSAP
Date:
23 Mar 2022 13:13:17
Publisher:
The GAVO DC team
Description:
This dataset contains spectroscopic observations of 29 globular
clusters in the Magellanic Clouds and the Milky Way performed with
VLT/X-shooter over eight full nights.