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Results 1 to 20 of 534 for query "M. Rosati". (0.00 sec.)

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Possible influence of Dark Energy on the Dark Matter Relic Abundance
Antonio Masiero; Francesca Rosati;
26 Dec 2004

Chandra X-ray analysis of the massive high-redshift galaxy clusters ClJ1113.1-2615 and ClJ0152.7-1357
B. J. Maughan; L. R. Jones; H. Ebeling; E. Perlman; P. Rosati; C. Frye; C. R. Mullis;
13 Dec 2002 / Astrophys.J. 587 (2003) 589-604

The Chandra Deep Field South: the 1 Million Second
P.Rosati; P.Tozzi; R.Giacconi; R.Gilli; G.Hasinger; L.Kewley; V.Mainieri; M.Nonino; C.Norman; G.Szokoly; J.X.Wang; A.Zirm; J.Bergeron; S.Borgani; R.Gilmozzi; N.Grogin; A.Koekemoer; E. Schreier; W.Zheng;
19 Oct 2001 / Astrophys.J.Suppl. 139 (2002) 369-410

A Serendipitous Deep Cluster Survey from ROSAT--PSPC pointed observations
P.Rosati;
9 Sep 1995

A FIRST DETERMINATION OF THE SURFACE DENSITY OF GALAXY CLUSTERS AT VERY LOW X--RAY FLUXES
P. Rosati; R. Della Ceca; R. Burg; C. Norman; R. Giacconi;
16 Mar 1995

The Possible z=0.83 Precursors of z=0 M* Early-type Cluster Galaxies
B. P. Holden; M. Franx; G. D. Illingworth; M. Postman; J. P. Blakeslee; N. Homeier; R. Demarco; H. Ford; P. Rosati; D. Kelson; K.-V. Tran;
31 Mar 2006

The XMM-2df Cluster Survey
T. Gaga; M. Plionis; I. Georgantopoulos; A. Georgakakis; S. Basilakos; G. C. Stewart; V. Kolokotronis; A. M. Stobbart;
14 Oct 2003

