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The Karl G. Jansky Very Large Array (VLA) is a centimeter-wavelength radio astronomy observatory in the southwestern United States built in the 1970s. It lies in central New Mexico on the Plains of San Agustin, between the towns of Magdalena and Datil, approximately 50 miles (80 km) west of Socorro. The VLA comprises 28 25-meter (82 ft) radio telescopes…
The analysis highlights Characters, History, Measurement and Science as prominent areas in the source structure around Very Large Array.
Source areas are shown by the number of related topics found in each part of the analysis. Use smaller areas too: they can reveal specialized angles and content gaps.
Smaller areas are not necessarily less important. They contain fewer connections in this analysis and can be useful for finding specialized angles or coverage gaps.
High-confidence facts extracted from structured source data. Use them as anchors for further research.
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The extracted context around Very Large Array shows recurring relationship patterns in the source. For example, Very Large Array → Array, GHz, In June, National Radio Astronomy Observatory, Next Generation Very Large, North America, Upgrading Another extracted example is Very Large Array → VLA. Use these groups to spot repeated connection types before inspecting the individual relationships.
Use these terms to understand the vocabulary surrounding the topic, not as a checklist for keyword stuffing.
vla radio new array mexico large ft nrao center antennae west observatory located science astronomy telescopes ngvla 50 project site
TTTA extracted 13 structured relationships around Very Large Array. Examples in this analysis include Very Large Array → Alternative names → VLA and Very Large Array → Altitude → 2,124 m (6,969 ft). The table shows each extracted connection, where it came from and its confidence.
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Very Large Array | Alternative names | VLA | 1.00 | infobox |
| Very Large Array | Altitude | 2,124 m (6,969 ft) | 1.00 | infobox |
| Very Large Array | Built | 1973–1981 | 1.00 | infobox |
| Very Large Array | Location | Socorro County, New Mexico | 1.00 | infobox |
| Very Large Array | Wavelength | 0.6 cm (50 GHz)–410 cm (73 MHz) | 1.00 | infobox |
| Very Large Array | Website | science.nrao.edu/facilities/vla/ | 1.00 | infobox |
| Very Large Array | related to ngVLA upgrade | In June | 0.60 | section |
| Very Large Array | related to ngVLA upgrade | National Radio Astronomy Observatory | 0.60 | section |
| Very Large Array | related to ngVLA upgrade | North America | 0.60 | section |
| Very Large Array | related to ngVLA upgrade | GHz | 0.60 | section |
| Very Large Array | related to ngVLA upgrade | Next Generation Very Large | 0.60 | section |
| Very Large Array | related to ngVLA upgrade | Array | 0.60 | section |
The concept neighborhoods around Very Large Array bring nearby vocabulary together. In this analysis, examples include Large, Radio and Baseline. Use the clusters to find adjacent concepts and terminology that may deserve separate research.
For Very Large Array, one of the stronger structural bridges in this analysis connects Very Large Array with History. Bridges highlight paths between different parts of the map and can reveal research angles that are easy to miss in a flat list.
TTTA analyzes the structure around Very Large Array to surface related topics, entities, relationships, concept neighborhoods and bridge connections. Use the map to explore areas such as Characters, History, Measurement & Science, including less central topics that may reveal useful research gaps. Automatically extracted connections are research leads rather than rewritten encyclopedia content.
Source: Wikipedia — Very Large Array · EN edition · Analysis: TopicsToTalkAbout