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Systems Distributed Sape Mullender Chapter 13 Notes - Dan Ellard Chapter 13 - Transaction-Processing Techniques William E. Weihl Overview: Distributed systems must tolerate failures, and distributed systems can require complex synchronization of concurrent processes. Both of these issues are interesting; together they are a headache. One approach to this combo is ATOMIC TRANSACTIONS. An atomic transaction *appears* to occur indivisibly (and can have several other useful properties wrt failures) and so they are relatively easy to reason about-- instead of worrying about concurrency, the programmer can treat these transactions as sequential operations even though several might be going on concurrently. 13.1 -- Problem Addressed Concurrency and synchronization - controlling access to shared data. Grouping operations into a single atomic operation. Operations within atomic transactions cannot appear as though they are interleaved. Failures - to tolerate failures, replicated servers can be used. In spite of failures, we want all replicas to reach the same state at the "end" of each transaction. It's all or nothing, everywhere-- either every replica completes the transaction, in the same manner, or all replicas decide to abandon the transaction. 13.2 -- What Are Transactions? This chapter deals almost exclusively with transactions defined in terms of the ACID properties. There are other properties, which might be useful in other situations, but ACID transactions are very easy to deal with. A - Atomic Each operation appears indivisible wrt crashes-- it occurs completely or not at all. "Partial effects" are invisible. COMMIT - a transactions that completed successfully ABORT - the transaction has failed and all evidence of its operations are erased. This property is also called RECOVERABILITY (because we can recover from aborted transactions-- they leave no damage behind). C - Consistent The transaction, when executed alone and committed, preserves some set of invariants which have been defined on the system state. (The outcome system state is consistent with a set of invariants.) I - Isolated (aka serializability or concurrency atomicity) Transactions are indivisible wrt each other. If a set of transactions are performed concurrently, the result is the same as if the same set of transactions had been performed in *some* order sequentially. (Often we also want to define what that order would be, in terms of real time or some other measure, but this is not necessary for isolation.) D - Durable (aka permanence) "The effects of committed transactions are very likely to survive subsequent failures." Of course, if the system catches on fire, or some other catastrophic event occurs, then some state might be lost. But barring some disaster, the system does not "lose" or "forget" the effect of a committed transaction. If we have a way to do ACID transactions, life is easy. We can have many concurrent transactions going on at the same time, and they won't get in each others hair, violate their invariants, or be forgotten later. (The rest of this section goes deeper into defining these terms, and gives a very precise if somewhat confusing specification for an ACID system.) 13.3 -- Concurrency Control This section begins discussing algorithms that can be used to implement the ACID spec. TWO-PHASE LOCKING - a common synchronization method. - Ensures that a transaction can always commit without violating serializability. Operates by locking the data so that: a. Operations of concurrent transactions commute. b. Operations reflect the results of all committed transactions. We can "serialize" the transactions by their commit order. The locks must be set up so that if two operations do not commute, they require conflicting locks and so one must block until the other is finished. The "two-phase" comes from the fact that all locks are acquired, and then all locks are released. No lock is acquired after any lock is released. As spec'd, there is a possibility of deadlock. This can be avoided by the usual means-- prevention, avoidance, or detection. The actual locking mechanism required might be simpler; it depends on the semantics required by the system. 13.4 -- Single-Site Recovery First, we consider recovery for a single site. Failure model: - Transaction abort: the operations need to be undone for some reason detected by the algorithm. - System crash: thud. Nonvolatile storage survives, but no other state. - Media failure: nonvolatile storage is lost, but the system continues to run. - Catastrophe: all storage (volatile and nonvolatile) is lost. There is no recovery from catastrophe. 13.4.1 -- Abort Recovery We assume that the transaction aborts, but no other failures occur. Our goal is to make it look as though the transaction never took place (as far as the state of the system is concerned). Two main approaches: Update-in-place: state is modified as the transaction proceeds, and if the transaction aborts, the changes are "undone". Deferred-update: state is not modified until the transaction is ready to commit, and then all updates are made at once. Update-in-place seems to have much better performance in general, particularly if operations are likely to commit. However, deferred-update can have some benefits in the area of concurrency. 