Content Level: Research / Capability Type: Custom Service

ID:: ivo://org.gavo.dc/pcc/q/cone
Title:: A Catalog of Galaxies in the Direction of the Perseus Cluster
Short Name:: pcc cone
Date:: 27 Dec 2024 08:31:02
Publisher:: The GAVO DC team
Description:: This is a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope. Additionally, we used archival Subaru multiband imaging data in order to measure aperture colors and to perform a morphological classification. The catalog reaches its 50 per cent completeness limit at an absolute V-band luminosity of -12 mag and a V-band surface brightness of 26 mag arcsec^-2 . In addition to the published table, this service also contains cutout images of the objects investigated.

ID:: ivo://fai.kz/fai_agn/q/i
Title:: AGN observations obtained at FAI
Short Name:: fai_agn siap
Date:: 05 Dec 2024 14:51:56
Publisher:: Fesenkov Astrophysical Institute
Description:: The database of Active Galactic Nuclea (AGN) photometrical observations obtained on defferent telescopes at Fesenkov Astrophysical Institute, Almaty, Kazakhstan since 2016. Observations were carried out in the optical range.

ID:: ivo://fai.kz/spectra_agn_archive/q/ssa
Title:: Archive of AGN spectral observations
Short Name:: AGN Arch. SSAP
Date:: 06 Mar 2025 07:24:23
Publisher:: Fesenkov Astrophysical Institute
Description:: The archive of AGN spectral observations is obtained on AZT-8 telescope at the Fesenkov Astrophysical Institute (FAI), Almaty, Kazakhstan. It represents the result of observations for abot 25 years - from 1970 to 1995. All observations were carried out at AZT-8 (D = 700 mm, F[main] = 2800 mm, F[Cassegrain] = 11000 mm) with a high-power spectrograph. In 1967-68, on the basis of the image intensifier (https://doi.org/10.1080/1055679031000084795a) developed and assembled the spectrograph of the original design in the workshops of the FAI.

ID:: ivo://lam.cesam.aspic/aspic_muse_wide/q/cone
Title:: ASPIC MUSE-Wide DR1 - Simple Cone Search
Short Name:: MUSEWIDE1 SCS
Date:: 19 May 2021 13:21:10
Publisher:: The CeSAM VO team
Description:: Photometry, spectral features, and physical parameters of MUSE-Wide sources on GOODS-South field.

ID:: ivo://lam.cesam.aspic/aspic_vuds/q/cone_cosmos
Title:: ASPIC VUDS-DR1 COSMOS - Simple Cone Search
Short Name:: VUDS-COSMOS SCS
Date:: 19 May 2021 09:57:10
Publisher:: The CeSAM VO team
Description:: Photometry, spectral features, and physical parameters of VUDS (DR1) sources on COSMOS field.

ID:: ivo://lam.cesam.aspic/aspic_vuds/q/cone_ecdfs
Title:: ASPIC VUDS-DR1 ECDFS - Simple Cone Search
Short Name:: VUDS-ECDFS SCS
Date:: 19 May 2021 09:57:10
Publisher:: The CeSAM VO team
Description:: Photometry, spectral features, and physical parameters of VUDS (DR1) sources on ECDFS field.

ID:: ivo://wfau.roe.ac.uk/atlasDR1-dsa
Title:: ATLAS DR1 - VST ATLAS Survey
Date:: 23 Jan 2024 09:42:24
Publisher:: WFAU, Institute for Astronomy, University of Edinburgh
Description:: This DSA hosts data release 1 of the ATLAS Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands. The ATLAS will complement the proposed VISTA Hemisphere Survey in the South.

ID:: ivo://org.gavo.dc/bgds/q/sia
Title:: Bochum Galactic Disk Survey (BGDS) images
Short Name:: bgds sia
Date:: 27 Dec 2024 08:31:07
Publisher:: The GAVO DC team
Description:: The Bochum Galactic Disk Survey is a project to monitor the stellar content of the Galactic disk in a 6 degree wide stripe centered on the Galactic plane. The data has been recorded from September 2010 to September 2019 with the RoBoTT Telecsope at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It contains measurements of more than 2x10^7 stars. The second and final data release contains follow-up observations from January 2017 to September 2019 in Sloan r and i and intermittent measurements in Johnson UVB, Sloan z and the narrowbands OIII, NB, Halpha and SII.

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