CERN Accelerating science

CERN Document Server 32 record trovati  1 - 10successivofine  salta al record: La ricerca ha impiegato 0.60 secondi. 
1.
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
2.
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
3.
Constraints on the Richness-Mass Relation and the Optical-SZE Positional Offset Distribution for SZE-Selected Clusters / DES Collaboration
We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg$^2$ of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey (DES) science verification data. We identify 25 clusters between $0.1\lesssim z\lesssim 0.8$ in the union of the SPT-SZ and redMaPPer (RM) samples. [...]
arXiv:1506.07814; FERMILAB-PUB-15-295-AE.- 2015-12-11 - 15 p. - Published in : Mon. Not. R. Astron. Soc. 454 (2015) 2305-2319 Fulltext: arXiv:1506.07814 - PDF; openaccess_MNRAS-2015-Saro-2305-19 - PDF; Oxford Univ. Press Open Access article: PDF; External links: Fermilab Library Server (fulltext available); Open Access fulltext
4.
Theoretical Advanced Study Institute in Elementary Particle Physics - Physics of the Large and the Small TASI 2009   1 - 26 June 2009  - Boulder, CO, USA  / Csaki, Csaba (ed.); Dodelson, Scott (ed.)
This volume presents a set of pedagogical lectures that introduce particle physics beyond the standard model and particle cosmology to advanced graduate students..
Singapore : World Scientific, 2009
e-proceedings
5.
Constraining cosmological dark matter annihilation with gamma ray observations / Dodelson, Scott (Fermilab ; Chicago U., Astron. Astrophys. Ctr. ; Chicago U., KICP) ; Belikov, Alexander V. (Chicago U.) ; Hooper, Dan (Fermilab ; Chicago U., Astron. Astrophys. Ctr.) ; Serpico, Pasquale (Fermilab ; CERN)
Annihilation of cosmologically distributed dark matter is predicted to produce a potentially observable flux of high energy photons. Neglecting the contribution from local structure, this signal is predicted to be virtually uniform on the sky and, in order to be identified, must compete with various extragalactic backgrounds. [...]
arXiv:0903.2829; FERMILAB-PUB-09-063-A; CERN-PH-TH-2009-030.- 2009 - 8 p. - Published in : Phys. Rev. D 80 (2009) 083504 APS Published version, local copy: PDF; Fulltext: PDF; External link: Fermilab Library Server (fulltext available)
6.
CMBPol Mission Concept Study: Probing Inflation with CMB Polarization / Baumann, Daniel (Harvard U., Phys. Dept. ; Harvard U. ; Princeton U.) ; Jackson, Mark G. (Fermilab ; Leiden U.) ; Adshead, Peter (Yale U.) ; Amblard, Alexandre (UC, Irvine) ; Ashoorioon, Amjad (Michigan U.) ; Bartolo, Nicola (Padua U.) ; Bean, Rachel ; Beltran, Maria (Chicago U., KICP) ; de Bernardis, Francesco (Rome U.) ; Bird, Simeon (Cambridge U.) et al.
We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measurements to differentiate various inflationary mechanisms. [...]
arXiv:0811.3919; FERMILAB-PUB-08-601-A; CERN-PH-TH-2008-230.- 2009-06-17 - 107 p. - Published in : AIP Conf. Proc. 1041 (2009) 10-120 Fulltext: fermilab-pub-08-601-a - PDF; arXiv:0811.3919 - PDF; External link: Fermilab Library Server (fulltext available)
In : Workshop on CMB Polarization Theory and Foregrounds, Batavia, IL, USA, 23 - 26 Jun 2008, pp.10-120
7.
Workshop on CMB Polarization Theory and Foregrounds - CMB Polarization Theory and Foregrounds   23 - 26 Jun 2008  - Batavia, IL, USA  / Dodelson, Scott (ed.); Baumann, Daniel (ed.); Cooray, Asantha (ed.); Dunkley, Joanna (ed.); Fraisse, Aurelien (ed.); Jackson, Mark G (ed.); Kogut, Alan (ed.); Krauss, Lawrence (ed.); Zaldarriaga, Matias (ed.); Smith, Kendrick (ed.)
New York, NY : AIP, 2009 - 324 p.
8.
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)
9.
Stellar-Mass Black Holes in the Solar Neighborhood / Chisholm, James R. (Fermilab ; Chicago U.) ; Dodelson, Scott (Fermilab ; Chicago U., Astron. Astrophys. Ctr.) ; Kolb, Edward W. (CERN ; Fermilab ; Chicago U., Astron. Astrophys. Ctr.)
We search for nearby, isolated, accreting, ``stellar-mass'' (3 to $100M_\odot$) black holes. Models suggest a synchrotron spectrum in visible wavelengths and some emission in X-ray wavelengths. [...]
astro-ph/0205138; FERMILAB-PUB-02-036-A; CERN-TH-2002-032; CERN-TH-2002-032; FERMILAB-PUB-2002-036-A.- Geneva : CERN, 2003 - 33 p. - Published in : Astrophys. J. 596 (2003) 437 Access to fulltext document: PDF; Fulltext: arXiv:astro-ph_0205138 - PDF; Pub-02-036-A - PDF; External links: Fulltext; Fermilab Library Server (fulltext available) - Please contact the library if you need to access this document.
10.
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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