Ontology type: schema:ScholarlyArticle
2006-05
AUTHORSN. S. Soboleva, N. N. Bursov, A. V. Temirova
ABSTRACTWe discuss the results of deep surveys of a ±10′ strip of the sky, centered on the declination of SS 433, carried out on the Northern sector of the RATAN-600 telescope at 2.7 and 7.6 cm in 1987–2000. The survey objects are cross-identified with sources in the NVSS catalog and the corresponding two-frequency spectral indices determined. We find a decrease in the mean spectral index in the transition from objects with flux densities S21 ≥ 30 mJy to those with 15 < S21 < 30 mJy. The constructed log N — logS relation at 2.7 cm has a slope of 3/2 at flux densities ≥300 mJy and flattens at weaker flux densities. The 1.4 GHz (NVSS), 3.94 GHz (RATAN-600), and 11.11 GHz (RATAN-600) data are used to estimate the number of objects per square degree at a wavelength of 1 cm. More... »
PAGES341-345
http://scigraph.springernature.com/pub.10.1134/s1063772906050015
DOIhttp://dx.doi.org/10.1134/s1063772906050015
DIMENSIONShttps://app.dimensions.ai/details/publication/pub.1040451815
JSON-LD is the canonical representation for SciGraph data.
TIP: You can open this SciGraph record using an external JSON-LD service: JSON-LD Playground Google SDTT
[
{
"@context": "https://springernature.github.io/scigraph/jsonld/sgcontext.json",
"about": [
{
"id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/02",
"inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/",
"name": "Physical Sciences",
"type": "DefinedTerm"
},
{
"id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0201",
"inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/",
"name": "Astronomical and Space Sciences",
"type": "DefinedTerm"
}
],
"author": [
{
"affiliation": {
"alternateName": "St. Petersburg Division, Special Astrophysical Observatory, St. Petersburg, Russia",
"id": "http://www.grid.ac/institutes/grid.452760.2",
"name": [
"St. Petersburg Division, Special Astrophysical Observatory, St. Petersburg, Russia"
],
"type": "Organization"
},
"familyName": "Soboleva",
"givenName": "N. S.",
"id": "sg:person.012140616525.36",
"sameAs": [
"https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012140616525.36"
],
"type": "Person"
},
{
"affiliation": {
"alternateName": "Special Astrophysical Observatory, Nizhni\u012d Arkhyz, Russia",
"id": "http://www.grid.ac/institutes/grid.452760.2",
"name": [
"Special Astrophysical Observatory, Nizhni\u012d Arkhyz, Russia"
],
"type": "Organization"
},
"familyName": "Bursov",
"givenName": "N. N.",
"id": "sg:person.010360541444.22",
"sameAs": [
"https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010360541444.22"
],
"type": "Person"
},
{
"affiliation": {
"alternateName": "St. Petersburg Division, Special Astrophysical Observatory, St. Petersburg, Russia",
"id": "http://www.grid.ac/institutes/grid.452760.2",
"name": [
"St. Petersburg Division, Special Astrophysical Observatory, St. Petersburg, Russia"
],
"type": "Organization"
},
"familyName": "Temirova",
"givenName": "A. V.",
"id": "sg:person.013342041244.02",
"sameAs": [
"https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013342041244.02"
],
"type": "Person"
}
],
"datePublished": "2006-05",
"datePublishedReg": "2006-05-01",
"description": "We discuss the results of deep surveys of a \u00b110\u2032 strip of the sky, centered on the declination of SS 433, carried out on the Northern sector of the RATAN-600 telescope at 2.7 and 7.6 cm in 1987\u20132000. The survey objects are cross-identified with sources in the NVSS catalog and the corresponding two-frequency spectral indices determined. We find a decrease in the mean spectral index in the transition from objects with flux densities S21 \u2265 30 mJy to those with 15 < S21 < 30 mJy. The constructed log N \u2014 logS relation at 2.7 cm has a slope of 3/2 at flux densities \u2265300 mJy and flattens at weaker flux densities. The 1.4 GHz (NVSS), 3.94 GHz (RATAN-600), and 11.11 GHz (RATAN-600) data are used to estimate the number of objects per square degree at a wavelength of 1 cm.",
"genre": "article",
"id": "sg:pub.10.1134/s1063772906050015",
"isAccessibleForFree": false,
"isPartOf": [
{
"id": "sg:journal.1136138",
"issn": [
"0004-6299",
"1063-7729"
],
"name": "Astronomy Reports",
"publisher": "Pleiades Publishing",
"type": "Periodical"
},
{
"issueNumber": "5",
"type": "PublicationIssue"
},
{
"type": "PublicationVolume",
"volumeNumber": "50"
}
],
"keywords": [
"SS 433",
"RATAN-600 telescope",
"spectral index",
"weak flux densities",
"mean spectral index",
"Deep Survey",
"NVSS catalog",
"square degrees",
"GHz data",
"survey objects",
"flux density",
"telescope",
"mJy",
"sky",
"declination",
"GHz",
"wavelength",
"objects",
"catalogue",
"transition",
"flux",
"S21",
"density",
"number of objects",
"source",
"index",
"results",
"strips",
"relation",
"slope",
"decrease",
"data",
"number",
"degree",
"survey",
"sector",
"northern sector"
],
"name": "Deep RATAN-600 surveys at the declination of SS 433 carried out in 1987\u20132000 at 7.6 and 2.7 cm",
"pagination": "341-345",
"productId": [
{
"name": "dimensions_id",
"type": "PropertyValue",
"value": [
"pub.1040451815"
]
},
{
"name": "doi",
"type": "PropertyValue",
"value": [
"10.1134/s1063772906050015"
]
}
],
"sameAs": [
"https://doi.org/10.1134/s1063772906050015",
"https://app.dimensions.ai/details/publication/pub.1040451815"
],
"sdDataset": "articles",
"sdDatePublished": "2022-08-04T16:55",
"sdLicense": "https://scigraph.springernature.com/explorer/license/",
"sdPublisher": {
"name": "Springer Nature - SN SciGraph project",
"type": "Organization"
},
"sdSource": "s3://com-springernature-scigraph/baseset/20220804/entities/gbq_results/article/article_415.jsonl",
"type": "ScholarlyArticle",
"url": "https://doi.org/10.1134/s1063772906050015"
}
]
Download the RDF metadata as: json-ld nt turtle xml License info
JSON-LD is a popular format for linked data which is fully compatible with JSON.
