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CERN Document Server 15 records found  1 - 10próximo  jump to record: Search took 0.70 seconds. 
1.
Cosmology with the Laser Interferometer Space Antenna / LISA Cosmology Working Group Collaboration
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. [...]
arXiv:2204.05434; LISA CosWG-22-03; FERMILAB-PUB-22-349-SCD.- 2023-08-28 - 176 p. - Published in : Living Rev. Relativ. 26 (2023) 5 Fulltext: jt - PDF; 2204.05434 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
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2.
Dark Matter Science in the Era of LSST / Bechtol, Keith (Wisconsin U., Madison) ; Drlica-Wagner, Alex (Chicago U., Astron. Astrophys. Ctr. ; Chicago U., KICP ; Fermilab) ; Abazajian, Kevork N. (UC, Irvine) ; Abidi, Muntazir (Cambridge U., DAMTP) ; Adhikari, Susmita (KIPAC, Menlo Park) ; Ali-Haïmoud, Yacine (New York U.) ; Annis, James (Fermilab) ; Ansarinejad, Behzad (Durham U.) ; Armstrong, Robert (LLNL, Livermore) ; Asorey, Jacobo (Queensland U. ; Unlisted, AU) et al.
Astrophysical observations currently provide the only robust, empirical measurements of dark matter. [...]
arXiv:1903.04425. - 2019. - 11 p.
Fulltext
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3.
Electromagnetic probes of primordial black holes as dark matter / Kashlinsky, A. (NASA, Goddard ; SSAI, Lanham) ; Ali-Haimoud, Y. (New York U.) ; Clesse, S. (Louvain U. ; Namur U.) ; Garcia-Bellido, J. (Madrid, IFT ; CSIC, Madrid) ; Wyrzykowski, L. (Warsaw U.) ; Achucarro, A. (Leiden U.) ; Amendola, L. (Heidelberg U.) ; Annis, J. (Fermilab) ; Arbey, A. (Lyon, IPN) ; Arendt, R.G. (NASA, Goddard ; Maryland U., Baltimore County) et al.
The LIGO discoveries have rekindled suggestions that primordial black holes (BHs) may constitute part to all of the dark matter (DM) in the Universe. [...]
arXiv:1903.04424 ; FERMILAB-PUB-19-111-CD. - 2019 - 19.
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4.
Dark Energy Survey Year 1 Results: Constraints on Intrinsic Alignments and their Colour Dependence from Galaxy Clustering and Weak Lensing / DES Collaboration
We perform a joint analysis of intrinsic alignments and cosmology using tomographic weak lensing, galaxy clustering and galaxy-galaxy lensing measurements from Year 1 (Y1) of the Dark Energy Survey. We define early- and late-type subsamples, which are found to pass a series of systematics tests, including for spurious photometric redshift error and point spread function correlations. [...]
arXiv:1811.06989; FERMILAB-PUB-18-622-AE.- 2019-11-11 - 30 p. - Published in : Mon. Not. R. Astron. Soc. 489 (2019) 5453-5482 Fulltext: 1811.06989 - PDF; fermilab-pub-18-622-ae - PDF; openaccess_stz2197 - PDF; External link: Fermilab Accepted Manuscript
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5.
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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6.
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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7.
Applying Chimera Virtual Data Concepts To Cluster Finding In The Sloan Sky Survey / Annis, J
FERMILAB-CONF-2002-180-A. - 2002.
Fulltext from Fermilab
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8.
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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9.
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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10.
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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Veja também: nomes de autores similares
99 Annis, J
3 Annis, J T
40 Annis, James
2 Annis, James T
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