Dust Properties Of Z~2 Infrared-Luminous Lyman Break Galaxies.,
2014
University of Louisville
Dust Properties Of Z~2 Infrared-Luminous Lyman Break Galaxies., Jennifer Leigh Wojno
Electronic Theses and Dissertations
Lyman break galaxies (LBGs) are well-known indicators of star formation. By analyzing the dust of moderate redshift (z ~ 2) LBGs, we can further investigate the properties of these strongly star forming galaxies at an epoch when global star formation is expected to peak. Using data observed by the Herschel satellite, we derive far-infrared fluxes for our color-selected sample of LBGs in the GOODS-S field, including a subsample of infrared-luminous LBGs (ILLBGs). This is one of the first samples of UV dropouts/partial dropouts, which are also infrared-luminous, to be studied for their far-IR properties. Fitting modified Planck curves and model …
Multidimensional Simulations Of Non-Linear Cosmic Ray Production In Supernova Remnant Evolution,
2014
Clemson University
Multidimensional Simulations Of Non-Linear Cosmic Ray Production In Supernova Remnant Evolution, Joshua Wood
All Dissertations
When a high-mass star (& 4Msun) explodes at the end of its life, a supernova occurs, leaving its degenerate core and a fast-moving shell of matter, known as a supernova remnant (SNR). The SNR shell lasts for many thousands of years, generating emissions from low-frequency radio (~ 10-7 eV) up to γ-ray regime (~ 1015 eV). It is also believed that SNRs are the predominant source of galactic cosmic rays, accelerating a population of thermal ions, primarily protons, up to relativistic energies by means of the diffusive shock acceleration (DSA) mechanism. The small population of thermal (Boltzmann) particles, p ~ …
Search For Gravitational Wave Ringdowns From Perturbed Intermediate Mass Black Holes In Ligo-Virgo Data From 2005–2010,
2014
The University of Texas Rio Grande Valley
Search For Gravitational Wave Ringdowns From Perturbed Intermediate Mass Black Holes In Ligo-Virgo Data From 2005–2010, J. Aasi, B. P. Abbott, Matthew Benacquista, H. Daveloza, Mario C. Diaz, Soma Mukherjee, Volker Quetschke, Malik Rakhmanov, Robert Stone, Cristina V. Torres
Physics & Astronomy Faculty Publications
We report results from a search for gravitational waves produced by perturbed intermediate mass black holes (IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ringdowns, with frequency 50 ≤ f0=Hz ≤ 2000 and decay timescale 0.0001 ≲ τ=s ≲ 0.1 characteristic of those produced in mergers of IMBH pairs. No significant gravitational wave candidate was detected. We report upper limits on the astrophysical coalescence rates of IMBHs with total binary mass 50 ≤ M=M⊙ ≤ 450 and component mass …
Mri Characterization Of Cobalt Dichloride-N-Acetyl Cysteine (C4) Contrast Agent Marker For Prostate Brachytherapy,
2014
The University of Texas Rio Grande Valley
Mri Characterization Of Cobalt Dichloride-N-Acetyl Cysteine (C4) Contrast Agent Marker For Prostate Brachytherapy, Tze Yee Lim, R. Jason Stafford, Rajat J. Kudchadker, Madhuri Sankaranarayanapillai, Geoffrey Ibbott, Arvind Rao, Karen S. Martirosyan, Steven J. Frank
Physics & Astronomy Faculty Publications
Brachytherapy, a radiotherapy technique for treating prostate cancer, involves the implantation of numerous radioactive seeds into the prostate. While the implanted seeds can be easily identified on a CT image, distinguishing the prostate and surrounding soft tissues is not as straightforward. Magnetic Resonance Imaging (MRI) offers superior anatomical delineation, but the seeds appear as dark voids and are difficult to identify, thus creating a conundrum. Cobalt dichloride-N-acetylcysteine (C4) has previously been shown to be promising as an encapsulated contrast agent marker. We performed spin-lattice relaxation time (T1) and spin-spin relaxation time (T2) measurements of C4 solutions with varying cobalt dichloride …
