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A list of all the posts and pages found on the site. For you robots out there is an XML version available for digesting as well.
Pages
Posts
publications
Paper Title Number 1
Published in Journal 1, 2009
This paper is about the number 1. The number 2 is left for future work.
Recommended citation: Your Name, You. (2009). "Paper Title Number 1." Journal 1. 1(1). http://academicpages.github.io/files/paper1.pdf
Paper Title Number 2
Published in Journal 1, 2010
This paper is about the number 2. The number 3 is left for future work.
Recommended citation: Your Name, You. (2010). "Paper Title Number 2." Journal 1. 1(2). http://academicpages.github.io/files/paper2.pdf
Paper Title Number 3
Published in Journal 1, 2015
This paper is about the number 3. The number 4 is left for future work.
Recommended citation: Your Name, You. (2015). "Paper Title Number 3." Journal 1. 1(3). http://academicpages.github.io/files/paper3.pdf
Paper Title Number 4
Published in GitHub Journal of Bugs, 2024
This paper is about fixing template issue #693.
Recommended citation: Your Name, You. (2024). "Paper Title Number 3." GitHub Journal of Bugs. 1(3). http://academicpages.github.io/files/paper3.pdf
research
talks
Conference Proceeding talk 3 on Relevant Topic in Your Field
Published:
This is a description of your conference proceedings talk, note the different field in type. You can put anything in this field.
Magnetic fields - Making life interesting
Published:
Abstract: In the vast cosmos, magnetic fields are seemingly omnipresent, influencing phenomena from the scale of interstellar dust grains to entire galaxies. Due to the inherent difficulties in studying and observing magnetic fields, they are often overlooked, but their presence and effects can lead to interesting consequences. Studying magnetic fields at cosmological distances is not easy; however, with the advent of methods like Rotation Measure (RM) synthesis, we have a way to probe magnetic fields at higher redshifts by utilizing the property of light known as Faraday rotation. In the first part of my talk, I will briefly explore the unknowns surrounding magnetic fields, their importance, and the challenges in studying them. In the second part of my talk, I will present broadband polarization observations made with the VLA from 1-3 GHz at 1” resolution. These observations are part of a comprehensive 106-hour survey targeting 201 radio quasars, of which 39 contain an intervening galaxy in their lines of sight. The goal is to use a statistical approach to estimate the RM of the intervening galaxies in the redshift range of 0.1 to 1. This dataset also includes a sub-sample of resolved quasars where we measured the RMs of the radio lobes. This sub-sample represents the first release of these observations, focusing on the fully resolved sources. I will present some of the results of the RMs of the radio lobes and also discuss our approach to understanding the evolution of the magnetic field with redshift in the context of galaxy evolution.