Capability Type: Simple Image Access Protocol and VOSI Tables

ID:: ivo://fai.kz/fai_agn/q/i
Title:: AGN observations obtained at FAI
Short Name:: fai_agn siap
Date:: 10 Oct 2023 11:48:20
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://astron.nl/apertif_dr_bootes/q/cutout
Title:: Apertif DR Bootes - Mosaic
Short Name:: DR Bootes
Date:: 23 Jun 2023 13:45:11
Publisher:: ASTRON
Description:: This service provides mosaic from the images of the Apertif DR Bootes.

ID:: ivo://org.gavo.dc/bgds/q/sia
Title:: Bochum Galactic Disk Survey (BGDS) images
Short Name:: bgds sia
Date:: 09 Feb 2023 14:31:11
Publisher:: The GAVO DC team
Description:: The Bochum Galactic Disk Survey is an ongoing 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 since mid-2010 in Sloan r and i simultaneously with the RoBoTT Telecsope at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It contains measurements of about 2x10^7 stars over more than seven years. Additionally, intermittent measurements in Johnson UVB and Sloan z have been recorded as well.

ID:: ivo://org.gavo.dc/cars/q/cutout
Title:: CARS image cutouts
Short Name:: CARS_cutout
Date:: 23 Mar 2022 13:13:18
Publisher:: The GAVO DC team
Description:: Images and data from from the CFHTLS archive research survey, a multi-band dataset spanning 37 square degrees of sky in high galactic latitudes.

ID:: ivo://org.gavo.dc/fornax/q/c
Title:: Deep Mosaic of the Fornax cluster core
Short Name:: fornax cutout
Date:: 27 Feb 2023 14:52:21
Publisher:: The GAVO DC team
Description:: This is a deep optical mosaic of the Fornax cluster’s core, covering 1.6 square degrees. The data were acquired with ESO/MPG 2.2m/WFI, using a transparent filter that nearly equals the no-filter throughput and thus provides a high signal-to-noise ratio. Based on an approximate conversion to V-band magnitudes, the unbinned and binned mosaics (0.24 and 0.71 arcsec/pixel) reach a median depth of 26.6 and 27.8 mag/sq.arcsec, respectively.

ID:: ivo://vopdc.obspm/gepi/vopsat/esor
Title:: ESO-R Survey
Short Name:: ESO-R
Date:: 10 Nov 2022
Publisher:: Paris Astronomical Data Centre - GEPI
Description:: VO-compliant publication of Schmidt survey ESO-R of the southern sky digitized with the MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI).

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