The White Dwarfs Within 25 Pc Of The Sun: Kinematics And Spectroscopic Subtypes,
2014
Villanova University
The White Dwarfs Within 25 Pc Of The Sun: Kinematics And Spectroscopic Subtypes, Edward M. Sion, J. B. Holberg, Terry D. Oswalt, George P. Mccook, Richard Wasatonic, Janine Myszka
Publications
We present the fractional distribution of spectroscopic subtypes, range and distribution of surface temperatures, and kinematical properties of the white dwarfs (WDs) within 25 pc of the Sun. There is no convincing evidence of halo WDs in the total 25 pc sample of 224 WDs. There is also little to suggest the presence of genuine thick disk subcomponent members within 25 pc. It appears that the entire 25 pc sample likely belongs to the thin disk. We also find no significant kinematic differences with respect to spectroscopic subtypes. The total DA to non-DA ratio of the 25 pc sample is …
The Luminosity Function At Z ~ 8 From 97 Y-Band Dropouts : Inferences About Reionization.,
2014
University of California, Santa Barbara
The Luminosity Function At Z ~ 8 From 97 Y-Band Dropouts : Inferences About Reionization., Kasper B. Schmidt, Tommaso Treu, Michele Trenti, Larry D. Bradley, Brandon C. Kelly, Pascal A. Oesch, Benne W. Holwerda, J. Michael Shull, Massimo Stiavelli
Faculty and Staff Scholarship
We present the largest search to date for Y-band dropout galaxies (z ∼ 8 Lyman break galaxies, LBGs) based on 350 arcmin2 of Hubble Space Telescope observations in the V, Y, J, and H bands from the Brightest of Reionizing Galaxies (BoRG) survey. In addition to previously published data, the BoRG13 data set presented here includes approximately 50 arcmin2 of new data and deeper observations of two previous BoRG pointings, from which we present 9 new z ∼ 8 LBG candidates, bringing the total number of BoRG Y-band dropouts to 38 with 25.5 mJ 27.6 (AB system). We introduce a …
The Catalog Of Edge-On Disk Galaxies From Sdss. I. The Catalog And The Structural Parameters Of Stellar Disks,
2014
Apache Point Observatory and New Mexico State University; Moscow State University
The Catalog Of Edge-On Disk Galaxies From Sdss. I. The Catalog And The Structural Parameters Of Stellar Disks, D. V. Bizyaev, Stefan Kautsch, A. V. Mosenkov, V. P. Reshetnikov, N. Ya. Sotnikova, N. V. Yablokova
Chemistry and Physics Faculty Articles
We present a catalog of true edge-on disk galaxies automatically selected from the Seventh Data Release of the Sloan Digital Sky Survey (SDSS). A visual inspection of the g, r, and iimages of about 15,000 galaxies allowed us to split the initial sample of edge-on galaxy candidates into 4768 (31.8% of the initial sample) genuine edge-on galaxies, 8350 (55.7%) non-edge-on galaxies, and 1865 (12.5%) edge-on galaxies not suitable for simple automatic analysis because these objects either show signs of interaction and warps, or nearby bright stars project on it. We added more candidate galaxies from RFGC, EFIGI, …
Experimental Observation Of Lasing Shutdown Via Asymmetric Gain,
2014
Wesleyan University
Experimental Observation Of Lasing Shutdown Via Asymmetric Gain, M. Chitsazi, S. Factor, J. Schindler, Hamidreza Ramezani, F. M. Ellis, T. Kottos
Physics & Astronomy Faculty Publications
Using a pair of coupled RLC cavities we experimentally demonstrate that amplification action can be tamed by a spatially inhomogeneous gain. Under specific conditions we observe the counterintuitive phenomenon of stabilization of the system even when the overall gain provided is increased. This behavior is directly related to lasing shutdown via asymmetric pumping, recently proposed in M. Liertzer et al. [Phys. Rev. Lett. 108, 173901 (2012)]. The analysis of other simple systems reveals the universal nature of the lasing shutdown phenomenon as having its roots in managing impedance matching.
