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  • 73.20.Dx  (1)
  • Astronomy  (1)
  • 2005-2009
  • 1995-1999  (2)
  • 1960-1964
  • 1940-1944
  • 1
    ISSN: 1573-7357
    Keywords: 79.60.Bm ; 73.20.Dx ; 74.70.Ad ; 74.80.Dm
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract With high-resolution (≈22 meV) angle-resolved photoemission spectroscopy, the Fermi surface of the first copper free layered-perovskite superconductor, Sr2RuO4, was determined. We observed three bands to cross the Fermi energy in qualitative agreement with LDA band structure calculations; one electron-like surface encircling the $$\overline \Gamma$$ point in the projected Brillouin zone, and two hole-like surfaces around the $$\overline X$$ point. The most striking aspect of the measurements is the observation of an extended van Hove singularity. It is located 17 meV below the Fermi energy and extends around the $$\overline M$$ point for about 0.2 Å−1 along both the $$\overline \Gamma$$ — $$\overline M$$ — $$\overline \Gamma$$ and the $$\overline X$$ — $$\overline M$$ — $$\overline X$$ directions.These observations demonstrate that van Hove singularities near the Fermi surface are a more generic feature of layered oxides, and call for a clarification of their exact role in oxide superconductivity.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-08-15
    Description: The ROSAT Deep Survey includes a complete sample of 50 X-ray sources with fluxes in the 0.5 - 2 keV band larger than 5.5 x 10(exp -15)erg/sq cm/s in the Lockman field (Hasinger et al., Paper 1). We have obtained deep broad-band CCD images of the field and spectra of many optical objects near the positions of the X-ray sources. We define systematically the process leading to the optical identifications of the X-ray sources. For this purpose, we introduce five identification (ID) classes that characterize the process in each case. Among the 50 X-ray sources, we identify 39 AGNs, 3 groups of galaxies, 1 galaxy and 3 galactic stars. Four X-ray sources remain unidentified so far; two of these objects may have an unusually large ratio of X-ray to optical flux.
    Keywords: Astronomy
    Type: ASTRO-PH/9709144 , Astronomy and Astrophysics (ISSN 0004-6361)
    Format: text
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