110 results on '"Kaluzny, J"'
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2. Plasma cleaning of the SLAC Linac Coherent Light Source II high energy verification cryomodule cavities
3. 200 MV record voltage of vCM and LCLS-II-HE cryomodules production start at FERMILAB [Poster]
4. High gradient performance and quench behavior of a verification cryomodule for a high energy continuous wave linear accelerator
5. Results of plasma processing applied to the LCLS-II-HE vCM cavities [Poster]
6. Preparation and Characterization of TeO2 Based Glasses
7. LCLS-II 1.3 GHz cryomodule design - lessons learned from testing at Fermilab
8. Effects of thermal acoustic oscillations on LCLS-II cryomodule testing
9. Operational experience from LCLS-II cryomodule testing
10. A ground-based proper motion study of 12 nearby globular clusters
11. Stainless steel to titanium bimetallic transitions
12. THE CLUSTER AGES EXPERIMENT (CASE). VII. ANALYSIS OF TWO ECLIPSING BINARIES IN THE GLOBULAR CLUSTER NGC 6362
13. Activity of Contact Binaries
14. The First DIRECT Distance to a Detached Eclipsing Binary in M33
15. SALT long-slit spectroscopy of LBQS 2113-4538: variability of the Mg II and Fe II component
16. New Observations of the Old Magnetic Nova GQ Muscae
17. Two low-cost, modular sub-λ test cryostats
18. THE CLUSTER AGES EXPERIMENT (CASE). V. ANALYSIS OF THREE ECLIPSING BINARIES IN THE GLOBULAR CLUSTER M4
19. Absolute parameters of AE For – a highly active detached binary of late K type★
20. A SECOND NEUTRON STAR IN M4?
21. A VIMOS spectroscopy study of photometric variables and straggler candidates inω Centauri
22. A proper motion study of the globular cluster M55
23. Absolute properties of BG Ind - a bright F3 system just leaving the main sequence★
24. A search for dormant binaries with degenerate components inω Centauri and NGC 6397
25. THE CLUSTER AGES EXPERIMENT (CASE). IV. ANALYSIS OF THE ECLIPSING BINARY V69 IN THE GLOBULAR CLUSTER 47 Tuc
26. Electro-optical characterization of Ge–Se–Te glasses
27. A Large-Scale Survey for Variable Stars in M 33
28. A complete census of variable stars in the upper half of the HR diagram in M 33
29. Cluster AgeS Experiment (CASE): deficiency of observed dwarf novae in globular clusters
30. Correlation of spectral optical coherence tomography with fluorescein and indocyanine green angiography in multiple evanescent white dot syndrome
31. THE CLUSTER AGES EXPERIMENT (CASE). III. ANALYSIS OF THE ECCENTRIC ECLIPSING BINARY V32 IN THE GLOBULAR CLUSTER NGC 6397
32. Paucity of Dwarf Novae in Globular Clusters
33. Variable stars in the field of the old open cluster Melotte 66
34. The Clusters Ages Experiment (CASE). II. The Eclipsing Blue Straggler OGLEGC 228 in the Globular Cluster 47 Tuc
35. The Clusters Ages Experiment (CASE). I. V209 ω Cen: An Eclipsing Post-Common-Envelope Binary in the Globular Cluster ω Cen
36. The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33
37. Deep Canada���France���Hawaii Telescope photometric survey of the entire M33 galaxy ��� I. Catalogue of 36���000 variable point sources
38. The First DIRECT Distance to a Detached Eclipsing Binary in M33
39. Photometric study of the variable star population in the globular cluster NGC 6397
40. CCD photometry of distant open clusters NGC 2425, Haffner 10 and Czernik 29
41. Cluster Ages Experiment (CASE): SX Phe stars from the globular cluster Centauri
42. Coherent noise-free ophthalmic imaging by spectral optical coherence tomography
43. Cluster Ages Experiment (CASE): Detection of a dwarf nova in the globular cluster M55
44. Preparation and Characterization of TeO2 Based Glasses
45. BVIPhotometric Variability Survey of M3
46. Eclipsing binaries in globular clusters as age and distance indicators
47. Cluster AgeS Experiment Catalog of variable stars in the globular clusterω Centauri
48. Photometry and Spectroscopy of GRB 030329 and Its Associated Supernova 2003dh: The First Two Months
49. Cluster AgeS Experiment (CASE): RR Lyrae stars from the globular cluster ω Centauri as standard candles
50. DIRECT Distances to Nearby Galaxies Using Detached Eclipsing Binaries and Cepheids. IX. Variables in the Field M31Y Discovered with Image Subtraction
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