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http://hdl.handle.net/10261/170102
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dc.contributor.author | Carrera, Francisco J. | - |
dc.contributor.author | Barcons, Xavier | - |
dc.contributor.author | Butcher, J. A. | - |
dc.contributor.author | Fabian, Andrew C. | - |
dc.contributor.author | Stewart, G. C. | - |
dc.contributor.author | Warwick, R. S. | - |
dc.contributor.author | Hayashida, K. | - |
dc.contributor.author | Kii, T. | - |
dc.date.accessioned | 2018-09-24T11:08:53Z | - |
dc.date.available | 2018-09-24T11:08:53Z | - |
dc.date.issued | 1991 | - |
dc.identifier | doi: 10.1093/mnras/249.4.698 | - |
dc.identifier | issn: 0035-8711 | - |
dc.identifier | e-issn: 1365-2966 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society 249(4): 698-703 (1991) | - |
dc.identifier.uri | http://hdl.handle.net/10261/170102 | - |
dc.description.abstract | The angular autocorrelation function of the X-ray background in the energy band 4–12 keV has been explored on scales of 2∘−25∘ using 132 exposures obtained with the Large Area Counter (LAC) on board the GINGA satellite. No significant signal is found over the whole range. An upper limit at 2∘of10−4 is found for the autocorrelation function at 95 per cent confidence level, significantly lower than previous values obtained in the 2–10 keV band at 3° separation. This upper limit is shown to constrain clustering on scales about ∼10 − 300 Mpc in the high-redshift (z∼0.1−5) universe, and in particular the cluster–cluster and AGN–AGN correlation functions. | - |
dc.description.sponsorship | FC and XB thank the CICYT and the Comisión Mixta Caja Cantabria/universida de cantabria for financial help. XB and ACF acknowledge partial finacial support by a NATO Collaborative Research Grant 0250/88. ACF thanks the Royal Society for support, GCS and JB acknowledge the support of a SERC Advanced Research Fellowship and Studentship respectively. | - |
dc.publisher | Oxford University Press | - |
dc.relation.isversionof | Publisher's version | - |
dc.rights | openAccess | - |
dc.title | The correlation function of the 4-12 keV X-ray background intensity measured with the GINGA LAC | - |
dc.type | artículo | - |
dc.identifier.doi | 10.1093/mnras/249.4.698 | - |
dc.relation.publisherversion | https://doi.org/10.1093/mnras/249.4.698 | - |
dc.date.updated | 2018-09-24T11:08:53Z | - |
dc.description.version | Peer Reviewed | - |
dc.language.rfc3066 | eng | - |
dc.contributor.funder | Universidad de Cantabria | - |
dc.contributor.funder | North Atlantic Treaty Organization | - |
dc.contributor.funder | Royal Society (UK) | - |
dc.relation.csic | Sí | - |
dc.identifier.funder | http://dx.doi.org/10.13039/100004415 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100006365 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100000288 | es_ES |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.openairetype | artículo | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
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