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FIRE: Feedback In Realistic Environments | Increasing the predictive power of galaxy formation simulations

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. Above: The large-scale gas distribution (left), face-on star light (middle), and edge-on star light (right) in a FIRE cosmological simulation of a Milky Way-mass galaxy. FIRE in the Field: Simulating the Threshold of Galaxy Formation. The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations. Why do high-redshift galaxies show diverse gas-phase metallicity gradients?

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FIRE: Feedback In Realistic Environments | Increasing the predictive power of galaxy formation simulations | fire.northwestern.edu Reviews

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FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. Above: The large-scale gas distribution (left), face-on star light (middle), and edge-on star light (right) in a FIRE cosmological simulation of a Milky Way-mass galaxy. FIRE in the Field: Simulating the Threshold of Galaxy Formation. The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations. Why do high-redshift galaxies show diverse gas-phase metallicity gradients?

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FIRE: Feedback In Realistic Environments | Increasing the predictive power of galaxy formation simulations | fire.northwestern.edu Reviews

https://fire.northwestern.edu

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. Above: The large-scale gas distribution (left), face-on star light (middle), and edge-on star light (right) in a FIRE cosmological simulation of a Milky Way-mass galaxy. FIRE in the Field: Simulating the Threshold of Galaxy Formation. The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations. Why do high-redshift galaxies show diverse gas-phase metallicity gradients?

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MassiveFIRE | FIRE: Feedback In Realistic Environments

http://fire.northwestern.edu/massivefire

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. Above: A star forming galaxy at z 1.7 in the MassiveFIRE sample. Left: Stellar light in rest frame U, V, and J broad bands. Right: Gas density, temperature, and metallicity. Top panels show the stellar and gas disk of the galaxy in a face-on projection. The bottom panels show a zoomed-out view of the same galaxy. What is the structure and composition of the halo gas surrounding massive galaxies?

2

FIREBox | FIRE: Feedback In Realistic Environments

http://fire.northwestern.edu/firebox

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. FIREBox is a next-generation extension of FIRE which will simulate full cosmological volumes at the resolution of the FIRE zoom-in simulations. FIREBox will provide the galaxy statistics necessary to fully interpret galaxy surveys and will be ideally suited for studies of the intergalactic medium. Stay tuned! FIRE in the Field: Simulating the Threshold of Galaxy Formation. New Papers from FIRE.

3

New Papers from FIRE | FIRE: Feedback In Realistic Environments

http://fire.northwestern.edu/2016/04/18/new-papers-from-fire

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. New Papers from FIRE. April 18, 2016. August 5, 2016. The past several months have been highly productive for the FIRE project, with a large number of new papers submitted on a variety of science topics. Among others, the first paper from MassiveFIRE. By Feldmann et al. Van de Voort et al. On “Giant Clumps in the FIRE Simulations: a Case Study of a Massive High-Redshift Galaxy”. On “Breathing ...

4

When the Jeans don’t fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies | FIRE: Feedback In Realistic Environments

http://fire.northwestern.edu/2016/12/30/when-the-jeans-dont-fit-how-stellar-feedback-drives-stellar-kinematics-and-complicates-dynamical-modeling-in-low-mass-galaxies

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. When the Jeans don’t fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies. December 30, 2016. December 30, 2016. El-Badry et al., available on arXiv. Why do high-redshift galaxies show diverse gas-phase metallicity gradients? The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations. Latte Reconciles Dwarf Galaxies with LCDM.

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Data | FIRE: Feedback In Realistic Environments

http://fire.northwestern.edu/data

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. Following are links to FIRE products:. A public version of the GIZMO simulation code is available here. To generate initial conditions. MUSIC parameter files to generate ICs exactly matching the FIRE simulations are available here. For the Firefly interactive visualization app, see this link. HI CGM data in ASCII format from Hafen et al. 2016. Latte Reconciles Dwarf Galaxies with LCDM.

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Feedback-regulated star formation and the FIRE simulations | GalForm@NU

http://galaxies.northwestern.edu/2013/08/11/feedback-regulated-star-formation-in-galactic-discs-and-molecular-clouds

Faucher-Giguère galaxy formation group. Resources for students and pdocs. Feedback-regulated star formation and the FIRE simulations. August 11, 2013. August 12, 2014. Galaxies convert their gas into stars at a rate which is typically only a few percent of what unimpeded gravitational collapse would imply. Understanding why star formation is so slow in galaxies is a central problem in astrophysics. Equivalently, what is the origin of the Kennicutt-Schmidt law. Based on the small-scale properties of super...

galaxies.northwestern.edu

Daniel Angles-Alcazar will join GalForm@NU as a CIERA Postdoctoral Fellow | GalForm@NU

http://galaxies.northwestern.edu/2014/03/12/daniel-angles-alcazar-galformnu-as-a-ciera-postdoctoral-fellow

Faucher-Giguère galaxy formation group. Resources for students and pdocs. Daniel Angles-Alcazar will join GalForm@NU as a CIERA Postdoctoral Fellow. March 12, 2014. August 12, 2014. We are proud and thrilled to have recruited Daniel Angles-Alcazar to join our group as a CIERA Postdoctoral Fellow in fall 2014! View all posts by Claude-Andre Faucher-Giguere →. Research opportunities for undergraduates. Shyam Bharadwaj wins Illinois Space Grant. You may like these posts. CIERA hosts FIRE project workshop.

