Image courtesy Amber Harmon.

Computing pioneer, renowned computer scientist, and former CACR Director Paul Messina has been presented with the distinguished Thomas Hart Benton Mural Medallion at Indiana University. “Paul Messina, Indiana University salutes you. Throughout your distinguished career, your work helped lay the foundation for grid and cloud computing, and helped bring parallel computing technology to the forefront of scientific computing,” said IU President Michael McRobbie.

“Paul established the effective use of high-performance computing at Caltech, and was instrumental in showing the broader research community its potential for advancing science at the national scale. His legacy lives on at CACR to this day, for which we are grateful, and we salute his accomplishments” said Mark Stalzer, CACR’s current director.

(Read more at http://www.isgtw.org/spotlight/computing-pioneer-honored-big-red-ii-dedication)

The central disk of our Milky Way galaxy with the Gemini stellar stream highlighted in the top right of the image. Credit: Andrew Drake/Axel Mellinger

A stream of at least 150 ancient variable stars has been confirmed to extend some 130,000 light years beyond our own galaxy’s stellar halo — on the fringes of the Intergalactic Medium, where aside from hot gas and dark matter, space-time becomes as sparse as the deep Sahara. The confirmation, based on analysis of 10 billion year-old dying RR Lyrae stars in the Gemini constellation, was done by an international team of astronomers, including CACR scientist Andrew Drake, who report their findings in The Astrophysical Journal.

(Read the full story)

Andrew Drake, CACR

We have performed an extensive search for RR Lyrae among the 500 million sources observed by the Catalina Surveys. We detect ~26,000 type-AB RR Lyrae (of which 20,000 are new discoveries) from a region spanning 3/4 of the sky. By determining accurate distances to the stars, we investigate the spatial distribution of structures within the Milky Way halo. Combining the RR Lyrae distances with SDSS spectroscopy we are able accurately trace the velocities and metallicities of hundreds of sources within the Sagittarius tidal streams system. We find the first strong evidence for a dense tidal stream that overlaps the Sagittarius system to distances beyond 100kpc, yet remains unexplained by any existing model.

Map covering around 29.4 by 24 degrees on the sky, indicating the huge scale of the newly discovered structure. Credit: R. G. Clowes / UCLan

An international team of astronomers, led by academics from the University of Central Lancashire and including CACR Senior Computational Scientist Matthew Graham, has found the largest known structure in the universe. The large quasar group (LQG) is so large that it would take a vehicle travelling at the speed of light some 4 billion years to cross it. The team published their results in the journal Monthly Notices of the Royal Astronomical Society…(more)

“General purpose GPU programming by CUDA—an introductory tutorial”
Dr. Hailiang Zhang, Caltech Center for Advanced Computing Research (CACR)

Abstract:
In recent years, various fields of large-scale scientific computations
have greatly benefit from the massively parallel programming.  This talk
presents a brief introduction and tutorial on the state-of-the-art
general-purpose GPU programming platform—CUDA.  The GPU device
architecture, memory hierarchy, and the general CUDA programming model
will be introduced.  The CUDA numerical schemes of some vector and matrix
operations will be demonstrated as examples.  Some CUDA applications on
molecular and biophysical modeling will be presented.  The standard CUDA
toolkit libraries and some third party APIs will also be introduced.

“Software Challenges for Extreme Scale Systems”
Vivek Sarkar, E.D. Butcher Chair in Engineering, Professor of Computer Science, Rice University

ABSTRACT:

It is widely recognized that  computer systems anticipated in the
2020 timeframe will be qualitatively different from current
and past computer systems.  Specifically, they will be built using
homogeneous and heterogeneous many-core processors with 100’s of
cores per chip, their performance will be driven by parallelism
(million-way parallelism just for a departmental server), and
constrained by energy and data movement.  They will also be subject to
frequent faults and failures.  Unlike previous generations of hardware
evolution, these Extreme Scale systems will have a profound impact on
future software.  The software challenges are further compounded by
the need to support new workloads and application domains
that have traditionally not had to worry about large scales of
parallelism in the past.

The challenges across the entire software stack for Extreme Scale
systems are driven by programmability and performance requirements,
and impose new requirements on programming models, languages, compilers, and runtime systems.
We focus on the critical role played by the runtime
system in enabling programmability in upper layers of the software
stack that interface with the programmer, and in enabling performance
in lower levels of the software stack that interface with the
hardware.  Examples of key runtime primitives will be drawn from early
experiences in the Habanero Multicore Software Research project
(http://habanero.rice.edu) which targets a wide range of homogeneous
and heterogeneous manycore processors.  On the programmability front,
the runtime primitives are shown to support important semantic guarantees
for different classes of programs.  On the performance front, we show how general structures for
task creation, synchronization, and termination can be implemented in a scalable manner
on manycore processor testbeds that are representative of the challenges
that we will face in future Extreme Scale processors.

BIO:

Vivek Sarkar conducts research in multiple aspects of parallel
software including programming languages, program analysis, compiler
optimizations and runtimes for parallel and high performance computer
systems.  He currently leads the Habanero Multicore Software Research
project at Rice University, and serves as Associate Director of the
NSF Expeditions project on the Center for Domain-Specific Computing.
Prior to joining Rice in July 2007, Vivek was Senior Manager of
Programming Technologies at IBM Research.  His responsibilities at IBM
included leading IBM’s research efforts in programming model, tools,
and productivity in the PERCS project during 2002- 2007 as part of the
DARPA High Productivity Computing System program.  His past projects
include the X10 programming language, the Jikes Research Virtual
Machine for the Java language, the MIT RAW multicore project, the ASTI
optimizer used in IBM’s XL Fortran product compilers, the PTRAN
automatic parallelization system, and profile-directed partitioning
and scheduling of Sisal programs.  Vivek holds a B.Tech. degree from
the Indian Institute of Technology, Kanpur, an M.S. degree from
University of Wisconsin-Madison, and a Ph.D. from Stanford University.
He became a member of the IBM Academy of Technology in 1995, the
E.D. Butcher Chair in Engineering at Rice University in 2007, and was
inducted as an ACM Fellow in 2008.  Vivek has been serving as a member
of the US Department of Energy’s Advanced Scientific Computing
Advisory Committee (ASCAC) since 2009.

Four undergrads have spent the summer developing and refining the prototypes as part of the cell-phone medicine project, headed by Julian Bunn of the Center for Advanced Computing Research (CACR) and Mani Chandy, Simon Ramo Professor and professor of computer science at Caltech. The lofty long-term goal of the project?  To make the “10-cent medical checkup” a reality.

( … read more at http://features.caltech.edu/features/210 )

The night sky is filled with objects like asteroids that dash across the sky and others—like exploding stars and variable stars-that flash, dim, and brighten. Studying such phenomena can help astronomers better understand the evolution of stars, massive black holes in the centers of galaxies, and the structure of the Milky Way. These types of objects were also essential for the recent discovery of dark energy-the mysterious energy that dominates the expansion of the universe—which earned last year’s Nobel Prize.

Using the Catalina Real-Time Transient Survey (CRTS), a project led by Caltech and including CACR staff Andrew Drake and Matthew Graham, the astronomers systematically scanned the heavens for these dynamic objects, producing an unprecedented data set that will allow scientists worldwide to pursue new research.

Read the full Caltech press release here.