curl -H 'Accept: application/ld+json' 'https://scigraph.springernature.com/pub.10.1134/s1063772906050015'
N-Triples is a line-based linked data format ideal for batch operations.
curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1134/s1063772906050015'
Turtle is a human-readable linked data format.
curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1134/s1063772906050015'
RDF/XML is a standard XML format for linked data.
curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1134/s1063772906050015'
This table displays all metadata directly associated to this object as RDF triples.
110 TRIPLES
20 PREDICATES
62 URIs
54 LITERALS
6 BLANK NODES
Subject | Predicate | Object | |
---|---|---|---|
1 | sg:pub.10.1134/s1063772906050015 | schema:about | anzsrc-for:02 |
2 | ″ | ″ | anzsrc-for:0201 |
3 | ″ | schema:author | Ne8e837d1fa604033b0fe580bc5afabc5 |
4 | ″ | schema:datePublished | 2006-05 |
5 | ″ | schema:datePublishedReg | 2006-05-01 |
6 | ″ | schema:description | We discuss the results of deep surveys of a ±10′ strip of the sky, centered on the declination of SS 433, carried out on the Northern sector of the RATAN-600 telescope at 2.7 and 7.6 cm in 1987–2000. The survey objects are cross-identified with sources in the NVSS catalog and the corresponding two-frequency spectral indices determined. We find a decrease in the mean spectral index in the transition from objects with flux densities S21 ≥ 30 mJy to those with 15 < S21 < 30 mJy. The constructed log N — logS relation at 2.7 cm has a slope of 3/2 at flux densities ≥300 mJy and flattens at weaker flux densities. The 1.4 GHz (NVSS), 3.94 GHz (RATAN-600), and 11.11 GHz (RATAN-600) data are used to estimate the number of objects per square degree at a wavelength of 1 cm. |
7 | ″ | schema:genre | article |
8 | ″ | schema:isAccessibleForFree | false |
9 | ″ | schema:isPartOf | N01a47f878c274bccbb061dcc28162bb1 |
10 | ″ | ″ | Nbfdd837659ab45dfaed8f7fb0a44e625 |
11 | ″ | ″ | sg:journal.1136138 |
12 | ″ | schema:keywords | Deep Survey |
13 | ″ | ″ | GHz |
14 | ″ | ″ | GHz data |
15 | ″ | ″ | NVSS catalog |
16 | ″ | ″ | RATAN-600 telescope |
17 | ″ | ″ | S21 |
18 | ″ | ″ | SS 433 |
19 | ″ | ″ | catalogue |
20 | ″ | ″ | data |
21 | ″ | ″ | declination |
22 | ″ | ″ | decrease |
23 | ″ | ″ | degree |
24 | ″ | ″ | density |
25 | ″ | ″ | flux |
26 | ″ | ″ | flux density |
27 | ″ | ″ | index |
28 | ″ | ″ | mJy |
29 | ″ | ″ | mean spectral index |
30 | ″ | ″ | northern sector |
31 | ″ | ″ | number |
32 | ″ | ″ | number of objects |
33 | ″ | ″ | objects |
34 | ″ | ″ | relation |
35 | ″ | ″ | results |
36 | ″ | ″ | sector |
37 | ″ | ″ | sky |
38 | ″ | ″ | slope |
39 | ″ | ″ | source |
40 | ″ | ″ | spectral index |
41 | ″ | ″ | square degrees |
42 | ″ | ″ | strips |
43 | ″ | ″ | survey |
44 | ″ | ″ | survey objects |
45 | ″ | ″ | telescope |
46 | ″ | ″ | transition |
47 | ″ | ″ | wavelength |
48 | ″ | ″ | weak flux densities |
49 | ″ | schema:name | Deep RATAN-600 surveys at the declination of SS 433 carried out in 1987–2000 at 7.6 and 2.7 cm |
50 | ″ | schema:pagination | 341-345 |
51 | ″ | schema:productId | N852a7dc42b1a4b57822266a2718f50ca |
52 | ″ | ″ | Nc80c14d702b44bed8c28ee902754fa70 |
53 | ″ | schema:sameAs | https://app.dimensions.ai/details/publication/pub.1040451815 |
54 | ″ | ″ | https://doi.org/10.1134/s1063772906050015 |