13.4.2 -- Crash Recovery Updates might involve several physical reads and writes; how do we make them appear atomic, so that the state of the nonvolatile storage always is consistent (or at least contains a consistent view of the state)? The typical mechanism is a LOG. The log records which updates correspond to committed or aborted transactions. It is noted that reconstructing the state of the world when the crash took place from the log has subtleties. We can also use a log-like structure to batch writes. (this is the basic idea behind log-structured file systems). ARIES is described. This is an update-in-place system. All activity is recorded in the log. In the case of an abort, COMPENSATION RECORDS are recorded in the log to represent the "undoing" of a previous update in the log. The log is FORCED to disk whenever a commit occurs. This can be a bottleneck, so group commit can be used. The committed log entries form a REDO; since they can be replayed to simulate the "redo" of the actions and reconstruct the state. Note that the actual state is updated separately and does not reside in the log! Therefore, there is a possibility that the actual state (i.e. some file) may be updated, and then a crash occurs, so no mention of that update appears in the log. We could reverse the problem by making sure that the log entries are written before the actual updates, but that doesn't help. Instead, we require that redo log records and their corresponding undo records be recorded before the update can actually happen. This way, no matter what the state of the log and the file, we can find a consistent state to restart in. To recover-- 1. Replay all "redo" records. 2. Replay all "undo" records that belong to uncommitted transactions. But there's a catch: what if we crash in the middle of a recovery? How do we recover from *that*? The redo records must be idempotent, so we can replay them (in the same order) and get the same result. We can keep track of what log records have successfully been redone so we don't have to do them again and again. To keep the log (and the recovery process) from growing without bound, we can CHECKPOINT the system from time to time, effectively recording a snapshot of the system state at some point in the log, and then removing all prior entries in the log. 13.4.3 -- Recovery from Media Failure Reach for the backup tapes... and then redo the log from the last archive. There are problems with getting a good archive without stopping the system. This has been solved with current file systems, but most people aren't using "current" file systems... 13.4.4 -- Discussion We haven't discussed how to combine recovery with concurrency control. Now we must. The redo/undo records in the log must commute wrt operations in other transactions. Beware-- the undo doesn't generally commute with anything. We need to ensure that "the granularity of the locks is at least as large as the granularity of recovery." 13.5 -- Distributed Recovery And now, for distributed systems. We must make sure that all the sites (replicas) are in a consistent state. There must be agreement whether to commit or abort each operation (the ATOMIC COMMITMENT PROBLEM we saw earlier in the semester). Common approach: two-phase commit (or, as we saw before, three-phase commit in order to tolerate different kinds of faults). Note the use of INCARNATION NUMBERS-- the crash count. If during a commit protocol a process gets two different messages from the same process with different incarnation numbers, then the other process must have crashed; abort. 13.6 -- Other Concurrency Control Methods There are other concurrency control methods besides two-phase locking, and for some purposes these methods are better. One strategy worth mentioning is OPTIMISTIC; the idea is to do no locking at all until commit, and then check to see whether any concurrency restrictions would have been violated. If so, then abort and retry the transaction; otherwise proceed. If conflicts are unlikely, this is a win, but if conflicts are common this is a big lose. 13.7 -- Distributed Concurrency Control Sites must coordinate to make sure that the same concurrency control is applied everywhere. They must also agree on a serialization order for all transactions (or at least those that must be serialized). This is not a problem when everyone is running the same software. But when the system is heterogeneous, it's an unsolved headache. 13.8 -- Nested Transactions It may be desirable to structure transactions themselves in terms of pieces that can succeed or fail, and are serializable (and may run concurrently)-- the pieces are themselves transactions. These are called SUBTRANSACTIONS or NESTED TRANSACTIONS. In most ways they are similar to ordinary transactions, but there are differences: - The commit of the subtransactions does not actually take effect until the parent commits. If any subtransaction aborts, all are aborted and undone. - Subtransactions "inherit" locks: = The child won't block on a lock the parent holds. = The child cannot release a lock that the parent holds. They are useful because they allow high degrees of concurrency without extra locking and with only one actual commit/abort action. 13.9 -- Discussion More discussion of how atomic transactions are not the best solution for all problems. However, the stigma of slowness has been overcome by the newer algorithms that reduce or eliminate the need for synchronous I/O to nonvolatile storage. 13.10 -- Bibliographic and Historical Notes There's been a long history of work in this area, and many interesting or notable ideas. See references for more info...
