Subject: spectroscopy / Result Type: application/x-votable+xml

ID:: ivo://org.gavo.dc/califa/q3/s
Title:: CALIFA DR3
Short Name:: califa ssa
Date:: 20 Apr 2023 00:19:47
Publisher:: The GAVO DC team
Description:: Split spectra from the CALIFA DR3 cubes. This service serves one spectrum each per pixel in each cube where there is at least one valid spaxel. Where both V500 and COMB data is available, COMB spectra are served. WARNING: The individual spectra are not independent. Also, error estimates over wide spectral ranges based on the error estimates served here are unreliable.

ID:: ivo://purx/datacentral-ssa
Title:: Data Central SSA
Short Name:: DCSSA
Date:: 08 Jun 2021 09:24:53
Publisher:: Data Central
Description:: Spectra from surveys hosted by Data Central. Most spectra were taken with the multi-object spectroscopy facilities 2dF (Anglo-Australian Telescope) and 6dF (UK Schmidt Telescope).

ID:: ivo://org.gavo.dc/dfbsspec/q/getssa
Title:: Digitized First Byurakan Survey (DFBS) Spectra Query Service
Short Name:: DFBS SSAP
Date:: 06 Feb 2024 09:11:09
Publisher:: The GAVO DC team
Description:: The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.

ID:: ivo://byu.arvo/dfbsspec/q/getssa
Title:: Digitized First Byurakan Survey (DFBS) Spectra Query Service
Short Name:: DFBS SSAP
Date:: 24 Aug 2020 16:45:07
Publisher:: The staff at the ArVO Data Center
Description:: The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.

ID:: ivo://org.gavo.dc/feros/q/ssa
Title:: FEROS Public Spectra
Short Name:: FEROS SSAP
Date:: 20 Apr 2023 00:19:48
Publisher:: The GAVO DC team
Description:: Spectra from FEROS spectrograph at La Silla's 1.5m telescope as obtained during commissioning and guaranteed time.

ID:: ivo://org.gavo.dc/flashheros/q/echssa
Title:: Flash/Heros Split-Order SSAP Service
Short Name:: F/H Orders SSAP
Date:: 31 Mar 2023 10:58:42
Publisher:: The GAVO DC team
Description:: Spectra from the Flash and Heros Echelle spectrographs developed at Landessternwarte Heidelberg and mounted at La Silla and various other observatories. The data mostly contains spectra of OB stars. Heros was the name of the instrument after Flash got a second channel in 1995.

ID:: ivo://org.gavo.dc/flashheros/q/ssa
Title:: Flash/Heros SSAP
Short Name:: Flash/Heros SSAP
Date:: 31 Mar 2023 10:58:42
Publisher:: The GAVO DC team
Description:: Spectra from the Flash and Heros Echelle spectrographs developed at Landessternwarte Heidelberg and mounted at La Silla and various other observatories. The data mostly contains spectra of OB stars. Heros was the name of the instrument after Flash got a second channel in 1995.

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