New large-scale constraints on a phenomenological spectrum
I consider the constraints that large-scale clustering puts on a three-parameter phenomenological power spectrum. In particular, I exploit the trend of the average density in volume-limited surveys with the sample size when large-scale fluctuations are present. Applying the method to recent determin...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
01 September 1997
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 1997, Jahrgang: 290, Heft: 1, Pages: 59-65 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/290.1.59 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/290.1.59 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/290/1/59/1107953 
|
| Verfasserangaben: | Luca Amendola |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 156550609X | ||
| 003 | DE-627 | ||
| 005 | 20220814024640.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 171120s1997 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1093/mnras/290.1.59 |2 doi | |
| 035 | |a (DE-627)156550609X | ||
| 035 | |a (DE-576)495506095 | ||
| 035 | |a (DE-599)BSZ495506095 | ||
| 035 | |a (OCoLC)1340982085 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Amendola, Luca |d 1963- |e VerfasserIn |0 (DE-588)1029171270 |0 (DE-627)732547482 |0 (DE-576)377045128 |4 aut | |
| 245 | 1 | 0 | |a New large-scale constraints on a phenomenological spectrum |c Luca Amendola |
| 264 | 1 | |c 01 September 1997 | |
| 300 | |a 7 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 20.11.2017 | ||
| 520 | |a I consider the constraints that large-scale clustering puts on a three-parameter phenomenological power spectrum. In particular, I exploit the trend of the average density in volume-limited surveys with the sample size when large-scale fluctuations are present. Applying the method to recent determinations of the correlation function in volume-limited samples, it is shown that, if luminosity biasing is not dominant, then a high galaxy power spectrum normalization (bias factor larger than 2.6) or a primordial slope n > 1 is necessary. In this case, reporting even a modest scaling of the correlation function would put strong constraints on the power spectrum. If on the contrary the luminosity biasing completely accounts for the observed scaling of the correlation function, then a low normalization (bias less than or equal to unity) or n < 1 is more likely. | ||
| 773 | 0 | 8 | |i Enthalten in |a Royal Astronomical Society |t Monthly notices of the Royal Astronomical Society |d Oxford : Oxford Univ. Press, 1827 |g 290(1997), 1, Seite 59-65 |h Online-Ressource |w (DE-627)314059164 |w (DE-600)2016084-7 |w (DE-576)090955420 |x 1365-2966 |7 nnas |
| 773 | 1 | 8 | |g volume:290 |g year:1997 |g number:1 |g pages:59-65 |g extent:7 |a New large-scale constraints on a phenomenological spectrum |
| 856 | 4 | 0 | |u http://dx.doi.org/10.1093/mnras/290.1.59 |x Verlag |x Resolving-System |z kostenfrei |3 Volltext |
| 856 | 4 | 0 | |u https://academic.oup.com/mnras/article/290/1/59/1107953 |x Verlag |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20171120 | ||
| 993 | |a Article | ||
| 994 | |a 1997 | ||
| 998 | |g 1029171270 |a Amendola, Luca |m 1029171270:Amendola, Luca |p 1 |x j |y j | ||
| 999 | |a KXP-PPN156550609X |e 2987604939 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"name":{"displayForm":["Luca Amendola"]},"id":{"doi":["10.1093/mnras/290.1.59"],"eki":["156550609X"]},"origin":[{"dateIssuedDisp":"01 September 1997","dateIssuedKey":"1997"}],"relHost":[{"physDesc":[{"extent":"Online-Ressource"}],"origin":[{"publisherPlace":"Oxford ; Oxford [u.a.] ; Oxford [u.a.]","dateIssuedKey":"1827","publisher":"Oxford Univ. Press ; Blackwell ; Wiley-Blackwell","dateIssuedDisp":"1827-"}],"id":{"issn":["1365-2966"],"eki":["314059164"],"doi":["10.1111/(ISSN)1365-2966"],"zdb":["2016084-7"]},"pubHistory":["1.1827 -"],"part":{"text":"290(1997), 1, Seite 59-65","volume":"290","extent":"7","year":"1997","pages":"59-65","issue":"1"},"type":{"bibl":"periodical","media":"Online-Ressource"},"note":["Gesehen am 15.01.2018"],"disp":"Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society","corporate":[{"display":"Royal Astronomical Society","roleDisplay":"VerfasserIn","role":"aut"}],"language":["eng"],"recId":"314059164","title":[{"title_sort":"Monthly notices of the Royal Astronomical Society","title":"Monthly notices of the Royal Astronomical Society"}]}],"physDesc":[{"extent":"7 S."}],"person":[{"role":"aut","roleDisplay":"VerfasserIn","display":"Amendola, Luca","given":"Luca","family":"Amendola"}],"title":[{"title":"New large-scale constraints on a phenomenological spectrum","title_sort":"New large-scale constraints on a phenomenological spectrum"}],"language":["eng"],"recId":"156550609X","type":{"bibl":"article-journal","media":"Online-Ressource"},"note":["Gesehen am 20.11.2017"]} | ||
| SRT | |a AMENDOLALUNEWLARGESC0119 | ||