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The University of California High Performance AstroComputing Center | Home

The Formation of Population III Binaries from Cosmological Initial Conditions. Simulation by Matthew Turk, Tom Abel, and Brian O'Shea. Image by Ralf Kaehler. Still from a simulation depicting an early stage of a gamma-ray burst. Collaborators: Stan Woosley (UCSC) and Weiqun Zhang (Stanford University). Simulated Observations" generated using the Sunrise code. Image credit: Chris Moody. BigBolshoi Cosmological Simulation. Image Credit: Stefan Gottloeber (AIP). Letter from the Director. A no-cost extension...

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The University of California High Performance AstroComputing Center | Home | hipacc.ucsc.edu Reviews

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The Formation of Population III Binaries from Cosmological Initial Conditions. Simulation by Matthew Turk, Tom Abel, and Brian O'Shea. Image by Ralf Kaehler. Still from a simulation depicting an early stage of a gamma-ray burst. Collaborators: Stan Woosley (UCSC) and Weiqun Zhang (Stanford University). Simulated Observations generated using the Sunrise code. Image credit: Chris Moody. BigBolshoi Cosmological Simulation. Image Credit: Stefan Gottloeber (AIP). Letter from the Director. A no-cost extension...

<META> KEYWORDS

1 about the center

2 mission and goals

3 consortium and leadership

4 hipacc affiliates

5 projects and collaborations

6 annual reports

7 conferences

8 summer school

9 annual summer school

10 news from uc hipacc

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about the center,mission and goals,consortium and leadership,hipacc affiliates,projects and collaborations,annual reports,conferences,summer school,annual summer school,news from uc hipacc,edu/outreach press room,hipacc e/po,apply for funding,support us

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The University of California High Performance AstroComputing Center | Home | hipacc.ucsc.edu Reviews

https://hipacc.ucsc.edu

The Formation of Population III Binaries from Cosmological Initial Conditions. Simulation by Matthew Turk, Tom Abel, and Brian O'Shea. Image by Ralf Kaehler. Still from a simulation depicting an early stage of a gamma-ray burst. Collaborators: Stan Woosley (UCSC) and Weiqun Zhang (Stanford University). Simulated Observations" generated using the Sunrise code. Image credit: Chris Moody. BigBolshoi Cosmological Simulation. Image Credit: Stefan Gottloeber (AIP). Letter from the Director. A no-cost extension...

INTERNAL PAGES

hipacc.ucsc.edu

1

The University of California High Performance AstroComputing Center | Annual Reports

http://hipacc.ucsc.edu/AnnualReports.html

Letter from the Director. Directions to the center. Media, Education, Outreach. Comp Astron. Press Room. Data Science Press Room. Letter from the Director. Directions to the center. UC-HiPACC—Five Year Report: 2010 2014/5. UC-HiPACC—The First Four-Plus Years: 2010–2014. UC-HiPACC The First Three Years: 2010 2012. 337 Natural Sciences 2 Building (NS2) Santa Cruz, CA 95064 (831) 459-1531 hipacc@ucsc.edu Administrator Login.

2

The University of California High Performance AstroComputing Center | UC Funding Discontinued for the University of California High-Performance AstroComputing Center (UC-HiPACC)

http://hipacc.ucsc.edu/PressRelease/UC-HiPACC-Closing-Release.html

Letter from the Director. Directions to the center. Media, Education, Outreach. Comp Astron. Press Room. Data Science Press Room. December 19, 2014 * FOR IMMEDIATE RELEASE*. View this as a PDF. View this as DOCX. December 19, 2014. University of California High-Performance AstroComputing Center (UC-HiPACC). Alternative Sources of Funding Sought. Funding has not been renewed for 2015 and beyond for the five-year-old University of California High-Performance AstroComputing Center (UC-HiPACC). UC-HiPACC...

3

The University of California High Performance AstroComputing Center | ISSAC

http://hipacc.ucsc.edu/SummerSchool.html

Letter from the Director. Directions to the center. Media, Education, Outreach. Comp Astron. Press Room. Data Science Press Room. The International Summer School on AstroComputing. International Summer School on AstroComputing: Class of 2013. Image credit: Trudy E. Bell. 337 Natural Sciences 2 Building (NS2) Santa Cruz, CA 95064 (831) 459-1531 hipacc@ucsc.edu Administrator Login.