Scaling properties of azimuthal anisotropy in Au+Au and Cu+Cu Collisions at sqrt[s NN]=200 GeV
A Adare; S Afanasiev; C Aidala; N N Ajitan; Y Akiba; H Al-Bataineh; J Alexander; A Al-Jamel; K Aoki; L Aphecetche; R Armendariz; S H Aronson; J Asai; E T Atomssa; R Averbeck; T C Awes; B Azmoun; V Babintsev; G Baksay; L Baksay; A Baldisseri; K N Barish; P D Barnes; B Bassalleck; S Bathe; S Batsouli; V Baublis; F Bauer; A Bazilevsky; S Belikov; R Bennett; Y Berdnikov; A A Bickley; M T Bjorndal; J G Boissevain; H Borel; K Boyle; M L Brooks; D S Brown; D Bucher; H Buesching; V Bumazhnov; G Bunce; J M Burward-Hoy; S Butsyk; S Campbell; J-S Chai; B S Chang; J-L Charvet; S Chernichenko; J Chiba; C Y Chi; M Chiu; I J Choi; T Chujo; P Chung; A Churyn; V Cianciolo; C R Cleven; Y Cobigo; B A Cole; M P Comets; P Constantin; M Csanád; T Csörgo; T Dahms; K Das; G David; M B Deaton; K Dehmelt; H Delagrange; A Denisov; D d'Enterria; A Deshpande; E J Desmond; O Dietzsch; A Dion; M Donadelli; J L Drachenberg; O Drapier; A Drees; A K Dubey; A Durum; V Dzhordzhadze; Y V Efremenko; J Egdemir; F Ellinghaus; W S Emam; A Enokizono; H En'yo; B Espagnon; S Esumi; K O Eyser; D E Fields; M Finger; M Finger; F Fleuret; S L Fokin; B Forestier; Z Fraenkel; J E Frantz; A Franz; A D Frawley; K Fujiwara; Y Fukao; S-Y Fung; T Fusayasu; S Gadrat; I Garishvili; F Gastineau; M Germain; A Glenn; H Gong; M Gonin; J Gosset; Y Goto; R Granier de Cassagnac; N Grau; S V Greene; M Grosse Perdekamp; T Gunji; H-A Gustafsson; T Hachiya; A Hadj Henni; C Haegemann; J S Haggerty; M N Hagiwara; H Hamagaki; R Han; H Harada; E P Hartouni; K Haruna; M Harvey; E Haslum; K Hasuko; R Hayano; M Heffner; T K Hemmick; T Hester; J M Heuser; X He; H Hiejima; J C Hill; R Hobbs; M Hohlmann; M Holmes; W Holzmann; K Homma; B Hong; T Horaguchi; D Hornback; M G Hur; T Ichihara; K Imai; M Inaba; Y Inoue; D Isenhower; L Isenhower; M Ishihara; T Isobe; M Issah; A Isupov; B V Jacak; J Jia; J Jin; O Jinnouchi; B M Johnson; K S Joo; D Jouan; F Kajihara; S Kametani; N Kamihara; J Kamin; M Kaneta; J H Kang; H Kano; H Kanou; T Kawagishi; D Kawall; A V Kazantsev; S Kelly; A Khanzadeev; J Kikuchi; D H Kim; D J Kim; E Kim; Y-S Kim; E Kinney; A Kiss; E Kistenev; A Kiyomichi; J Klay; C Klein-Boesing; L Kochenda; V Kochetkov; B Komkov; M Konno; D Kotchetkov; A Kozlov; A Král; A Kravitz; P J Kroon; J Kubart; G J Kunde; N Kurihara; K Kurita; M J Kweon; Y Kwon; G S Kyle; R Lacey; Y-S Lai; J G Lajoie; A Lebedev; Y Le Bornec; S Leckey; D M Lee; M K Lee; T Lee; M J Leitch; M A L Leite; B Lenzi; H Lim; T Liska; A Litvinenko; M X Liu; X Li; X H Li; B Love; D Lynch; C F Maguire; Y I Makdisi; A Malakhov; M D Malik; V I Manko; Y Mao; L Masek; H Masui; F Matathias; M C McCain; M McCumber; P L McGaughey; Y Miake; P Mikes; K Miki; T E Miller; A Milov; S Mioduszewski; G C Mishra; M Mishra; J T Mitchell; M Mitrovski; A Morreale; D P Morrison; J M Moss; T V Moukhanova; D Mukhopadhyay; J Murata; S Nagamiya; Y Nagata; J L Nagle; M Naglis; I Nakagawa; Y Nakamiya; T Nakamura; K Nakano; J Newby; M Nguyen; B E Norman; A S Nyanin; J Nystr; E O'Brien; S X Oda; C A Ogilvie; H Ohnishi; I D Ojha; H Okada; K Okada; M Oka; O O Omiwade; A Oskarsson; I Otterlund; M Ouchida; K Ozawa; R Pak; D Pal; A P T Palounek; V Pantuev; V Papavassiliou; J Park; W J Park; S F Pate; H Pei; J-C Peng; H Pereira; V Peresedov; D Yu Peressounko; C Pinkenburg; R P Pisani; M L Purschke; A K Purwar; H Qu; J Rak; A Rakotozafindrabe; I Ravinovich; K F Read; S Rembeczki; M Reuter; K Reygers; V Riabov; Y Riabov; G Roche; A Romana; M Rosati; S S E Rosendahl; P Rosnet; P Rukoyatkin; V L Rykov; S S Ryu; B Sahlmueller; N Saito; T Sakaguchi; S Sakai; H Sakata; V Samsonov; H D Sato; S Sato; S Sawada; J Seele; R Seidl; V Semenov; R Seto; D Sharma; T K Shea; I Shein; A Shevel; T-A Shibata; K Shigaki; M Shimomura; T Shohjoh; K Shoji; A Sickles; C L Silva; D Silvermyr; C Silvestre; K S Sim; C P Singh; V Singh; S Skutnik; M Slunecka; W C Smith; A Soldatov; R A Soltz; W E Sondheim; S P Sorensen; I V Sourikova; F Staley; P W Stankus; E Stenlund; M Stepanov; A Ster; S P Stoll; T Sugitate; C Suire; J P Sullivan; J Sziklai; T Tabaru; S Takagi; E M Takagui; A Taketani; K H Tanaka; Y Tanaka; K Tanida; M J Tannenbaum; A Taranenko; P Tarján; T L Thomas; M Togawa; A Toia; J Tojo; L Tomásek; H Torii; R S Towell; V-N Tram; I Tserruya; Y Tsuchimoto; S K Tuli; H Tydesjö; N Tyurin; C Vale; H Valle; H W van Hecke; J Velkovska; R Vertesi; A A Vinogradov; M Virius; V Vrba; E Vznuzdaev; M Wagner; D Walker; X R Wang; Y Watanabe; J Wessels; S N White; N Willis; D Winter; C L Woody; M Wysocki; W Xie; Y L Yamaguchi; A Yanovich; Z Yasin; J Ying; S Yokkaichi; G R Young; I Younus; I E Yushmanov; W A Zajc; O Zaudtke; C Zhang; S Zhou; J Zimányi; L Zolin; ;
20 Apr 2007 / Phys Rev Lett, 98 (16), 162301