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GalForm @ NU group launch | GalForm@NU

http://galaxies.northwestern.edu/2013/09/22/group-launch

Faucher-Giguère galaxy formation group. Resources for students and pdocs. GalForm @ NU group launch. September 22, 2013. August 12, 2014. I am excited to join the Northwestern faculty, where I am starting a new effort in galaxy formation modeling! During the academic year 2013-2014, the Einstein Fellowship. Is allowing me to focus on research, after which I will officially become Assistant Professor of Physics & Astronomy at Northwestern. Research, and seminar series. CIERA hosts FIRE project workshop.

galaxies.northwestern.edu

Publications | GalForm@NU

http://galaxies.northwestern.edu/publications

Faucher-Giguère galaxy formation group. Resources for students and pdocs. Papers from our group. For a fully up-to-date list, see this ADS link. Hopkins, P. F., Torrey, P., Faucher-Giguere, C.-A., Quataert, E., & Murray, N., “Stellar and Quasar Feedback in Concert: Effects on AGN Accretion, Obscuration, and Outflows,” MNRAS, submitted [arXiv:1504.05209]. Onorbe, J., Boylan-Kolchin, M., Bullock, J. S., Hopkins, P. F., Keres, D., Faucher-Giguere, C.-A., Quataert, E.,...Muratov, A., Keres, D., Fauch...Fauch...

galaxies.northwestern.edu

UV Background | GalForm@NU

http://galaxies.northwestern.edu/uvb

Faucher-Giguère galaxy formation group. Resources for students and pdocs. The ionizing background, from the ultraviolet to the x-rays, is a fundamental ingredient to both theoretical and empirical studies of both the intergalactic medium and galaxy formation as it determines the ionization balance of light elements as well as the thermal history of cosmic gas through photoheating. HI photoionization rate vs. z and detailed UV background spectrum at z=3 in our fiducial model [1]. 8211; December 2011 update.

galaxies.northwestern.edu

Postdoctoral fellowship opportunities | GalForm@NU

http://galaxies.northwestern.edu/2013/09/22/postdoctoral-fellowship-opportunities

Faucher-Giguère galaxy formation group. Resources for students and pdocs. September 22, 2013. August 12, 2014. This year, CIERA is particularly interested in postdoctoral fellows working in the broad area of galaxy formation and evolution, including star formation, stellar feedback, black hole-galaxy co-evolution, and the connection with the intergalactic medium. We anticipate to make several offers. Apply here before Dec. 1, 2013! GalForm @ NU group launch. Research opportunities for undergraduates.

galaxies.northwestern.edu

CIERA hosts FIRE project workshop | GalForm@NU

http://galaxies.northwestern.edu/2014/08/12/ciera-hosts-fire-project-workshop

Faucher-Giguère galaxy formation group. Resources for students and pdocs. CIERA hosts FIRE project workshop. August 12, 2014. August 12, 2014. On July 24-26, CIERA hosted a workshop for the FIRE. Niharika Sravan wins first prize for poster presented at Northwestern Computational Research Day. Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history. Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history. CIERA hosts FIRE project workshop.

galaxies.northwestern.edu

Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history | GalForm@NU

http://galaxies.northwestern.edu/2014/09/14/neutral-hydrogen-in-galaxy-halos-at-the-peak-of-the-cosmic-star-formation-history

Faucher-Giguère galaxy formation group. Resources for students and pdocs. Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history. September 14, 2014. August 8, 2016. We have just completed the first paper from the FIRE project (Faucher-Giguère et al., available on the arXiv. CIERA hosts FIRE project workshop. Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history. CIERA hosts FIRE project workshop. Shyam Bharadwaj wins Illinois Space Grant.

galaxies.northwestern.edu

FIRE | GalForm@NU

http://galaxies.northwestern.edu/fire-simulations

Faucher-Giguère galaxy formation group. Resources for students and pdocs. Central to the galaxy formation modeling efforts at Northwestern is the FIRE project. FIRE (Feedback In Realistic Environments) is a project aiming to dramatically increase the predictive power of cosmological simulations of galaxy formation by. 1) Directly resolving the formation of giant molecular clouds (GMCs), the rate limiting for star formation in galactic disks, and. CIERA hosts FIRE project workshop. As a CIERA Postdoctoral...

galaxies.northwestern.edu

People | GalForm@NU

http://galaxies.northwestern.edu/people

Faucher-Giguère galaxy formation group. Resources for students and pdocs. Assistant Professor of Physics and Astronomy (2014-). Einstein Fellow, Northwestern University (2013-2014). Miller Research Fellow, UC Berkeley (2010-2013). PhD in Astronomy, Harvard University (2010). Am in Astronomy, Harvard University (2007). BSc in Mathematics and Physics, McGill University (2005). Tech F243 [email protected]. Tech F238 [email protected]. Project. Daniel is also leading a comprehensive study of the cosmic b...

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FIRE: Feedback In Realistic Environments | Increasing the predictive power of galaxy formation simulations

FIRE: Feedback In Realistic Environments. Increasing the predictive power of galaxy formation simulations. Above: The large-scale gas distribution (left), face-on star light (middle), and edge-on star light (right) in a FIRE cosmological simulation of a Milky Way-mass galaxy. FIRE in the Field: Simulating the Threshold of Galaxy Formation. The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations. Why do high-redshift galaxies show diverse gas-phase metallicity gradients?

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