Update

_research/05-code-comparison.md

@@ -36,16 +36,39 @@ Further details on the structure and contents of submission data can be found in
 
 ### Preliminary Figures
 
-![A grid of dust density snapshots at various simulation times from different Lagrangian-dust codes for Problem BA with an average of one particle per gas grid cell at 512x512 resolution.](/assets/images/research/code-comparison/si/BA-np1-512.png)
+#### Lagrangian dust particles
+
+![A grid of dust density snapshots at various simulation times from different Lagrangian-dust codes for Problem BA with an average of one particle per gas grid cell at 512x512 resolution.](/assets/images/research/code-comparison/si/BA-np1-512_snapshots.png)
 A series of snapshots of the dust density field from various Lagrangian-dust codes for Problem BA with an average of one particle per gas cell, i.e. $$n_\mathrm{p} = 1$$, at a grid resolution of $$512 \times 512$$ (see Section 2.2.1 of the [Problem Set](#problem-set)).
 Increasing from top to bottom, each row corresponds to the simulation time $$t_\mathrm{sim}$$ in units of the local orbital period $$T$$, as labeled along the left margin.
 In alphabetical order from left to right, each column corresponds to a different code, as labeled along the top row of snapshots.
 The color-bar scale in the bottom right indicates the dust density $$\rho_\mathrm{p}$$ in units of the initially uniform gas density $$\rho_\mathrm{g,0}$$.
 Radial $$x$$ and vertical $$z$$ coordinates are in units of the vertical gas scale height $$H_\mathrm{g}$$.
 
-![A grid of dust density snapshots at various simulation times from different fluid-dust codes for Problem BA with an average of one particle per gas grid cell at 512x512 resolution.](/assets/images/research/code-comparison/si/BA-fluid-512.png)
+![TO DO](/assets/images/research/code-comparison/si/BA-np1-512_time_series.png)
+Maximum dust density as a function of time for codes implementing Lagrangian particles.
+Line colours represent different codes.
+Densities are normalised to the initially uniform gas density $$\rho_\mathrm{g,0}$$.
+
+![TO DO](/assets/images/research/code-comparison/si/BA-np1-512_CDF.png)
+Time-averaged cumulative distribution functions for the dust density for codes implementing Lagrangian particles.
+Solid lines represent the time-averaged densities, shaded areas represent the $$1\sigma$$ time variability, and different colours represent different codes.
+
+
+#### Pressureless dust fluid
+
+![A grid of dust density snapshots at various simulation times from different fluid-dust codes for Problem BA with an average of one particle per gas grid cell at 512x512 resolution.](/assets/images/research/code-comparison/si/BA-fluid-512_snapshots.png)
 A series of snapshots of the dust density field from various fluid-dust codes for Problem BA at a grid resolution of $$512 \times 512$$ (see Section 2.2.1 of the [Problem Set](#problem-set)).
 Increasing from top to bottom, each row corresponds to the simulation time $$t_\mathrm{sim}$$ in units of the local orbital period $$T$$, as labeled along the left margin.
 In alphabetical order from left to right, each column corresponds to a different code, as labeled along the top row of snapshots.
 The color-bar scale in the bottom right indicates the dust density $$\rho_\mathrm{p}$$ in units of the initially uniform gas density $$\rho_\mathrm{g,0}$$.
 Radial $$x$$ and vertical $$z$$ coordinates are in units of the vertical gas scale height $$H_\mathrm{g}$$.
+
+![FINISH.](/assets/images/research/code-comparison/si/BA--512_time_series.png)
+Maximum dust density as a function of time for codes implementing a pressureless fluid.
+Line colours represent different codes.
+Densities are normalised to the initially uniform gas density $$\rho_\mathrm{g,0}$$.
+
+![TO DO](/assets/images/research/code-comparison/si/BA--512_CDF.png)
+Time-averaged cumulative distribution functions for the dust density for codes implementing Lagrangian particles.
+Solid lines represent the time-averaged densities, shaded areas represent the $$1\sigma$$ time variability, and different colours represent different codes.

