Zobrazeno 1 - 10
of 33 271
pro vyhledávání: '"SMITH, PAUL A."'
Autor:
Fulgaro, Ivano
Publikováno v:
Confluencia, 2022 Apr 01. 37(2), 185-186.
Externí odkaz:
https://www.jstor.org/stable/27149747
Autor:
Ma, Chutian, Smith, Paul
We consider a simplified model for optimizing a single-asset portfolio in the presence of transaction costs given a signal with a certain autocorrelation and cross-correlation structure. In our setup, the portfolio manager is given two one-parameter
Externí odkaz:
http://arxiv.org/abs/2411.07949
Autor:
Shrestha, Manisha, DeSoto, Sabrina, Sand, David J., Williams, G. Grant, Hoffman, Jennifer L., Smith, Nathan, Smith, Paul S., Milne, Peter, McCall, Callum, Maund, Justyn R., Steele, Iain A, Wiersema, Klaas, Andrews, Jennifer E., Bilinski, Christopher, Anche, Ramya M., Bostroem, K. Azalee, Hosseinzadeh, Griffin, Pearson, Jeniveve, Leonard, Douglas C., Hsu, Brian, Dong, Yize, Hoang, Emily, Janzen, Daryl, Jencson, Jacob E., Jha, Saurabh W., Lundquist, M. J., Mehta, Darshana, Retamal, Nicolas Meza, Valenti, Stefano, Farah, Joseph, Howell, D. Andrew, McCully, Curtis, Newsome, Megan, Gonzalez, Estefania Padilla, Pellegrino, Craig, Terreran, Giacomo
We present multi-epoch optical spectropolarimetric and imaging polarimetric observations of the nearby Type II supernova (SN) 2023ixf discovered in M101 at a distance of 6.85 Mpc. The first imaging polarimetric observations were taken +2.33 days (600
Externí odkaz:
http://arxiv.org/abs/2410.08199
Autor:
Heitsch, Dorothea
Publikováno v:
Renaissance Quarterly, 2020 Apr 01. 73(1), 360-361.
Externí odkaz:
https://www.jstor.org/stable/26909667
Autor:
Lee, Sukhee
Publikováno v:
T’oung Pao, 2020 Jan 01. 106(3/4), 473-476.
Externí odkaz:
https://www.jstor.org/stable/27067818
Autor:
Gokus, Andrea, Böttcher, Markus, Errando, Manel, Kreter, Michael, Heßdörfer, Jonas, Eppel, Florian, Kadler, Matthias, Smith, Paul S., Benke, Petra, Gurvits, Leonid I., Kraus, Alex, Lisakov, Mikhail, McBride, Felicia, Ros, Eduardo, Rösch, Florian, Wilms, Jörn
Blazars can be detected from very large distances due to their high luminosity. However, the detection of $\gamma$-ray emission of blazars beyond $z=3$ has only been confirmed for a small number of sources. Such observations probe the growth of super
Externí odkaz:
http://arxiv.org/abs/2406.07635
Akademický článek
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Autor:
Smid, Deanna
Publikováno v:
Renaissance Quarterly, 2019 Apr 01. 72(1), 281-283.
Externí odkaz:
https://www.jstor.org/stable/26845696