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- ID:
- ivo://aip.gavo.org/tap
- Title:
- AIP DaCHS TAP service
- Short Name:
- AIP GAVO TAP
- Date:
- 17 Jul 2024 11:34:42
- Publisher:
- GAVO at Leibniz-Institute for Astrophysics Potsdam
- Description:
- The AIP DaCHS's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: dens256, fof, redshifts from the bolshoi schema, columns, services, tables from the glots schema, fof, fofmtree, fofparticles, particles85, redshifts, treesnapnums from the mdr1 schema, rave_dr4 from the ravedr4 schema, alt_identifier, authorities, capability, g_num_stat, interface, intf_param, registries, relationship, res_date, res_detail, res_role, res_schema, res_subject, res_table, resource, stc_spatial, stc_spectral, stc_temporal, subject_uat, table_column, tap_table, validation from the rr schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
- 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/).
- 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/).
- ID:
- ivo://org.gavo.dc/amanda/q/cone
- Title:
- AMANDA-II neutrino candidates
- Short Name:
- amanda cone
- Date:
- 27 Dec 2024 08:31:02
- Publisher:
- The GAVO DC team
- Description:
- A list of neutrino candidate events recorded by the AMANDA-II neutrino telescope during the period 2000-2006.
- ID:
- ivo://km3net.org/ant20_01/nu/cone
- Title:
- 2007-2017 ANTARES search for cosmic neutrino point sources
- Short Name:
- ANTARES2017
- Date:
- 09 Feb 2023 20:42:02
- Publisher:
- KM3NeT
- Description:
- The ANTARES neutrino telescope aims for the identification of neutrinos from cosmic accelerators. The good visibility towards the Southern sky for neutrino energies below 100 TeV and the good angular resolution for reconstructed events make the telescope excellent to test for the presence of point-like sources, especially of Galactic origin. The data set corresponds to the track sample (muon neutrino candidates) of a study meant to search for a point sources with data collected from January 2007 to December 2017 by the ANTARES neutrino telescope.
- ID:
- ivo://org.gavo.dc/antares/q/cone
- Title:
- 2007-2012 ANTARES search for cosmic neutrino point sources
- Short Name:
- antares cone
- Date:
- 27 Dec 2024 08:31:12
- Publisher:
- The GAVO DC team
- Description:
- A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2012 by the ANTARES neutrino telescope. This dataset includes a total of 5921 events obtained during the effective livetime of 1338 days.
- ID:
- ivo://org.gavo.dc/antares10/q/cone
- Title:
- 2007-2010 ANTARES search for cosmic neutrino point sources
- Short Name:
- antares10 cone
- Date:
- 27 Dec 2024 08:31:04
- Publisher:
- The GAVO DC team
- Description:
- A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2010 by the ANTARES neutrino telescope. This dataset includes a total of 3058 events obtained during the effective livetime of 813 days. This is legacy data. The most recently released data can be found at ivo://org.gavo.dc/antares/q/cone.
- ID:
- ivo://astron.nl/apertif_dr_bootes/q/cone
- Title:
- Apertif DR Bootes - Catalogue
- Short Name:
- DR Bootes
- Date:
- 01 Aug 2024 09:31:58
- Publisher:
- ASTRON
- Description:
- Apertif is a phased-array feed system for the Westerbork Synthesis Radio Telescope (WSRT), providing forty instantaneous beams over 300 MHz of bandwidth. This data release includes the catalogue and image observed by Apertif covering 26.5 square degree region in the Boötes constellation at 1.4 GHz. The image is a mosaic of 187 Apertif images from 8 different survey observations performed between April 2019 and November 2021. It has an angular resolution of 27×11.5 arcseconds and a median background noise of 40 μJy/beam. From this mosaic, 8994 sources were extracted and the catalogue is complete down to the 0.3 mJy level. This service queries the source catalogue of the Boötes field.
- ID:
- ivo://astron.nl/apertif_dr_bootes/q/cutout
- Title:
- Apertif DR Bootes - Mosaic
- Short Name:
- DR Bootes
- Date:
- 01 Aug 2024 09:31:58
- Publisher:
- ASTRON
- Description:
- Apertif is a phased-array feed system for the Westerbork Synthesis Radio Telescope (WSRT), providing forty instantaneous beams over 300 MHz of bandwidth. This data release includes the catalogue and image observed by Apertif covering 26.5 square degree region in the Boötes constellation at 1.4 GHz. The image is a mosaic of 187 Apertif images from 8 different survey observations performed between April 2019 and November 2021. It has an angular resolution of 27×11.5 arcseconds and a median background noise of 40 μJy/beam. From this mosaic, 8994 sources were extracted and the catalogue is complete down to the 0.3 mJy level. This service queries the mosaic image of the Boötes field.