Where Did The First Generation Of Stars Form In The Universe,
2014
The University of San Francisco
Where Did The First Generation Of Stars Form In The Universe, Long Yan Yung, Aparna Venkatesan
Creative Activity and Research Day - CARD
The first generation of stars in the universe are expected to contain no heavy elements beyond helium, and are considered “metal-free” Population III stars (or Pop III). These metal-free stars in the early universe are predicted to have hard ionizing photon spectra and unique element yields from their supernovae, leaving signatures through the reionization of the intergalactic medium and the metal enrichment of gas in the early universe. Here, we examine the metal abundances in a variety of systems in the nearby universe, from very metal-poor Galactic halo stars to ultra-faint dwarf spheroidal galaxies, and compare them with the latest …
Psychoacoustic Effects Of High-Resolution Directivity Measurements On Room Modeling Auralizations,
2014
Brigham Young University
Psychoacoustic Effects Of High-Resolution Directivity Measurements On Room Modeling Auralizations, Nathan Eyring, Dr. Timothy Leishman
Journal of Undergraduate Research
Over the past years research has been conducted to understand how sound radiates from musical instruments. This has been done by recording a sphere of 2664 data points around a player through the process of many repetitions. This sphere is called the instrument’s directivity This data can be input into room modeling software to predict how an instrument will sound in any given location even before it is built. However there is the legitimate question of whether or not there this new data will change how room model sounds, and if someone listening would care. This research was an attempt …
Phase-Correlation And Propagation Analysis Of Near-Field Military Jet Noise,
2014
Brigham Young University
Phase-Correlation And Propagation Analysis Of Near-Field Military Jet Noise, Jazz Myres, Dr. Kent Gee
Journal of Undergraduate Research
According to the Office of Naval Research (ONR), the United States Department of Veteran Affairs spent over $1 billion dollars on military hearing loss compensation in 2010 alone1. A major cause of hearing loss is exposure to high Sound Pressure Levels, which are caused by military aircraft. These severe levels and high risks are what motivate the overarching goal of all jet noise research: to attenuate the sound impact and reduce the risk of hearing loss. My research project helps this overall purpose by characterizing jet noise and innovating more complete methods of jet noise study. The purpose of this …
Development Of A Data Reduction Pipeline For The Rovor Observatory,
2014
Brigham Young University
Development Of A Data Reduction Pipeline For The Rovor Observatory, Thayne Mccombs, Dr. Joseph Ward Moody
Journal of Undergraduate Research
The ROVOR observatory is a robotic, remotely controlled telescope in Delta, Utah. Since it is remotely controlled and semi-automated, it produces a very large amount of raw data. Unfortunately it took much longer to process and analyze the data than to acquire it, and, therefore, we had a backlog of over two years of data that was waiting to be processed. This delay in analyzing data was detrimental to monitoring projects because without the analysis of recent data it is difficult to determine the most interesting targets to observe.
Magnetic Symmetry-Mode Analysis Of La0.5 Ca0.5 Mno3,
2014
Brigham Young University
Magnetic Symmetry-Mode Analysis Of La0.5 Ca0.5 Mno3, Eric Gibbs, Dr. Branton Campell
Journal of Undergraduate Research
This project focuses on solving magnetic crystal structures using symmetry-mode analysis (SMA). A crystal is an arrangement of atoms in a repeating spatial pattern with the smallest repeating unit being known as the unit cell. A magnetic crystal contains atoms with a non-zero magnetic moment. A magnetic crystal’s unit cell repeats both the atomic and magnetic structure of the crystal. Neutron diffraction is a common method for studying magnetic crystals as the diffraction pattern can be used to determine the arrangement of atoms and magnetic moments within the unit cell.
Developing Microwave-Generated Hydrogen Atoms As A Reducing Agent For Tungsten Atomic Layer Deposition,
2014
Brigham Young University
Developing Microwave-Generated Hydrogen Atoms As A Reducing Agent For Tungsten Atomic Layer Deposition, Jason Kyle Anderson, Dr. David Allred
Journal of Undergraduate Research
Traditional micro fabrication processes are confined to a small subset of possible materials due to limitations on etching and are confined to low aspect ratio fabrication due to limits in both etching and stability of thicker film deposition processes.
