Countering weapons of mass destruction

Autor: Pete V. Domenici

Publikováno v: The Washington Quarterly. 18:143-152

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::4c442babcf63454b6e2779645d48e7a2
https://doi.org/10.1080/01636609509550137

The Reality of Science Funding

Autor: Pete V. Domenici

Publikováno v: Science. 273:1319-1319

The author is a Republican Senator from New Mexico. When John F. Kennedy was president, over two-thirds of the federal budget was available for discretionary spending, the category of federal spending that supports vital national missions such as the

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::96171c4b0549923b37ff843096d3b7a1
https://doi.org/10.1126/science.273.5280.1319

A swordof Damocles for the debt

Autor: Pete V. Domenici, Alice Rivlin

Publikováno v: Washington Post, The. 05/16/2011.

A dusty compact object bridging galaxies and quasars at cosmic dawn.

Autor: Fujimoto S; Cosmic Dawn Center (DAWN), Copenhagen, Denmark. fujimoto@nbi.ku.dk.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark. fujimoto@nbi.ku.dk., Brammer GB; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Watson D; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Magdis GE; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.; DTU-Space, Technical University of Denmark, Kongens Lyngby, Denmark., Kokorev V; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Greve TR; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; DTU-Space, Technical University of Denmark, Kongens Lyngby, Denmark., Toft S; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Walter F; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Max Planck Institute for Astronomy, Heidelberg, Germany.; National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, Socorro, NM, USA., Valiante R; INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy., Ginolfi M; European Southern Observatory, Garching, Germany., Schneider R; INAF-Osservatorio Astronomico di Roma, Monteporzio Catone, Italy.; Dipartimento di Fisica, Universitá di Roma La Sapienza, Rome, Italy., Valentino F; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Colina L; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Centro de Astrobiología (CAB, CSIC-INTA), Madrid, Spain., Vestergaard M; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.; Steward Observatory, University of Arizona, Tucson, AZ, USA., Marques-Chaves R; Geneva Observatory, University of Geneva, Versoix, Switzerland., Fynbo JPU; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Krips M; IRAM, Domaine Universitaire, Saint-Martin-d'Hères, France., Steinhardt CL; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Cortzen I; IRAM, Domaine Universitaire, Saint-Martin-d'Hères, France., Rizzo F; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Oesch PA; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Geneva Observatory, University of Geneva, Versoix, Switzerland.

Publikováno v: Nature [Nature] 2022 Apr; Vol. 604 (7905), pp. 261-265. Date of Electronic Publication: 2022 Apr 13.

Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6.

Autor: Decarli R; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Walter F; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany.; National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, PO Box O, Socorro, New Mexico 87801, USA.; Astronomy Department, California Institute of Technology, MC105-24, Pasadena, California 91125, USA., Venemans BP; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Bañados E; The Observatories of the Carnegie Institute of Washington, 813 Santa Barbara Street, Pasadena, California 91101, USA., Bertoldi F; Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, Bonn 53121, Germany., Carilli C; National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, PO Box O, Socorro, New Mexico 87801, USA.; Battcock Centre for Experimental Astrophysics, Cavendish Laboratory, Cambridge CB3 0HE, UK., Fan X; Steward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA., Farina EP; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Mazzucchelli C; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Riechers D; Cornell University, 220 Space Sciences Building, Ithaca, New York 14853, USA., Rix HW; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Strauss MA; Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08533, USA., Wang R; Kavli Institute of Astronomy and Astrophysics at Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, China., Yang Y; Korea Astronomy and Space Science Institute, Daedeokdae-ro 776, Yuseong-gu Daejeon 34055, South Korea.

Publikováno v: Nature [Nature] 2017 May 24; Vol. 545 (7655), pp. 457-461.