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"Bowler, Troy"
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Trading the fixed income, inflation and credit markets : a relative value guide
\"In this book, the authors give an applied approach to relative value techniques, showing readers how to decide on the best place to put their money in order to get the best return. They cover multiple asset classes - fixed income, commodities and equities although the main focus is fixed income. They cover products that are rarely documented such as CMS floaters and structured interest and credit products. The initial part of the book will consider the main derivative products and their pricing interrelationships. It argues that within any asset class there are mathematical relationships that tie together four key building blocks: cash products, forwards / futures, swaps and options. The nature of these interrelationships means that there may be a variety of different ways in which a particular strategy can be expressed. The second part of the book will be focused primarily on relative value within a fixed income context and will look at strategies that build on the pricing relationships between products as well as those that focus on how to identify the optimal way to express a view on the movement of the yield curve. The third part of the book will take the main themes of relative value and show how they could be applied within other asset classes. \"-- Provided by publisher.
Planet Hunters. VIII. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data
by
Poile, Trevor
,
Wang, Ji
,
Dean Joseph Simister
in
Adaptive optics
,
Astronomical catalogs
,
Extrasolar planets
2015
The census of exoplanets is incomplete for orbital distances larger than 1 AU. Here, we present 41 long-period planet candidates in 38 systems identified by Planet Hunters based on Kepler archival data (Q0-Q17). Among them, 17 exhibit only one transit, 14 have two visible transits and 10 have more than three visible transits. For planet candidates with only one visible transit, we estimate their orbital periods based on transit duration and host star properties. The majority of the planet candidates in this work (75%) have orbital periods that correspond to distances of 1-3 AU from their host stars. We conduct follow-up imaging and spectroscopic observations to validate and characterize planet host stars. In total, we obtain adaptive optics images for 33 stars to search for possible blending sources. Six stars have stellar companions within 4\". We obtain high-resolution spectra for 6 stars to determine their physical properties. Stellar properties for other stars are obtained from the NASA Exoplanet Archive and the Kepler Stellar Catalog by Huber et al. (2014). We validate 7 planet candidates that have planet confidence over 0.997 (3-{\\sigma} level). These validated planets include 3 single-transit planets (KIC-3558849b, KIC-5951458b, and KIC-8540376c), 3 planets with double transits (KIC-8540376b, KIC-9663113b, and KIC-10525077b), and 1 planet with 4 transits (KIC-5437945b). This work provides assessment regarding the existence of planets at wide separations and the associated false positive rate for transiting observation (17%-33%). More than half of the long-period planets with at least three transits in this paper exhibit transit timing variations up to 41 hours, which suggest additional components that dynamically interact with the transiting planet candidates. The nature of these components can be determined by follow-up radial velocity and transit observations.