79 results on '"Castellano, M"'
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2. Early Results from GLASS-JWST. XV. Properties of the Faintest Red Sources in the NIRCAM Deep Fields.
3. Early Results From GLASS-JWST. XII. The Morphology of Galaxies at the Epoch of Reionization.
4. Early Results from GLASS-JWST. X. Rest-frame UV-optical Properties of Galaxies at 7 < z < 9.
5. Early Results from GLASS-JWST. XI. Stellar Masses and Mass-to-light Ratio of z > 7 Galaxies.
6. Euclid: Estimation of the Impact of Correlated Readout Noise for Flux Measurements with the Euclid NISP Instrument*
7. The first flight of the OLIMPO experiment: instrument performance
8. Euclid: Estimation of the Impact of Correlated Readout Noise for Flux Measurements with the Euclid NISP Instrument.
9. Kinetic Inductance Detectors and readout electronics for the OLIMPO experiment
10. Kinetic inductance detectors for the OLIMPO experiment: design and pre-flight characterization
11. Constraints on Dynamical Dark Energy Models from the Abundance of Massive Galaxies at High Redshifts.
12. Al/Ti/Al phonon-mediated KIDs for UV–vis light detection over large areas
13. Exploring cosmic origins with CORE: Cluster science
14. Characterization of a fabrication process for the integration of superconducting qubits and rapid-single-flux-quantum circuits
15. CALDER - Neutrinoless double-beta decay identification in TeO2bolometers with kinetic inductance detectors
16. First non-intercepting emittance measurement by means of optical diffraction radiation interference
17. Observation of 65 GHz Coherent Oscillation in a Superconducting Flux Qubit Manipulated by Pulses
18. Characterization of anomalous pair currents in Josephson junction networks
19. Artificial neural network based on SQUIDs: demonstration of network training and operation
20. The THz Radiation Source at the SPARC Facility
21. Non-intercepting diagnostic for high brightness electron beams using Optical Diffraction Radiation Interference (ODRI)
22. The THz radiation source at SPARC
23. Superconducting qubit manipulated by fast pulses: experimental observation of distinct decoherence regimes
24. Deep-well ultrafast manipulation of a SQUID flux qubit
25. A tunable rf SQUID manipulated as flux and phase qubits
26. Coherent oscillations in a superconducting tunable flux qubit manipulated without microwaves
27. Quantum dynamics of a microwave-driven SQUID
28. The EXPLORER gravitational wave antenna: recent improvements and performances
29. Characterization of superconducting devices spanning the charging to Josephson regimes
30. An integrated system of SQUIDs for the study of macroscopic quantum coherence
31. DIFFUSE OPTICAL INTRACLUSTER LIGHT AS A MEASURE OF STELLAR TIDAL STRIPPING: THE CLUSTER CL0024+17 AT z ∼ 0.4 OBSERVED AT THE LARGE BINOCULAR TELESCOPEObservations have been carried out using the Large Binocular Telescope at Mt. Graham, AZ. The LBT is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are the University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; the Ohio State University; and The Research Corporation, on behalf of the University of Notre Dame, University of Minnesota, and University of Virginia.
32. An absolute magnetometer based on dc Superconducting QUantum Interference Devices
33. SERENDIPITOUS DISCOVERY OF A MASSIVE cD GALAXY AT z = 1.096: IMPLICATIONS FOR THE EARLY FORMATION AND LATE EVOLUTION OF cD GALAXIES.
34. SPECTROSCOPIC CONFIRMATION OF z ~ 7 LYMAN BREAK GALAXIES: PROBING THE EARLIEST GALAXIES AND THE EPOCH OF REIONIZATION.
35. A LOW ESCAPE FRACTION OF IONIZING PHOTONS OF L > L* LYMAN BREAK GALAXIES AT z = 3.3.
36. First Cooling Below 0.1 K of the New Gravitational-Wave Antenna “Nautilus” of the Rome Group
37. Sensitivity of the Rome Gravitational Wave Experiment with the Explorer Cryogenic Resonant Antenna Operating at 2 K
38. Kinetic Inductance Detectors for the OLIMPO experiment: in-flight operation and performance.
39. Erratum: Kinetic inductance detectors for the OLIMPO experiment: design and pre-flight characterization.
40. Data Recordered by the Rome Room Temperature Gravitational Wave Antenna, during the Supernova SN 1987 a in the Large Magellanic Cloud
41. Exploring cosmic origins with CORE: The instrument.
42. STELLAR MASSES FROM THE CANDELS SURVEY: THE GOODS-SOUTH AND UDS FIELDS.
43. NEW OBSERVATIONS OF z ∼ 7 GALAXIES: EVIDENCE FOR A PATCHY REIONIZATION.
44. PdBI COLD DUST IMAGING OF TWO EXTREMELY RED H – [4.5] > 4 GALAXIES DISCOVERED WITH SEDS AND CANDELS.
45. EVIDENCE OF VERY LOW METALLICITY AND HIGH IONIZATION STATE IN A STRONGLY LENSED, STAR-FORMING DWARF GALAXY AT z = 3.417.
46. Observation of 65 GHz Coherent Oscillation in a Superconducting Flux Qubit Manipulated by Pulses.
47. CHARACTERIZING FAINT GALAXIES IN THE REIONIZATION EPOCH: LBT CONFIRMS TWO L < 0.2 L⋆ SOURCES AT z = 6.4 BEHIND THE CLASH/FRONTIER FIELDS CLUSTER MACS0717.5+3745The Large Binocular Telescope (LBT) is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are: The University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; The Ohio State University; and The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota, and University of Virginia.
48. ACTIVE GALACTIC NUCLEI AS MAIN CONTRIBUTORS TO THE ULTRAVIOLET IONIZING EMISSIVITY AT HIGH REDSHIFTS: PREDICTIONS FROM A Λ-CDM MODEL WITH LINKED AGN/GALAXY EVOLUTION.
49. The Cosmic-Ray Electron and Positron Spectra Measured at 1 AU during Solar Minimum Activity.
50. Data Recordered by the Rome Room Temperature Gravitational Wave Antenna, during the Supernova SN 1987a in the Large Magellanic Cloud.
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