Cosmological evolution of Alpha driven by a general coupling with Quintessence
Valerio Marra; Francesca Rosati;
24 Dec 2004 / JCAP 0505 (2005) 011 DOI: 10.1088/1475-7516/2005/05/011

10.

The spatial clustering of X-ray selected AGN and galaxies in the Chandra Deep Field South and North
R. Gilli; E. Daddi; G. Zamorani; P. Tozzi; S. Borgani; J. Bergeron; R. Giacconi; G. Hasinger; V. Mainieri; C. Norman; P. Rosati; G. Szokoly; W. Zheng;
30 Sep 2004

11.

Dark Energy and the Dark Matter relic abundance
Francesca Rosati;
22 Sep 2004

12.

Quintessence and the dark matter abundance
Francesca Rosati;
11 Sep 2003

13.

Quintessential Enhancement of Dark Matter Abundance
F. Rosati;
18 Feb 2003 / Phys.Lett. B570 (2003) 5-10

14.

Scalar fields and cosmological attractor solutions
F. Rosati;
19 Oct 2002 / Proceedings of the XVIII IAP Colloquium `On the nature of dark energy', Frontier Group (2002), p.297. Edited by Ph. Brax, J. Martin, J.Ph. Uzan

15.

Renormalization Group Approach to Spin Glass Systems
G. Parisi; R. Petronzio; F. Rosati;
4 Dec 2000 / Eur. Phys. J. B 21, 605-609 (2001)

16.

X-ray temperature and morphology of z>0.8 clusters of galaxies
B. Holden; S. A. Stanford; P. Rosati; P. Tozzi; G. Squires; S. Borgani; P. Eisenhardt;
1 Oct 2001

17.

Applications of scalar attractor solutions to Cosmology
S.C.C. Ng; N.J. Nunes; F. Rosati;
17 Jul 2001 / Phys.Rev. D64 (2001) 083510

18.

Measuring $Omega_m$ with the ROSAT Deep Cluster Survey
S. Borgani; P. Rosati; P. Tozzi; S.A. Stanford; P.E. Eisenhardt; C. Lidman; B. Holden; R. Della Ceca; C. Norman; G. Squires;
24 Jun 2001

19.

Supergravity models of Quintessence and Supersymmetry breaking
Francesca Rosati;
15 Dec 2000 / Nucl.Phys.Proc.Suppl. 95 (2001) 74-77

20.

Can the Inflaton and the Quintessence scalar be the same field?
Francesca Rosati;
8 Feb 2000 / In 'COSMO-99 Proceedings of the 3^ Intern. Workshop on Particle Physics and the Early Universe', pag. 126, World Scientific (2000)

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