55 | ″ | schema:sdDatePublished | 2022-08-04T16:55 |
56 | ″ | schema:sdLicense | https://scigraph.springernature.com/explorer/license/ |
57 | ″ | schema:sdPublisher | Nc07a391297bb41df89de599ac113d525 |
58 | ″ | schema:url | https://doi.org/10.1134/s1063772906050015 |
59 | ″ | sgo:license | sg:explorer/license/ |
60 | ″ | sgo:sdDataset | articles |
61 | ″ | rdf:type | schema:ScholarlyArticle |
62 | N01a47f878c274bccbb061dcc28162bb1 | schema:volumeNumber | 50 |
63 | ″ | rdf:type | schema:PublicationVolume |
64 | N852a7dc42b1a4b57822266a2718f50ca | schema:name | dimensions_id |
65 | ″ | schema:value | pub.1040451815 |
66 | ″ | rdf:type | schema:PropertyValue |
67 | Nbfc43cc0edba4a2e9a5f75899deb5dd0 | rdf:first | sg:person.013342041244.02 |
68 | ″ | rdf:rest | rdf:nil |
69 | Nbfdd837659ab45dfaed8f7fb0a44e625 | schema:issueNumber | 5 |
70 | ″ | rdf:type | schema:PublicationIssue |
71 | Nc07a391297bb41df89de599ac113d525 | schema:name | Springer Nature - SN SciGraph project |
72 | ″ | rdf:type | schema:Organization |
73 | Nc80c14d702b44bed8c28ee902754fa70 | schema:name | doi |
74 | ″ | schema:value | 10.1134/s1063772906050015 |
75 | ″ | rdf:type | schema:PropertyValue |
76 | Ne8e837d1fa604033b0fe580bc5afabc5 | rdf:first | sg:person.012140616525.36 |
77 | ″ | rdf:rest | Nfd2dcf7f7bd74e08b6a13f6d21466bc0 |
78 | Nfd2dcf7f7bd74e08b6a13f6d21466bc0 | rdf:first | sg:person.010360541444.22 |
79 | ″ | rdf:rest | Nbfc43cc0edba4a2e9a5f75899deb5dd0 |
80 | anzsrc-for:02 | schema:inDefinedTermSet | anzsrc-for: |
81 | ″ | schema:name | Physical Sciences |
82 | ″ | rdf:type | schema:DefinedTerm |
83 | anzsrc-for:0201 | schema:inDefinedTermSet | anzsrc-for: |
84 | ″ | schema:name | Astronomical and Space Sciences |
85 | ″ | rdf:type | schema:DefinedTerm |
86 | sg:journal.1136138 | schema:issn | 0004-6299 |
87 | ″ | ″ | 1063-7729 |
88 | ″ | schema:name | Astronomy Reports |
89 | ″ | schema:publisher | Pleiades Publishing |
90 | ″ | rdf:type | schema:Periodical |
91 | sg:person.010360541444.22 | schema:affiliation | grid-institutes:grid.452760.2 |
92 | ″ | schema:familyName | Bursov |
93 | ″ | schema:givenName | N. N. |
94 | ″ | schema:sameAs | https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010360541444.22 |
95 | ″ | rdf:type | schema:Person |
96 | sg:person.012140616525.36 | schema:affiliation | grid-institutes:grid.452760.2 |
97 | ″ | schema:familyName | Soboleva |
98 | ″ | schema:givenName | N. S. |
99 | ″ | schema:sameAs | https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012140616525.36 |
100 | ″ | rdf:type | schema:Person |
101 | sg:person.013342041244.02 | schema:affiliation | grid-institutes:grid.452760.2 |
102 | ″ | schema:familyName | Temirova |
103 | ″ | schema:givenName | A. V. |
104 | ″ | schema:sameAs | https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013342041244.02 |
105 | ″ | rdf:type | schema:Person |
106 | grid-institutes:grid.452760.2 | schema:alternateName | Special Astrophysical Observatory, Nizhniĭ Arkhyz, Russia |
107 | ″ | ″ | St. Petersburg Division, Special Astrophysical Observatory, St. Petersburg, Russia |
108 | ″ | schema:name | Special Astrophysical Observatory, Nizhniĭ Arkhyz, Russia |
109 | ″ | ″ | St. Petersburg Division, Special Astrophysical Observatory, St. Petersburg, Russia |
110 | ″ | rdf:type | schema:Organization |