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notes-chap05.txt
Path: Harvard >> CS >> 299 Fall, 2009
Description: Fault tolerant broadcasts and related problems Distributed Systems: Chapter 5 Geoff Wyant 11/24/93 updated 2/21/99 by Dan Ellard Overview - This chapter presents algorithms for broadcasting in distributed systems. Some of...
AaronMandel.txt
Path: Harvard >> CS >> 50 Fall, 2009
Description: From amandel@fas.harvard.edu Wed Nov 27 00:06:44 1996 Date: Wed, 27 Nov 1996 00:06:42 -0500 (EST) From: Aaron Mandel <amandel@husc.harvard.edu> To: ellard@deas.harvard.edu Subject: Final Project Proposal MIME-Version: 1.0 Content-Type: TEXT/PLAIN; ch...
HuaTang.txt
Path: Harvard >> CS >> 50 Fall, 2009
Description: /* * proposal.txt - Hua Tang * This is the proposal for my final project. * Id: proposa2.txt,v 1.1 1995/12/02 18:35:37 huatang Exp huatang **/ Abstract This project aims to construct a tool to study population genetics. The program takes the...
HuaTang.txt
Path: Harvard >> CS >> 95 Fall, 2009
Description: /* * proposal.txt - Hua Tang * This is the proposal for my final project. * Id: proposa2.txt,v 1.1 1995/12/02 18:35:37 huatang Exp huatang **/ Abstract This project aims to construct a tool to study population genetics. The program takes the...
dup.2.txt
Path: Harvard >> CS >> 50 Fall, 2009
Description: dup(2) dup(2) NAME dup - duplicate an open file descriptor SYNOPSIS #include <unistd.h> int dup(int fildes); DESCRIPTION fildes is a file descriptor obtain...
s9-ans.txt
Path: Harvard >> CS >> 50 Fall, 2009
Description: # $Id: s9-ans.txt,v 1.3 1995/11/27 17:22:08 ellard2 Exp ellard2 $ # Dan Ellard - 11/15/94 - Section Quiz Assume you have the following binary tree structure: typedef struct _tree_t { struct _tree_t *left; struct _tree_t *right; int value; ...
marks.pdf
Path: Harvard >> ISS >> 17 Fall, 2009
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Path: Harvard >> ISS >> 18 Fall, 2009
Description: FINDING THE BALANCE BETWEEN LIBERTY AND SECURITY: THE LORDS\' DECISION ON BRITAIN\'S ANTI-TERRORISM ACT In December 2001, following the lead of the United States, the United Kingdom responded to September 11 by passing the Anti-Terrorism, Crime and Sec...
steiner.pdf
Path: Harvard >> ISS >> 20 Fall, 2009
Description: \\server05\\productn\\H\\HLH\\20\\HLH2015.txt unknown Seq: 1 12-JUN-07 16:31 Human Rights: The Deepening Footprint Henry J. Steiner* The human rights movementyoung, fragile, universal, and consensual in its official discourse about norms but internall...
booknotes.pdf
Path: Harvard >> ISS >> 20 Fall, 2009
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Path: Harvard >> ISS >> 21 Fall, 2009
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Path: Harvard >> ISS >> 20 Fall, 2009
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Path: Harvard >> ISS >> 20 Fall, 2009
Description: \\server05\\productn\\H\\HLH\\20\\HLH2016.txt unknown Seq: 1 12-JUN-07 16:31 The Closeted Comparative Lawyer: On How to Pass for Human Rights Material Amr Shalakany* The Harvard Human Rights Program (HRP) was kind enough to accept me as a visiting fel...
shattuck.pdf
Path: Harvard >> ISS >> 16 Fall, 2009
Description: Religion, Rights, and Terrorism John Shattuck I understand that I was invited to give this keynote address because of my State Department credentials. It is true that I recently worked at the Human Rights Bureau and the Secretary of State\'s Adviso...
