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CERN Document Server 2,045 Datensätze gefunden  1 - 10nächsteEnde  gehen zum Datensatz: Die Suche hat 2.43 Sekunden gedauert. 
1.
(100)
KL Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early SDSS Data / SDSS Collaboration
We present measurements of parameters of the 3-dimensional power spectrum of galaxy clustering from 222 square degrees of early imaging data in the Sloan Digital Sky Survey. The projected galaxy distribution on the sky is expanded over a set of Karhunen-Loeve eigenfunctions, which optimize the signal-to-noise ratio in our analysis. [...]
astro-ph/0107419; FERMILAB-PUB-01-270-A; FERMILAB-PUB-2001-270-A.- Batavia, IL : FERMILAB, 2002 - 25 p. - Published in : Astrophys. J. 571 (2002) 191-205 Access to fulltext document: PDF; Fulltext: arXiv:astro-ph_0107419 - PDF; Pub-01-270-A - PDF; External link: Fermilab Library Server (fulltext available)
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2.
(91)
The First Data Release of the Sloan Digital Sky Survey / SDSS Collaboration
The Sloan Digital Sky Survey has validated and made publicly available its First Data Release. This consists of 2099 square degrees of five-band (u, g, r, i, z) imaging data, 186,240 spectra of galaxies, quasars, stars and calibrating blank sky patches selected over 1360 square degrees of this area, and tables of measured parameters from these data. [...]
astro-ph/0305492; FERMILAB-PUB-03-176-A.- Princeton, NJ : Princeton Univ., 2003 - 16 p. - Published in : Astron. J. 126 (2003) 2081 Access to fulltext document: 0305492.fig1 - PS.GZ; 0305492.fig3 - PS.GZ; 0305492.fig2 - PS.GZ; 0305492.fig5 - PS.GZ; 0305492.fig4 - PS.GZ; 0305492 - PDF; Fulltext: PDF; External link: Fermilab Library Server (fulltext available)
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3.
(91)
Galaxy Clustering in Early SDSS Redshift Data / SDSS Collaboration
We present the first measurements of clustering in the Sloan Digital Sky Survey (SDSS) galaxy redshift survey. Our sample consists of 29,300 galaxies with redshifts 5,700 km/s < cz < 39,000 km/s, distributed in several long but narrow (2.5-5 degree) segments, covering 690 square degrees. [...]
astro-ph/0106476; FERMILAB-PUB-01-091-A; FERMILAB-PUB-2001-091-A.- Batavia, IL : FERMILAB, 2002 - 54 p. - Published in : Astrophys. J. 571 (2002) 172-190 Access to fulltext document: 0106476.fig6 - PS.GZ; 0106476.fig7 - PS.GZ; 0106476.fig4 - PS.GZ; 0106476.fig5 - PS.GZ; 0106476.fig2 - PS.GZ; 0106476 - PDF; 0106476.fig1 - PS.GZ; 0106476.fig13 - PS.GZ; 0106476.fig8 - PS.GZ; 0106476.fig9 - PS.GZ; 0106476.fig18 - PS.GZ; 0106476.fig19 - PS.GZ; 0106476.fig14 - PS.GZ; 0106476.fig15 - PS.GZ; 0106476.fig16 - PS.GZ; 0106476.fig17 - PS.GZ; 0106476.fig10 - PS.GZ; 0106476.fig11 - PS.GZ; 0106476.fig12 - PS.GZ; 0106476.fig3 - PS.GZ; Fulltext: Pub-01-091-A - PDF; arXiv:astro-ph_0106476 - PDF; External link: Fermilab Library Server (fulltext available)
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4.
(90)
The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data / SDSS Collaboration
Early photometric data from the Sloan Digital Sky Survey (SDSS) contain angular positions for 1.5 million galaxies. In companion papers, the angular correlation function $w(\theta)$ and 2D power spectrum $C_l$ of these galaxies are presented. [...]
astro-ph/0107421; FERMILAB-PUB-01-271-A; FERMILAB-PUB-2001-271-A.- Batavia, IL : FERMILAB, 2001 - 25 p. - Published in : Astrophys. J. 572 (2001) 140-156 Access to fulltext document: PDF; Fulltext: Pub-01-271-A - PDF; arXiv:astro-ph_0107421 - PDF; External link: Fermilab Library Server (fulltext available)
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5.
(68)
Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies and the Distant Universe / Blanton, Michael R. (Stanford U., Phys. Dept.) ; Bershady, Matthew A. (Wisconsin U., Madison, Astron.) ; Abolfathi, Bela ; Albareti, Franco D. (Madrid, Autonoma U. ; Madrid, IFT) ; Allende Prieto, Carlos ; Almeida, Andres ; Alonso-García, Javier ; Anders, Friedrich (Potsdam, Astrophys. Inst.) ; Anderson, Scott F. (LLNL, Livermore) ; Andrews, Brett et al.
We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratio in the near-infrared. [...]
arXiv:1703.00052.- 2017 - Published in : Astron. J. 154 (2017) 28 Fulltext: PDF;
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6.
(55)
The Second Data Release of the Sloan Digital Sky Survey / SDSS Collaboration
The Sloan Digital Sky Survey has validated and made publicly available its Second Data Release. This data release consists of 3324 square degrees of five-band (u g r i z) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars and calibrating blank sky patches selected over 2627 degrees of this area, and tables of measured parameters from these data. [...]
astro-ph/0403325; FERMILAB-PUB-04-360-A.- 2004 - 24 p. - Published in : Astron. J. 128 (2004) 502-512 Fulltext: PDF; External link: Fermilab Library Server (fulltext available)
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7.
(54)
Planck 2015 results. V. LFI calibration / Planck Collaboration
We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. [...]
arXiv:1505.08022.- 2016-09-20 - 24 p. - Published in : Astron. Astrophys. 594 (2016) A5 Fulltext: PDF; External link: Preprint
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8.
(51)
Celestial mechanics : perspectives for the next ten years / Miller, R H (Chicago U., Astron. Astrophys. Ctr.)
1986 - Published in : Part. Accel.: 19 (1986) , pp. 257-262 Fulltext: PDF;
In : Workshop on Orbital Dynamics and Applications to Accelerators, Berkeley, CA, USA, 7 - 12 Mar 1985, pp.257-262
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9.
(49)
Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts / Planck Collaboration
We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. [...]
arXiv:1303.5080; CERN-PH-TH-2013-133; CERN-PH-TH-2013-133.- 2014-10-29 - 20 p. - Published in : Astron. Astrophys. 571 (2014) A20 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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10.
(44)
Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters / Planck Collaboration
This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of CMB temperature and polarization. They use the hybrid approach employed previously: pixel-based at low multipoles, $\ell$, and a Gaussian approximation to the distribution of cross-power spectra at higher $\ell$. [...]
arXiv:1507.02704.- 2016-09-20 - 99 p. - Published in : Astron. Astrophys. 594 (2016) A11 Fulltext: PDF; External link: Preprint
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