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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/QqndG
Repositorysid.inpe.br/mtc-m17@80/2007/06.11.13.33
Last Update2007:06.11.13.33.51 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/06.11.13.33.52
Metadata Last Update2018:06.05.03.34.15 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN1365-2966
Citation KeyGuimarãesPRCDSAC:2007:EvOvAr
TitleEvidence for overdensity around zem > 4 quasars from the proximity effect
Year2007
Monthmay
Access Date2024, May 16
Secondary TypePRE PI
Number of Files1
Size432 KiB
2. Context
Author1 Guimarães, R.
2 Petitjean, P.
3 Rollinde, E.
4 Carvalho, Reinaldo Ramos de
5 Djorgovski, S. G.
6 Srianand, R.
7 Aghaee, A.
8 Castro, S.
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ5B
Group1
2
3
4 DAS-INPE-MCT-BR
Affiliation1 Observatorio Nacional (ON)
2 Institut d’Astrophysique de Paris & Universit´e Pierre et Marie Curie
3 Observatoire de Paris
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Palomar Observatory
6 Inter University Centre for Astronomy and Astrophysics (IUCAA)
7 University of Sistan and Baluchestan
8 European Southern Observatory
JournalMonthly Notices of the Royal Astronomical Society
Volume377
Pages657-666
History (UTC)2007-06-29 19:12:15 :: rosemary -> simone ::
2007-12-19 14:12:56 :: simone -> administrator ::
2012-10-23 23:53:27 :: administrator -> simone :: 2007
2013-02-20 15:19:58 :: simone -> administrator :: 2007
2018-06-05 03:34:15 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsMethods: data analysis
Methods: statistical
Galaxies: Clusters: general
Quasars: absorption lines
Dark matter
ASTROPHYSICS
AbstractWe study the density field around zem > 4 quasars using high-quality medium spectral resolution Echelle Spectrograph and ImagerKeck spectra (R ∼ 4300, signal-to-noise ratio (S/N) > 25) of 45 high-redshift quasars selected from a total of 95 spectra. This large sample considerably increases the statistics compared to previous studies. The redshift evolution of the mean photoionization rate and the median optical depth of the intergalactic medium (IGM) are derived statistically from the observed transmitted flux and the pixel optical depth probability distribution function, respectively. This is used to study the so-called proximity effect, that is, the observed decrease of the median optical depth of the IGM in the vicinity of the quasar caused by enhanced photoionization rate due to photons emitted by the quasar. We show that the proximity effect is correlated with the luminosity of the quasars, as expected. By comparing the observed decrease of the median optical depth with the theoretical expectation, we find that the optical depth does not decrease as rapidly as expected when approaching the quasar if the gas in its vicinity is part of the standard IGM.We interpret this effect as revealing gaseous overdensities on scales as large as ∼15 h−1 Mpc. The mean overdensity is of the order of 2 and 5 within, respectively, 10 and 3 h−1 Mpc. If true, this would indicate that high-redshift quasars are located in the centre of overdense regions that could evolve with time into massive clusters of galaxies. The overdensity is correlated with luminosity: brighter quasars show higher overdensities..
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Evidence for overdensity...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://mtc-m16b.sid.inpe.br/ibi/6qtX3pFwXQZGivnK2Y/QqndG
zipped data URLhttp://mtc-m16b.sid.inpe.br/zip/6qtX3pFwXQZGivnK2Y/QqndG
Languageen
Target FileEvidence for overdensity.pdf
User Groupadministrator
rosemary
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.58.48 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
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7. Description control
e-Mail (login)marciana
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