S_Jorstad.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Connection between X-ray and Polarized Radio Emission in the Large-Scale Jets of Quasars Svetlana Jorstad X-ray Emission Processes in Large-Scale Jets 1. Synchrotron radiation from radio to X-ray wavelengths (S~-: 3C 273, Uchiyama et al. 2006). 2. S...
SS_Bus_Schedule_08.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Harvard Summer Shuttle Schedule Morning & Evening Bus Schedule, June 22nd through August 15th. SOCH/Quad/ Cabot House Harvard Sq/ Garden St Winthrop House Hurlbut Hall Annenberg Hall Lamont Library Boylston Gate 7:00AM 7:30 8:00 8:35 9:10 9:45 10:20...
poster.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Radio Galaxies in the Chandra Era Hosted by the Chandra X-ray Center Cambridge, Massachusetts July 8-11, 2008 Registration and Abstract Submission Deadline: April 30 (talks and posters) May 21 (posters only) Workshop Goals: Chandra has profoundly in...
poster.pdf
Path: Harvard >> XSURVEYS >> 06 Fall, 2009
Description: ...
R_Mittal.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: AGN heating in the HIFLUGCS sample of galaxy clusters: A self-regulated feedback mechanism? Rupal Mittal, Daniel Hudson and Thomas Reiprich Collaborators: Heinz Andernach (U. Mexico), Tracy Clarke (NRL) and Paul Nulsen (CfA) Emmy Noether Research Gro...
M_Bruggen.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: The physics of AGN feedback in clusters of galaxies Marcus Brggen (Jacobs) Evan Scannapieco (ASU) with help by Sebastian Heinz Mitch Begelman Mateusz Ruszkowski Aurora Simionescu Bill Forman Perseus Fabian et al (2000 MNRAS 318 L65) Slide from Bill...
Agenda1.pdf
Path: Harvard >> XGRATINGS >> 07 Fall, 2009
Description: X-ray Spectroscopy Workshop July 11-13 2007 PROGRAM WEDNESDAY, July 11 Photoionization I Chair: Jane Turner 8:40 am Welcome 8:45-9:15 Invited: Claude Canizares Perspectives on the Development of High Resolution XRay Spectroscopy 9:15-9:45 Invited: ...
abs.pdf
Path: Harvard >> STARS >> 05 Fall, 2009
Description: q` d Tv qpv p` Vp bv T q g ` g v !G e !@!p iGcccWT e r x d T d g v v T V g v T p X q g T ` g ` ` p ` V p v e d ` p R p V p b aWfWT e rrifWT e hx W@Fi` e 6WUcWT e iGi!iug i9fr de 9i!hts ` cgWT e !YFcg 9GcrT pV e V T V v` V p bv qcgr@p ...
D_Harris.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Variability Timescales in the M87 Jet D. E. Harris (SAO) C. C. Cheung (GSFC) L. Stawarz (KIPAC) INTRODUCTION, METHODS, & PROBLEMS THE TEV CONNECTION: SITE OF EXCESS SIGNATURES OF E2 LOSSES IMPULSIVE BRIGHTENING IN HST-1 BACKGROUND Nucleus...
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Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: VLBI Imaging of a High Luminosity X-ray Hotspot Leith Godfrey Research School of Astronomy & Astrophysics Australian National University Geoff Bicknell, ANU Jim Lovell, UTAS Dave Jauncey, ATNF Dan Schwartz, Harvard-Smithsonian CfA Northern Hotspot ...
P_Ogle.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Impact of Jet Feedback on H2 and Star Formation in Radio Galaxies Patrick Ogle (Caltech, Spitzer Science Center) R. Antonucci, C. Leipski, Phil Appleton, Francois Boulanger Normal Star-Forming Galaxies Spitzer SINGS survey of nearby galaxies (Smith...
G_Madejski.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Structure of jet cores in blazars: -ray observations Greg Madejski Stanford Linear Accelerator Center and Kavli Institute for Particle Astrophysics and Cosmology In collaboration with: Jun Kataoka, Tad Takahashi, Marek Sikora, Rie Sato, Lukasz Staw...
