Atomic Data for Resonance Absorption Lines. III. Wavelengths Longward of the Lyman Limit for the Elements Hydrogen to Gallium

By D. Morton. 2003

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Subfields: Atomic and Molecular Physics, and Optics, Mechanics of Materials, Statistics and Probability

View Paper: https://www.semanticscholar.org/paper/2308a43d859694c5664c1af073395086443b12d6

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Citations in the corpus

THE COS-HALOS SURVEY: AN EMPIRICAL DESCRIPTION OF METAL-LINE ABSORPTION IN THE LOW-REDSHIFT CIRCUMGALACTIC MEDIUM (2012, methodology): “For all line measurements, we have used atomic data from Morton (2003).”
THE BIMODAL METALLICITY DISTRIBUTION OF THE COOL CIRCUMGALACTIC MEDIUM AT z ≲ 1 (2013, background): “The atomic parameters are for the UV transitions from Morton (2003) and for the EUV transitions from Verner et al. (1994).”
An improved measurement of the flux distribution of the Lyα forest in QSO absorption spectra: the effect of continuum fitting, metal contamination and noise properties (2007, background): “The rest-frame wavelengths and oscillator strengths for transitions from these ions are given by Morton (2003).”
The Structure of the Local Interstellar Medium. V. Electron Densities (2007, positive): “The program makes use of rest wavelengths and oscillator strengths from Morton (2003), and the instrumental line spread functions for GHRS and STIS spectra are taken from Gilliland (1994) and Sahu et al. (1999), respectively.”
Deuterium abundance in the most metal-poor damped Lyman alpha system: converging on Ωb,0h2 (2008, methodology): “We used the compilation of laboratory wavelengths λlab and f-values by Morton (2003).”
DEMOGRAPHICS AND PHYSICAL PROPERTIES OF GAS OUTFLOWS/INFLOWS AT 0.4 < z < 1.4 (2012, methodology): “We adopt the atomic oscillator strengths and cosmic abundance ratios given by Morton (2003) as well as the associated vacuum wavelengths for transitions shortward of 3200Å.”
C, N, O abundances in the most metal-poor damped Lyman alpha systems★ (2007, methodology): “VPFIT takes into account the instrumental broadening function in its χ2 minimisation and error evaluation.4 We used the compilation of laboratory wavelengths and f -values by Morton (2003) with recent updates by Jenkins & Tripp (2006).”
EXTREME FEEDBACK AND THE EPOCH OF REIONIZATION: CLUES IN THE LOCAL UNIVERSE (2011, methodology): “We will use the following transitions (with the respective values of logλf from Morton 2003): SiλII1260.”
STUDIES OF THE DIFFUSE INTERSTELLAR BANDS. III. HD 183143 (2009, positive): “The zero point of the DIB wavelength scale adopted here is set by assigning the laboratory wavelength of 7698.9645 Å (Morton 2003) to the stronger of the two K i components.”
The evolution of the cosmic microwave background temperature Measurements of TCMB at high redshift from carbon monoxide excitation (2010, background): “For example, the accuracy of the oscillator strengths of C0 fine-structure levels (e.g. Jenkins & Tripp, 2001; Morton, 2003) is subject to discussions.”
Molecular hydrogen in high-redshift Damped Lyman-alpha systems: The VLT/UVES database (2008, methodology): “Solar abundances as listed in Morton (2003), based on meteoritic data from Grevesse & Sauval (2002), were adopted.”
A new, precise measurement of the primordial abundance of deuterium (2012, methodology): “Multiplet wavelengths for the emission lines were taken from Morton (2003).”
The most metal-poor damped Lyα systems: insights into chemical evolution in the very metal-poor regime★ (2011, background): “Table 3 lists laboratory wavelengths and oscillator strengths of relevant atomic transitions from the compilation by Morton (2003), with subsequent updates by Jenkins & Tripp (2006).”
PHYSICAL CONDITIONS IN A YOUNG, UNREDDENED, LOW-METALLICITY GALAXY AT HIGH REDSHIFT (2010, background): “For the two Si II lines, the oscillator strengths of the blue and red transitions are 1.18 and 0.133 respectively (Morton 2003), so that in the optically thin case W (1260)/W (1527) = 6.0.”
A UNIFIED REPRESENTATION OF GAS-PHASE ELEMENT DEPLETIONS IN THE INTERSTELLAR MEDIUM (2009, methodology): “Assigned errors of −0.10 dex and +0.20 dex; (22) Mostly used f -values from Morton (2003), but found deviations for two lines.”
The Circumgalactic Medium (2017, background): “Complete line lists are available in Morton (2003). that the relationship between O vi column density and absorption-line width for a wide range of physically diverse environments indicates a generic origin of O vi in collisionallyionized gas.”
Spatial variation in the fine-structure constant – new results from VLT/UVES (2012, background): “Column 12 shows the oscillator strengths, f , taken from Morton (2003) or the relative strengths of the hyperfine or isotopic components.”
The elemental composition of the Sun: II. The iron group elements Sc to Ni (2014, methodology): “We used the compilations of Martin et al. (1988), Fuhr et al. (1988), Doidge (1995) and especially Morton (2003) as guides and secondary comparators.”