Generation Of A Low Velocity Controlled Beam Of Sr Ions,
2014
Brigham Young University
Generation Of A Low Velocity Controlled Beam Of Sr Ions, Jarom Jackson, Dr. Dallin Durfee
Journal of Undergraduate Research
The purpose of this project was to produce a slow controlled beam of Strontium (Sr) ions. This is a key step in a proposed experiment to build an ion interferometer capable of measuring electric fields to a degree of sensitivity that has never been done before. This device will be useful in conducting a number of new experiments and will help test and push the boundaries of modern electromagnetic theory.
Modeling Supernovae Light Curves: A Vital Step Toward Photometric Classification,
2014
Brigham Young University
Modeling Supernovae Light Curves: A Vital Step Toward Photometric Classification, Brittany Spencer, Dr. Shane Reese
Journal of Undergraduate Research
Type Ia supernovae play a critical role in understanding the nature of the evolving universe. The Dark Energy Survey is currently investigating the expansion rate of the universe, with the intent to gain insight into the nature of dark energy. One of their primary measures of expansion is Type Ia supernovae (DES Projects, 2011). Due to this type of supernova’s uniformity in formation, most supernova of this type explode to approximately the same absolute brightness (Goobar, 2011).
Development Of A Surface Magneto-Optic Kerr Effect Magnetometer,
2014
Brigham Young University
Development Of A Surface Magneto-Optic Kerr Effect Magnetometer, Susan Stoffer Sorensen, Dr. Karine Chesnel
Journal of Undergraduate Research
The Kerr effect is a phenomenon in which as polarized visible light reflects off of a magnetized surface it experiences a small rotation in polarization. This is known as the Kerr rotation, denoted Δθ. This rotation is proportional to the magnetization of the sample, to a first-order approximation (Δθ∝M). The surface magneto-optic Kerr effect (SMOKE) is a subset of the Kerr effect which probes the magnetization of the surface of the sample. Since the samples measured by our SMOKE apparatus are as thin as 10 nm to 100 nm the surface magnetization equals the total magnetization. These samples can be …
Superparamagnetic Behavior Of Magnetite Nanoparticles: Preparation And Characterization,
2014
Brigham Young University
Superparamagnetic Behavior Of Magnetite Nanoparticles: Preparation And Characterization, Matea Trevino, Dr. Karine Chesnel
Journal of Undergraduate Research
Magnetite (Fe3O4) nanoparticles have the unique ability of being superparamagnetic. When no field is applied to the nanoparticles, the nanoparticles’ assembly has a net magnetization of zero, meaning that the nanoparticles’ magnetic moments align in random positions leading to a net magnetization of zero. When a field is applied, the particles’ magnetic moments align with the magnetic field. This is considered superparamagnetic because this is looked at on the nanometer (nm) scale and not the atomic scale. Being able to understand this phenomenon will open up many doors in technology and medical usage. Nanocrystals, such as Fe3O4 particles, are good …
Femtosecond Frequency Comb Lock,
2014
Brigham Young University
Femtosecond Frequency Comb Lock, Daniel Thrasher, Dr. Scott Bergeson
Journal of Undergraduate Research
Laser frequency control is imperative for cold atom experimentation. In our lab we use finely tuned lasers to optically cool and trap calcium atoms. Our ability to successfully trap atoms is highly dependent on the stability of the lasers we use to cool them. After trapping the atoms we use more finely tuned lasers to reveal how cold the atoms are and how quickly they leave our trap. Previous to this work our lasers were limited to 20 MHz precision. By installing a femtosecond laser as a standard by which to stabilize the other lasers in our experiment we successfully …
Dynamics Of Multi-Spin Systems : Landau-Lifshitz-Gilbert Model And Ferromagnetic Pattern Formation,
2014
Brigham Young University
Dynamics Of Multi-Spin Systems : Landau-Lifshitz-Gilbert Model And Ferromagnetic Pattern Formation, Soyoung Jung, Dr. Manuel Berrondo
Journal of Undergraduate Research
Modeling has been an important part of many fields of research. Even though it sometimes could be considered to be non-practical, it has sharpened the questions and has been a useful tool for experimental research to understand what is being observed in the laboratory. Likewise, the Heisenberg model constitutes an essential stepping stone to understand anti/ferromagnetism in magnetic materials. We have been able to develop a spin model using Landau-Lifshitz-Gilbert equation enhanced with anisotropy and long range interaction that is comparable to experimental results.