4

Bolshoi Simulation | Home

http://hipacc.ucsc.edu/Bolshoi

Merger Trees and Catalogs. The CosmoSim database provides results from cosmological simulations performed within different projects: the MultiDark project, the BolshoiP project, and the CLUES project. The Adaptive Refinement Tree code used to run the Bolshoi simulation and its variant. The MultiDark Database, hosted by Potsdam Astrophysics Institute in Germany, contains the Bolshoi simulation as well as its two vairants, BigBolshoi and miniBolshoi. Introduction: The Bolshoi Simulation. The Bolshoi simula...

5

Future of AstroComputing | The University of California High-Performance AstroComputing Center (UC-HIPACC)

http://hipacc.ucsc.edu/FOA2010.html

The Future of AstroComputing Conference: Home. Registration deadline: Please register as soon as possible to insure that proper accomodations are made. Conference dates: Thurs, Dec 16 and Fri, Dec 17. Download the official conference flyer. 2010 Future of AstroComputing conference attendees. 831)459-1531 website maintained by nina@hipacc.ucsc.edu.

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trudyebell.com

Trudy E. Bell, M.A. - Home

http://www.trudyebell.com/home.php

Trudy E. Bell, M.A. Articles - Astronomy, History, Environment. 1913 Flood - Articles and Research. Reports, Brochures, Outreach. Craig B. Waff, Ph.D., 1946-2012. This site is a bit like a business card - a brief introduction, with just a sampling of my writings and photography, primarily recent work. I invite you to contact me for details, a formal resume, or additional clips. 19th-century U.S. observatories and telescopes. Great Easter 1913 flood. Previously, I was an editor for. And senior editor for.

ucolick.org

UC Astronomy and Astrophysics

http://www.ucolick.org/ucedu.html

Astronomy and Astrophysics at UC. Friends of Lick Observatory. UC Astronomy and Astrophysics. Department of Astronomy and Astrophysics. Friday Lunchtime Astrophysical Seminar. Physics Department Colloquia and Seminars. Center for Adaptive Optics. Laboratory for Adaptive Optics. Santa Cruz Institute for Particle Physics. Institute for Geophysics and Planetary Physics. Center for the Origin, Dynamics, and Evolution of Planets. UC High-Performance AstroComputing Center. Lawrence Berkeley National Laboratory.

cge.uci.edu

Southern California Center for Galaxy Evolution

http://www.cge.uci.edu/news.html

The Near-Field Deep-Field Connection (February 2014). The CGE and HiPACC. Hosted a meeting on the connection between the local and distant Universe from February 12 to 14, 2014 in Irvine, CA. PDF copies of each presentation can be found on the meeting website. Discovery of Puniest Galaxy On Record (June 2013). CGE Fellow Evan Kirby. Finds the puniest galaxy on record. Read more about the discovery here. Baryon Cycle Conference (June 2012). The CGE and HiPACC.

sites.google.com

The AGORA High-resolution Galaxy Simulations Comparison

https://sites.google.com/site/santacruzcomparisonproject

The AGORA High-resolution Galaxy Simulations Comparison. 5th AGORA Workshop in 2016. 4th AGORA Workshop in 2015. 3rd AGORA Workshop in 2014. 2nd AGORA Workshop in 2013. 1st AGORA Workshop in 2012. Santa Cruz Galaxy Workshop 2016. The project launch on 08/17/2012. Welcome to Project AGORA! We investigate galaxy formation with high-resolution simulations and compare the results across code platforms and with observations. First Workshop and the working groups formed, please visit. 5th annual summer Workshop.

dawsonresearch.com

Will Dawson - Blog

http://www.dawsonresearch.com/blog.html

Keck Observing Run Sep. 4 2013. Dave Wittman and I are currently at the UC Berkeley remote observation room (pictured) on the Merging Cluster Collaboration's third Keck DEIMOS observing run. The previous two runs returned about 2000 galaxy spectra of our merging cluster sample, and this run will produce about another 1000. We are using these spectra to gain insight into the dynamical history of the mergers as well as quantify their observed configurations (using the method I developed. To establish a UC ...