_team/unlv-20-baronett-stanley.md

@@ -18,24 +18,26 @@ sidebar:
     <a href='https://orcid.org/0000-0003-0412-760X' target='_blank'><i class='fab fa-fw fa-orcid'></i>ORCiD</a>"
   - title: "Research Interests"
     text: "<ul>
+    <li> <a href='/research/#software-development'>Computational astrophysics</a>
     <li> <a href='https://github.com/PrincetonUniversity/athena/wiki/Non-relativistic-Radiation-Transport' target='_blank'>Radiation hydrodynamics</a>
     <li> <a href='https://ui.adsabs.harvard.edu/abs/2024MNRAS.529..275B/abstract' target='_blank'>Streaming instability</a>
-    <li> <a href='/research/planet-formation/#dust-gas-dynamics-and-planetesimal-formation'>Planetesimal formation</a>
-     <li> <a href='/research/#software-development'>Computational astrophysics</a>"
+    <li> <a href='/research/planet-formation/#dust-gas-dynamics-and-planetesimal-formation'>Planetesimal formation</a>"
 ---
-Stanley A. Baronett is a UNLV Foundation Board of Trustees Fellow in the <a href='https://www.physics.unlv.edu/' target='_blank'>Department of Physics and Astronomy</a> at the University of Nevada, Las Vegas (<a href='https://www.unlv.edu/' target='_blank'>UNLV</a>) and works with Ph.D. advisor <a href='https://www.physics.unlv.edu/~zhzhu/Home.html' target='_blank'>Zhaohuan Zhu</a>.
-In collaboration with <a href='https://www.simonsfoundation.org/people/yan-fei-jiang/' target='_blank'>Yan-Fei Jiang</a> (Center for Computational Astrophysics, <a href='https://www.simonsfoundation.org/flatiron/center-for-computational-astrophysics/' target='_blank'>CCA</a>) and <a href='https://www.simonsfoundation.org/people/phil-armitage/' target='_blank'>Phil Armitage</a> (<a href='https://www.astro.sunysb.edu/' target='_blank'>Stony Brook University</a>), he uses the <a href='https://github.com/PrincetonUniversity/athena/wiki/Non-relativistic-Radiation-Transport' target='_blank'>non-relativistic radiation transport module</a> for [Athena++](/research/#software-development) to study the effect of multifrequency dust opacities on the [thermodynamic structure of protoplanetary disks](/research/protoplanetary-disks/#accretion-and-structure).
-In collaboration with <a href='https://physics.ua.edu/people/chao-chin-yang/' target='_blank'>Chao-Chin Yang</a> (<a href='https://physics.ua.edu/' target='_blank'>University of Alabama</a>), he uses a particle–mesh module for [Athena++](/research/#software-development) to study [planetesimal formation](/research/planet-formation/#dust-gas-dynamics-and-planetesimal-formation) and <a href='https://ui.adsabs.harvard.edu/abs/2024MNRAS.529..275B/abstract' target='_blank'>dust–gas dynamics driven by the streaming instability with various pressure gradients</a>.
-In collaboration with <a href='https://www.hmc.edu/physics/faculty-staff/tamayo/' target='_blank'>Daniel Tamayo</a> (<a href='https://www.hmc.edu/physics/' target='_blank'>Harvey Mudd College</a>) and <a href='https://www.jasonhsteffen.com/' target='_blank'>Jason H. Steffen</a> (<a href='https://www.unlv.edu/' target='_blank'>UNLV</a>), he contributes to the N-body code <a href='https://reboundx.readthedocs.io/' target='_blank'>REBOUNDx</a> to study the effects of post-main sequence <a href='https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.6001B/abstract' target='_blank'>stellar evolution and tidal dissipation</a> on planetary dynamics.
+Stanley A. Baronett is a UNLV Foundation Board of Trustees Fellow in the <a href='https://www.physics.unlv.edu/' target='_blank'>Department of Physics and Astronomy</a> at the University of Nevada, Las Vegas (<a href='https://www.unlv.edu/' target='_blank'>UNLV</a>), and works with Ph.D. advisor <a href='https://unlv-spfg.github.io/team/zhu-zhaohuan/' target='_blank'>Zhaohuan Zhu</a>.
+As a <a href='https://www.simonsfoundation.org/people/stanley-a-baronett/' target='_blank'>Pre-Doctoral Research Analyst</a> at the Center for Computational Astrophysics (<a href='https://www.simonsfoundation.org/flatiron/center-for-computational-astrophysics/' target='_blank'>CCA</a>), he began collaborating with <a href='https://www.simonsfoundation.org/people/yan-fei-jiang/' target='_blank'>Yan-Fei Jiang</a> (<a href='https://www.simonsfoundation.org/flatiron/center-for-computational-astrophysics/' target='_blank'>CCA</a>) and <a href='https://www.simonsfoundation.org/people/phil-armitage/' target='_blank'>Phil Armitage</a> (<a href='https://www.simonsfoundation.org/flatiron/center-for-computational-astrophysics/' target='_blank'>CCA</a>/<a href='https://www.astro.sunysb.edu/' target='_blank'>Stony Brook University</a>) to use and help contribute to the <a href='https://github.com/PrincetonUniversity/athena/wiki/Non-relativistic-Radiation-Transport' target='_blank'>non-relativistic radiation transport module</a> for [Athena++](/research/#software-development) to study the effect of multifrequency dust opacities on the [thermodynamic structure of protoplanetary disks](/research/protoplanetary-disks/#thermodynamic-structure).
+As a <a href='https://nasa.epscorspo.nevada.edu/funding/2021-2022-nvsgc-fellowship/'>Nevada NASA Space Grant Consortium Graduate Research Fellow</a>, he began collaborating with <a href='https://physics.ua.edu/people/chao-chin-yang/' target='_blank'>Chao-Chin Yang</a> (<a href='https://physics.ua.edu/' target='_blank'>University of Alabama</a>) to use a particle–mesh module for [Athena++](/research/#software-development) to study [planetesimal formation](/research/planet-formation/#planetesimal-formation) and <a href='https://ui.adsabs.harvard.edu/abs/2024MNRAS.529..275B/abstract' target='_blank'>dust–gas dynamics driven by the streaming instability with various pressure gradients</a>.
+In collaboration with <a href='https://www.hmc.edu/physics/faculty-staff/tamayo/' target='_blank'>Daniel Tamayo</a> (<a href='https://www.hmc.edu/physics/' target='_blank'>Harvey Mudd College</a>) and <a href='https://www.jasonhsteffen.com/' target='_blank'>Jason H. Steffen</a> (<a href='https://www.unlv.edu/' target='_blank'>UNLV</a>), he contributes to [REBOUNDx](/research/#software-development) to study the effects of post-main sequence <a href='https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.6001B/abstract' target='_blank'>stellar evolution and tidal dissipation on planetary dynamics</a>.
+Prior to pursuing an academic career in astrophysics, he earned a <a href='https://hawaii.edu/phil/undergraduate/major-requirements/' target='_blank'>B.A.</a> and <a href='https://hawaii.edu/phil/graduate/ma-requirements/' target='_blank'>M.A. in Philosophy</a> at the University of Hawaiʻi at Mānoa (<a href='https://manoa.hawaii.edu/' target='_blank'>UHM</a>) and worked in information technology (IT) for nearly a decade.
 
