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.
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.
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/).
