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![Rational Contagion and the Globalization of Securities Markets](https://writelatex.s3.amazonaws.com/published_ver/2451.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=adc02660e2527a171c59e3ebf98f9c518413721a40887a6e59e7b1673f078d00)
Rational Contagion and the Globalization of Securities Markets
Presentation with equations
Chen Yuting
![Prática 04 - Capacidade Térmica](https://writelatex.s3.amazonaws.com/published_ver/4583.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=52625de12ed094f79df0ea07dfdc345958ee416cc280245ed5075740ae13b1fe)
Prática 04 - Capacidade Térmica
Trabalho em grupo
Egmon Pereira
![Vedanshu Nagar's Résumé](https://writelatex.s3.amazonaws.com/published_ver/9686.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=c3bf1a80566454d0e319421b644e86e11e954773836e8c0b94fecf3f79c0ca15)
Vedanshu Nagar's Résumé
Vedanshu Nagar's Résumé
Vedanshu Nagar
![Two Simple Proofs for Cramer's Rule](https://writelatex.s3.amazonaws.com/published_ver/3647.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=608c987f73e43c5d530983050b661a9dcb53271a221abbd38fbfd40fdde5d10b)
Two Simple Proofs for Cramer's Rule
Cramer's rule is usually explained by cofactor expansion of determinant. This note explains two alternative and simple proofs.
Frank the Bunny
![Aditya Tikone's Résumé](https://writelatex.s3.amazonaws.com/published_ver/9654.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=b1b25f01492441f2a6874f2cda30353debe8bb2c2c8d5498e90efb0a12219312)
Aditya Tikone's Résumé
Aditya Tikone's résumé. Created based on the Deedy CV template.
Aditya Tikone
![Iftkharul islam Parvez's CV](https://writelatex.s3.amazonaws.com/published_ver/9666.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=f50d5aa045c7b3136c9eda3e46b4475087d84fa6a9a6c06a61cd0d44bde13c7e)
Iftkharul islam Parvez's CV
Iftkharul islam Parvez's CV. Created with the Twenty Seconds CV template.
Iftekhar
![Research Report of Characterizing Transient Noise Sources to Find Gravitational wave Signals From Black Holes](https://writelatex.s3.amazonaws.com/published_ver/9641.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=860f965cc21a232d7216b339de6d4e1fda56bf107e40f337c27b01c7beed0900)
Research Report of Characterizing Transient Noise Sources to Find Gravitational wave Signals From Black Holes
With the detectors currently off, LIGO has detected and gathered an abundance of data from the second observing run (O2). Some of which, captures the most recent triggers that are potential candidates for future gravitational waves, are analyzed more thoroughly. My responsibility as a student researcher is to perform independent checks on four of the most recent Compact Binary Coalescence (CBC) triggers. In order to do so, I compare the \(h(t)\) Omega scans of these events to the Gravity Spy classes. Omega scans are a detector characterization tool to help measure the Signal-to-Noise-Ratio (SNR) of transient noises during detections. This helps scientists distinguish the difference between a gravitational wave signal, which looks like a `chirp' versus a glitch in the data. Gravity Spy is a citizen science program that helps LIGO in classifying glitches to improve machine learning for gravitational wave signals. For each event I determine if it looks like one of the known categories of solved or unsolved glitches seen in the Advanced LIGO detectors? My results are then recorded in the O2 event detection checklist. Omega scans are a `burst-type' search pipeline that detect glitches efficiently. The Omega scan is labeled using time measured in seconds on the x-axis, frequency measured in Hz on the y-axis and the signal measured is normalized to demonstrate how `loud' the noise is.
Jomardee A Perkins
![Propuesta de Proyecto de Inteligencia Artificial](https://writelatex.s3.amazonaws.com/published_ver/2824.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=07ba7688a14d046017a6ab9649ea8a6b2e59912b09fdefb3fb4f0ec47018add8)
Propuesta de Proyecto de Inteligencia Artificial
juego de ajedrez
Mariana Paucar
![Señales y Sistemas](https://writelatex.s3.amazonaws.com/published_ver/2784.jpeg?X-Amz-Expires=14400&X-Amz-Date=20240702T112450Z&X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=AKIAWJBOALPNFPV7PVH5/20240702/us-east-1/s3/aws4_request&X-Amz-SignedHeaders=host&X-Amz-Signature=00d56500929fc0891244480d79c8726b3f91242a21126863d90bf6f81430cc45)
Señales y Sistemas
Señales y Sistemas
Raymar Ortega