 
 ## Timeline
-- __2022—present__: <a href='https://www.unlv.edu/degree/phd-astronomy' target='_blank'>Ph.D. Astronomy</a>, <a href='https://www.unlv.edu/' target='_blank'>UNLV</a>
+- __2022—present__: <a href='https://www.unlv.edu/degree/phd-astronomy' target='_blank'>Ph.D. in Astronomy</a>, <a href='https://www.unlv.edu/' target='_blank'>UNLV</a>
 - __2024—2026__: <a href='https://www.unlv.edu/' target='_blank'>UNLV</a> Foundation Board of Trustees Fellow
-- __2023—2024__: <a href='https://www.simonsfoundation.org/flatiron-institute-center-for-computational-astrophysics-pre-doctoral-program' target='_blank'>Pre-Doctoral Research Fellow</a>, <a href='https://www.simonsfoundation.org/flatiron/center-for-computational-astrophysics/' target='_blank'>CCA</a>
-- __2020—2022__: <a href='https://www.unlv.edu/degree/ms-astronomy' target='_blank'>M.S. Astronomy</a>, <a href='https://www.unlv.edu/' target='_blank'>UNLV</a>
-- __2018—2020__: <a href='https://www.unlv.edu/degree/bs-physics' target='_blank'>B.S. Computational Physics</a>, <a href='https://www.unlv.edu/' target='_blank'>UNLV</a>
+- __2023—2024__: <a href='https://www.simonsfoundation.org/people/stanley-a-baronett/' target='_blank'>Pre-Doctoral Research Analyst</a>, <a href='https://www.simonsfoundation.org/flatiron/center-for-computational-astrophysics/' target='_blank'>CCA</a>
+- __2020—2022__: <a href='https://www.unlv.edu/degree/ms-astronomy' target='_blank'>M.S. in Astronomy</a>, <a href='https://www.unlv.edu/' target='_blank'>UNLV</a>
+- __2021—2022__: <a href='https://nasa.epscorspo.nevada.edu/funding/2021-2022-nvsgc-fellowship/'>Nevada Space Grant Consortium Graduate Fellow</a> (<a href='https://www.unlv.edu/' target='_blank'>UNLV</a>)
+- __2018—2020__: <a href='https://www.unlv.edu/degree/bs-physics' target='_blank'>B.S. in Computational Physics</a>, <a href='https://www.unlv.edu/' target='_blank'>UNLV</a>
 - __2016—2018__: IT Consultant, <a href='https://www.qdigital.com/' target='_blank'>Qdigital Technology Services</a>
 - __2009—2016__: IT Specialist, <a href='https://www.hnei.hawaii.edu/' target='_blank'>Hawaiʻi Natural Energy Institute</a>
-- __2013—2015__: <a href='https://hawaii.edu/phil/graduate/ma-requirements/' target='_blank'>M.A. Philosophy</a>, <a href='https://manoa.hawaii.edu/' target='_blank'>University of Hawaiʻi at Mānoa</a>
-- __2007—2012__: <a href='https://hawaii.edu/phil/undergraduate/major-requirements/' target='_blank'>B.A. Philosophy</a>, <a href='https://manoa.hawaii.edu/' target='_blank'>University of Hawaiʻi at Mānoa</a>
+- __2013—2015__: <a href='https://hawaii.edu/phil/graduate/ma-requirements/' target='_blank'>M.A. in Philosophy</a>, <a href='https://manoa.hawaii.edu/' target='_blank'>UHM</a>
+- __2007—2012__: <a href='https://hawaii.edu/phil/undergraduate/major-requirements/' target='_blank'>B.A. in Philosophy</a>, <a href='https://manoa.hawaii.edu/' target='_blank'>UHM</a>