snsc.org

UC Astronomy and Astrophysics

http://www.snsc.org/ucedu.html

Astronomy and Astrophysics at UC. Friends of Lick Observatory. UC Astronomy and Astrophysics. Department of Astronomy and Astrophysics. Friday Lunchtime Astrophysical Seminar. Physics Department Colloquia and Seminars. Center for Adaptive Optics. Laboratory for Adaptive Optics. Santa Cruz Institute for Particle Physics. Institute for Geophysics and Planetary Physics. Center for the Origin, Dynamics, and Evolution of Planets. UC High-Performance AstroComputing Center. Lawrence Berkeley National Laboratory.

cge.uci.edu

Southern California Center for Galaxy Evolution

http://www.cge.uci.edu/meetings.html

The CGE and HiPACC. Will be hosting a meeting on the Near Field–Deep Field Connection. On February 12–14, 2014 in Irvine, CA. Registration. The CGE and HiPACC. Hosted a meeting on the Baryon Cycle. From June 14–16, 2012 in Irvine, CA. The inaugural CGE meeting. Took place on March 1–2, 2011 at the Beckman Center of the National Academies near UC Irvine, with over 140 scientists from Southern California in attendance. August 19-20, 2013 at UCSB).

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HiPAC: high performance packet classification. See also our project page at:. Nf-HiPAC is a full featured packet filter for Linux which demonstrates the power and flexibility of HiPAC. HiPAC is a novel framework for packet classification which uses an advanced algorithm to reduce the number of memory lookups per packet. It is ideal for environments involving large rulesets and/or high bandwidth networks. Nf-HiPAC provides the same rich feature set as iptables ( http:/ www.iptables.org. The performance of...

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Hipaca Cargas S.A.

NEWSLETTER (ingrese su email). Lavalle 1718 1ºD (1048) Bs.As. Rep.Argentina. Phone: 54 011 4372-2697 / 4478. Fax: 54 011 4375-5190.

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HIPAcc

The Heterogeneous Image Processing Acceleration Framework. Allows to design image processing kernels and algorithms in a domain-specific language (DSL). From this high-level description, low-level target code for GPU accelerators is generated using source-to-source translation. As back ends, the framework supports C/C , CUDA, OpenCL, and Renderscript. There is also a fork of HIPA. That targets Vivado HLS. Class LinearFilter : public Kernel uchar4 { private: Accessor uchar4 &input; Mask float &mask; publi...

hipacc.ucsc.edu

The University of California High Performance AstroComputing Center | Home

The Formation of Population III Binaries from Cosmological Initial Conditions. Simulation by Matthew Turk, Tom Abel, and Brian O'Shea. Image by Ralf Kaehler. Still from a simulation depicting an early stage of a gamma-ray burst. Collaborators: Stan Woosley (UCSC) and Weiqun Zhang (Stanford University). Simulated Observations" generated using the Sunrise code. Image credit: Chris Moody. BigBolshoi Cosmological Simulation. Image Credit: Stefan Gottloeber (AIP). Letter from the Director. A no-cost extension...

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HIP Accounting

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hipace-test.washburn.edu

HiPACE - Washburn University

HiPACE is a high-performance computing system operated and adminstered by faculty and students primarily in the Natural Sciences Division of Washburn University. The mission of HiPACE is to enrich and enliven the science and technology education of all Washburn students and to enhance the capabilities of faculty, staff and members of the community through technology. HiPACE was generously funded by Washburn University's Innovation Grant from 2006 to 2009. The HiPACE system consists of three basic parts:.

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Hassle-free Home Information Pack (HIP) and Energy Performance Certificate EPC in the North West London Area

The requirement to provide Home Information Pack (HIP) has now been suspended. However, all of the HIP documents are still needed to complete a property sale transaction. These will now be obtained by the buyer of a property rather than being provided by the seller. So how does this affect you? We are local and more responsive to your needs. You do not need to put up with poor service levels and turnaround time. Just test our claims and you will notice the difference straight away.