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Start Over Resource Type Archive Validation Level 2
1. ACS Galactic Globular Cluster Survey (ACSGGCT)
ID:
ivo://mast.stsci/acsggct
Title:
ACS Galactic Globular Cluster Survey (ACSGGCT)
Short Name:
HST.ACSGGCT
Date:
22 Jul 2020 22:26:50
Publisher:
Space Telescope Science Institute Archive
Description:
The ACSGGCT program used the HST ACS/WFC instrument to obtain uniform imaging of 65 of the nearest globular clusters to provide an extensive homogeneous dataset for a broad range of scientific investigations. An overview of the project was published by Sarajedini, A. et al. 2007, "The ACS Survey of Galactic Globular Clusters. I. Overview and Clusters Without Previous Hubble Space Telescope Photometry" AJ, 133, 1658.
2. Advanced Camera for Surveys
ID:
ivo://archive.stsci.edu/hst/acs
Title:
Advanced Camera for Surveys
Short Name:
HST.ACS
Date:
23 Jul 2020 19:47:47
Publisher:
Space Telescope Science Institute Archive
Description:
HST Advanced Camera for Surveys (ACS) - Images: CCD images between 3,700 - 11
3. AKARI Far-infrared All-Sky Survey Maps
ID:
ivo://jvo/isas/akari/fis_v1
Title:
AKARI Far-infrared All-Sky Survey Maps
Short Name:
AKARI_FIS_V1
Date:
18 Dec 2022 01:11:53
Publisher:
JVO
Description:
The AKARI Far-infrared All-Sky Survey Maps is produced with the participation of people from the following institutes: University of Tokyo, ISAS/JAXA, Tohoku University, and University of Tsukuba. The image data in this release are produced based on the AKARI All-Sky Survey with 4 far-infrared bands at N60 (65 um), WIDE-S (90 um), WIDE-L (140 um), and N160 (160 um).
4. AKARI N60
ID:
ivo://nasa.heasarc/skyview/akari
Title:
AKARI N60
Short Name:
AKARI
Date:
28 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
The AKARI (formerly Astro-F) mission is a Japanese second generation all-sky infrared survey mission. SkyView currently includes surveys from the four bands of the FIS instrument: N60, WIDE-S, WIDE-L and N160. <p> These surveys cover 99% of the sky in four photometric bands centred at 65μm, 90μm, 140μm, and 160μm, with spatial resolutions ranging from 1-1.5'. <p> These data provide crucial information on the investigation and characterisation of the proper- ties of dusty material in the interstellar medium (ISM), since a significant portion of its energy is emitted between ∼50 and 200 μm. The large-scale distribution of interstellar clouds, their thermal dust temperatures, and their column densities can be investigated with the improved spatial resolution compared to earlier all-sky survey observations. In addition to the point source distribution, the large-scale distribution of ISM cirrus emis- sion, and its filamentary structure, are well traced. <p> Data are obtained using using the <a href="https://jvo.nao.ac.jp/index-e.html">JVO</a> AKARI Simple Image Access Service. Provenance: AKARI FIS map making team [Univ of Tokyo, ISAS/JAXA, Tohoku Univ, Tsukuba Univ, The Rutherford Appleton Laboratory, The Open Univ]. This is a service of NASA HEASARC.
5. ALHAMBRA Final Archive: F814W images
ID:
ivo://svo.cab/alhambra_siap_f814w
Title:
ALHAMBRA Final Archive: F814W images
Short Name:
ALHAMBRA_F814W
Date:
14 Mar 2019 08:14:29
Publisher:
Spanish Virtual Observatory
Description:
This data server provides access to the F814W images of the ALHAMBRA Final Archive. The ALHAMBRA (Advance Large Homogeneous Area Medium Band Redshift Astronomical) survey (Moles et al. 2008) has observed 8 different regions of the sky, including sections of the COSMOS, DEEP2, ELAIS, GOODS-N, SDSS and Groth fields using a new photometric system with 20 contiguous, non-overlapping, equal width (~ 300A) filters, covering the optical range (3500A-9700A), plus the standard broadband NIR J, H and Ks filters. The observations were carried out with the Calar Alto (CAHA) 3.5m telescope using the wide field, 0.25 deg2 FOV optical camera LAICA and the NIR instrument Omega-2000. The ALHAMBRA survey dataset represents a ~700hrs of total exposure time, gathered in between the 2005 and 2012.Further information on the project can be found at the ALHAMBRA web page.
