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CERN Document Server 2,030 record trovati  1 - 10successivofine  salta al record: La ricerca ha impiegato 0.84 secondi. 
1.
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The circumstellar environment of low-mass protostars / Motte, F (Bonn, Max Planck Inst., Radioastron. ; DAPNIA, Saclay) ; André, P (DAPNIA, Saclay)
DAPNIA-SAP-2000-63.- Saclay : DAPNIA, 2001 - 30 p. - Published in : Astron. Astrophys. 365 (2001) 440-464 Access to fulltext document: PDF;
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Usage of the CERN MORPURGO magnet for the MADMAX prototype / MADMAX Collaboration
The MAgnetized Disk and Mirror Axion eXperiment (MADMAX) is a new initiative to search for dark matter axions in the mass range of 40 to 400 $\mu$eV. [...]
CERN-SPSC-2020-012 ; SPSC-P-366. - 2020. - 32.
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3.
(47)
FIRST and the earliest stages of star formation / André, P ; Motte, F
DAPNIA-SAP-2000-02. - 2000.
Access to fulltext document - Access to fulltext document
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The second data release from the European Pulsar Timing Array - IV. Implications for massive black holes, dark matter, and the early Universe / EPTA Collaboration
The European Pulsar Timing Array (EPTA) and Indian Pulsar Timing Array (InPTA) collaborations have measured a low-frequency common signal in the combination of their second and first data releases respectively, with the correlation properties of a gravitational wave background (GWB). Such signal may have its origin in a number of physical processes including a cosmic population of inspiralling supermassive black hole binaries (SMBHBs); inflation, phase transitions, cosmic strings and tensor mode generation by non-linear evolution of scalar perturbations in the early Universe; oscillations of the Galactic potential in the presence of ultra-light dark matter (ULDM). [...]
arXiv:2306.16227.- 2024-05-01 - 30 p. - Published in : Astron. Astrophys. 685 (2024) A94 Fulltext: 2306.16227 - PDF; document - PDF;
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Kinematics of millimeter prestellar condensations in the $\rho$ Ophiuchi protocluster / Belloche, A ; André, P ; Motte, F
DAPNIA-SAP-2001-36.- Saclay : DAPNIA, 2001 - 6 p. - Published in : Astron. Soc. Pac. Conf. Proc.: 243 (2001) Access to fulltext document: PDF;
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One-pion-exchange model analysis of the $\delta^{++}$ (1236) region and of the n $\pi^{+}$ low-mass enhancement in the reaction pp -> p $\pi^{+}$ n / Lipatov, L N (Hamburg U. ; St. Petersburg Nuclear Physics Institute) ; Carmony, D D (Max-Planck-Inst. München) ; Fesefeldt, H S (DESY, Hamburg) ; Franz, H (Max-Planck-Inst. München) ; Kobe, P (Bonn Univ.) ; Hellwig, B (DESY, Hamburg) ; Mönkemeyer, D (DESY, Hamburg) ; Schrankel, W (Max-Planck-Inst. München) ; Schwarz, B (Max-Planck-Inst. München) ; Selonke, F (Bonn Univ.) et al.
1973 - Published in : Nucl. Phys. B 67 (1973) 284-308
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One-pion-exchange model analysis of the $\lambda^{++}$ (1236) region and of the n $\pi^{+}$ low-mass enhancement / Blobel, Volker (DESY, Hamburg) ; Carmony, D D (Max-Planck Inst. München) ; Fesefeldt, H S (DESY, Hamburg) ; Franz, H (Max-Planck Inst. München) ; Hellwig, B (DESY, Hamburg) ; Kobe, P (Bonn Univ.) ; Mönkemeyer, D (DESY, Hamburg) ; Schrankel, W (Max-Planck Inst. München) ; Schwarz, B (DESY, Hamburg) ; Selonke, F (Bonn Univ.) et al.
1973 - Published in : Nucl. Phys. B 67 (1973) 284-308
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The International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background / Antoniadis, J. (FORTH, Heraklion ; Bonn, Max Planck Inst., Radioastron. ; Argelander Inst. Astron.) ; Arzoumanian, Z. (NASA, Goddard) ; Babak, S. (APC, Paris) ; Bailes, M. (Swinburne U. Tech., Hawthorn ; ARC, CoEPP, Australia) ; Nielsen, A.-S. Bak (Bonn, Max Planck Inst., Radioastron. ; Bielefeld U.) ; Baker, P.T. (Widener U.) ; Bassa, C.G. (ASTRON, Dwingeloo) ; Becsy, B. (Montana State U.) ; Berthereau, A. (LPC2E, Orleans ; Station Radioastronomy, Nancay) ; Bonetti, M. (Milan Bicocca U. ; INFN, Milan Bicocca) et al.
We searched for an isotropic stochastic gravitational wave background in the second data release of the International Pulsar Timing Array, a global collaboration synthesizing decadal-length pulsar-timing campaigns in North America, Europe, and Australia. In our reference search for a power law strain spectrum of the form $h_c = A(f/1\,\mathrm{yr}^{-1})^{\alpha}$, we found strong evidence for a spectrally-similar low-frequency stochastic process of amplitude $A = 3.8^{+6.3}_{-2.5}\times10^{-15}$ and spectral index $\alpha = -0.5 \pm 0.5$, where the uncertainties represent 95% credible regions, using information from the auto- and cross-correlation terms between the pulsars in the array. [...]
arXiv:2201.03980.- 2022-01-27 - 15 p. - Published in : Mon. Not. R. Astron. Soc. 510 (2022) 4873 Fulltext: PDF;
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AGAPEROS : Searches for microlensing in the LMC with the Pixel Method; 2, Selection of possible microlensing events / Melchior, A.L. (Queen Mary, U. of London ; College de France) ; Afonso, C (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Ansari, R (Orsay, LAL) ; Aubourg, E. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Baillon, P. (CERN) ; Bareyre, P. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Bauer, F. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Beaulieu, J.-Ph. (Paris, Inst. Astrophys.) ; Bouquet, A. (College de France) ; Brehin, S. (CEA, DSM, Saclay ; DAPNIA, Saclay) et al.
We apply the pixel method of analysis (sometimes called ``pixel lensing'') to a small subset of the EROS-1 microlensing observations of the bar of the Large Magellanic Cloud (LMC). The pixel method is designed to find microlensing events of unresolved source stars and had heretofore been applied only to M31 where essentially all sources are unresolved. [...]
astro-ph/9804321.- 1998 - 14 p. - Published in : Astron. Astrophys. 339 (1998) 658 Access to fulltext document: PDF; External link: astro-ph/9804321 PDF
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Enhanced production of low-mass electron pairs in 200 GeV/u S - Au collisions at the CERN-SPS / NA45 Collaboration
CERN-PPE-95-26.- Geneva : CERN, 1995 - 8 p. - Published in : Phys. Rev. Lett. 75 (1995) 1272-1275 APS Published version, local copy: PDF; Access to fulltext document: PDF; - CERN library copies
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