Parameter-Mapping Sonification of Tick-Data

Author(s):  
David Worrall
Keyword(s):  
2014 ◽  
Author(s):  
Jason Foran ◽  
Mark C. Hutchinson ◽  
Niall O'Sullivan

2021 ◽  
Vol 85 (6) ◽  
pp. 3211-3226
Author(s):  
Fang Liu ◽  
Richard Kijowski ◽  
Georges El Fakhri ◽  
Li Feng

2015 ◽  
Vol 15 (8) ◽  
pp. 1365-1374 ◽  
Author(s):  
Maria Pia Beccar Varela ◽  
Francis Biney ◽  
Ionut Florescu

2021 ◽  
Vol 923 (1) ◽  
pp. 78
Author(s):  
Amit N. Sawant ◽  
Eric W. Pellegrini ◽  
M. S. Oey ◽  
Jesús López-Hernández ◽  
Genoveva Micheva

Abstract We employ ionization-parameter mapping (IPM) to infer the optical depth of H ii regions in the northern half of M33. We construct [O iii]λ5007/[O ii]λ3727 and [O iii]λ5007/[S ii]λ6724 ratio maps from narrowband images continuum-subtracted in this way, from which we classify the H ii regions by optical depth to ionizing radiation, based on their ionization structure. This method works relatively well in the low-metallicity regime, 12 + log ( O / H ) ≤ 8.4 , where [O iii]λ λ4959, 5007 is strong. However, at higher metallicities, the method breaks down due to the strong dependence of the [O iii]λ λ4959, 5007 emission lines on the nebular temperature. Thus, although O++ may be present in metal-rich H ii regions, these commonly used emission lines do not serve as a useful indicator of its presence, and hence the O ionization state. In addition, IPM as a diagnostic of optical depth is limited by spatial resolution. We also report a region of highly excited [O iii] extending over an area ∼1 kpc across and [O iii]λ5007 luminosity of 4.9 ± 1.5 × 1038 erg s−1, which is several times higher than the ionizing budget of any potential sources in this portion of the galaxy. Finally, this work introduces a new method for continuum subtraction of narrowband images based on the dispersion of pixels around the mode of the diffuse-light flux distribution. In addition to M33, we demonstrate the method on C iii]λ1909 imaging of Haro 11, ESO 338-IG004, and Mrk 71.


2018 ◽  
Vol 31 (12) ◽  
pp. e4008 ◽  
Author(s):  
Georg R. Spinner ◽  
Johannes F.M. Schmidt ◽  
Constantin von Deuster ◽  
Christian Federau ◽  
Christian T. Stoeck ◽  
...  

Author(s):  
Yacine Aïıt-Sahalia ◽  
Jean Jacod

This chapter covers the various problems arising in the estimation of the integrated volatility when the observations are contaminated by a noise. The approach used is quite partial, and fundamentally phenomenological, in contrast with a microeconomical approach. That is, the authors assumed the existence of an underlying (nonobservable) efficient price, and what is called noise below is by definition the difference between the observed price and the efficient price. Henceforth, it certainly does not apply to tick-by-tick data, even if these were regularly spaced in time (which they are not). In the whole chapter, with the exception of one section, the underlying process X is one-dimensional.


2014 ◽  
Vol 73 (2) ◽  
pp. 655-661 ◽  
Author(s):  
Tao Zhang ◽  
John M. Pauly ◽  
Ives R. Levesque

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