6. Alma-Ata Geomagnetic Observatory Data Service
ID:
ivo://fai.kz/ssa/geomag/q
Title:
Alma-Ata Geomagnetic Observatory Data Service
Short Name:
Geomag. fields
Date:
12 Dec 2024 16:36:40
Publisher:
Fesenkov Astrophysical Institute
Description:
The Alma-Ata Geomagnetic Observatory provides continuous monitoring of Earth's geomagnetic field. Located at 1300 meters above sea level in the foothills of the Tien Shan Mountains, approximately 10 km from Almaty, Kazakhstan, the observatory operates state-of-the-art equipment certified by INTERMAGNET, including the fluxgate magnetometer LEMI-008 and the proton Overhauser magnetometer POS-1. The data service includes: * **Observables**: Three components of the geomagnetic field vector (X, Y, Z) and the total field amplitude (F), measured in nanoteslas (nT). * **Data Resolution**: - XYZ components measured at a 1-second frequency. - F component measured at a 5-second frequency. - Derived minute averages for XYZF components available in real time. - Absolute measurements performed two to three times per week. The service provides open access to minute and hourly data (XYZF components and K-index of geomagnetic activity) through the Institute of Ionosphere's website for data from 2003 onward. Additionally, INTERMAGNET hosts minute variations data since 2004. Data prior to 2003 are available upon request. The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
7. Alma-Ata Station Neutron Monitor Data Service
ID:
ivo://fai.kz/ssa/neutrons/q
Title:
Alma-Ata Station Neutron Monitor Data Service
Short Name:
neutrons data
Date:
12 Dec 2024 16:35:27
Publisher:
Fesenkov Astrophysical Institute
Description:
The Alma-Ata Cosmic Ray Station operates the 18NM-64 neutron supermonitor at an altitude of 3340 meters above sea level with a geomagnetic cutoff rigidity of 6.7 GeV. The station provides real-time minute-level measurements of cosmic ray intensity and atmospheric pressure, contributing data to the international NMDB network (http://www.nmdb.eu). This service publishes daily tables containing two columns: - **timestamp**: Actual measurement times, ensuring accurate tracking. - **counts/sec**: Cosmic ray intensity in counts per second. The timestamps reflect actual measurement times, ensuring accurate tracking even when delayed data from previous days is incorporated into current files due to communication delays with space stations. The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
8. APASS Data Archive
ID:
ivo://cadc.nrc.ca/APASS
Title:
APASS Data Archive
Short Name:
APASS Archive
Date:
15 Jun 2019 21:15:00
Publisher:
Canadian Astronomy Data Centre
Description:
9. Arches Cross-matched Catalogue
ID:
ivo://arches/xmatch/cs
Title:
Arches Cross-matched Catalogue
Short Name:
Arches-Xmatch
Date:
03 Feb 2025 08:32:20
Publisher:
ARCHES - Astronomical Resource Cross-matching for High Energy Studies
Description:
Each of the archival catalogues used for the crossmatch is referenced by single letter: 3XMM: x, Galex: g, UCAC:u CMC: c, SDSS: s, UKIDSS LAS: l, KIDS GPS: k ALLWISE; w AKARI: a and FIRST_NVSS_COMBO: r
10. Archive of AGN spectral observations
ID:
ivo://fai.kz/spectra_agn_archive/q/ssa
Title:
Archive of AGN spectral observations
Short Name:
AGN Arch. SSAP
Date:
09 Dec 2024 11:20:09
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.

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