Q_Hart.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: XrayandRadioAGNin ComaClusterProgenitors QuyenNguyenHart UniversityofColoradoatBoulder,CenterforAstrophysicsandSpaceAstronomy Collaborators CU-Boulder John Stocke Erica Ellingson Eric Hallman U. Of Michigan Gus Evrard OntheRoadtoComa More Massive...
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Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: X-ray and optical detection of the radio bent jet in 3C 17 F. Massaro & D. E. Harris, M. C hiabe , P. Grandi, rge F. D. Macche S A. Baum C P. O`De A. C tti tto, . , . a, ape Radio Galaxie in theC s handra Era X-ray jets in the Chandra archive PKS1...
M_Birkinshaw.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Radio galaxies in the Chandra era Jets: particle acceleration and entrainment Mark Birkinshaw University of Bristol Radio galaxies in the Chandra era Outline 1. Jets general physics issues 2. Deceleration through entrainment the Laing & Bridle a...
N_Isobe.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Hard X-ray study of lobes of radio galaxy Fornax A (RIKEN/Suzaku Help Desk) Naoki Isobe Makoto Tashiro, Hiromi Seta, Yuichi Yaji (Saitama Univ.) Keiko Matsuta, Hidehiro Kaneda (ISAS/JAXA), Kazuo Makishima (RIKEN/Univ.of Tokyo) etc. July 711, 2008 ...
M_Begelman.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: SPECIAL RELATIVITY FOR JET MODELERS Mitch Begelman JILA, University of Colorado Lorentz transformation 2 DISTINCT EFFECTS: Connects observers in different frames \"Rest\" (jet) frame \"Lab\" (observer) frame ( x, t ) ( x, t ) v cos t = t \'- x\'...
C_Jones.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Centaurus A Kraft, Hardcastle, Croston, Worrall, Birkinshaw, Nulsen, Forman, Murray, Goodger, Sivakoff ,Evans, Sarazin, Harris, Gilfanov, Jones Jet Southwest Inner Lobe Northern Middle Lobe Hot ISM X-ray composite image Centaurus A the Nearest Ra...
H_Li.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Magnetic Jets and Lobes in Cosmological MHD Hui Li Los Alamos National Laboratory NSF/DOE Center for Magnetic Self-Organization (CMSO) Collaborators: H. Xu, D. Collins, S. Li, M. Morman Overview of Observations and Magnetic Jet Model Results on 3D ...
S_Baum.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: There and Back Again: Cycles of Activity in Radio Galaxies Stefi Baum and Chris O\'Dea Rochester Institute of Technology 1 The Life Cycle Paradigm Birth Infancy (GPS/CSO) Youth (CSS) Adulthood (FR1/2) Death Rebirth 0 <NLR (10-1000pc) <Gal (1...
L_Birzan.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Radiative Efficiency and Content of Extragalactic Radio Sources Laura Brzan Collaborators: Brian McNamara (U. Waterloo), Paul Nulsen (CfA), Chris Carilli (NRAO), Mike Wise (U. Amsterdam) Radiative Efficiency / Scaling Relations An understanding of h...
S_Giancintucci.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Low frequency radio observations of galaxy groups S.Giacintucci (CfA), J. Vrtilek (CfA), E. O\'Sullivan (CfA), S. Raychaudhury (CfA, U. Birmingham), L.David (CfA), T.Venturi (INAF-IRA Italy), M. Murgia (INAF-Oss. Cagliari) With acknowledgements to: R...
D_Rafferty.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: The Regulation of Star Formation by AGN Feedback DAVID RAFFERTY (Penn State / Ohio U.) Collaborators: Brian McNamara (Waterloo) and Paul Nulsen (CfA) Star Formation & the ICM Indirect evidence links the ICM to star formation in the central galaxy...
M_Guainazzi.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: [and a note on Xray core spectra in lowpower radio RGs] \"Did I say radio quiet?\" Radioloudness in radioquiet Seyferts Matteo Guainazzi European Space Astronomy Center of ESA Villafranca del Castillo (Spain) XMMNewton Science Operations & Data Sys...
N_Jetha.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Shock heating in the group atmosphere of the radio galaxy B2 0838+32A Nazirah Jetha1, Martin Hardcastle2, Trevor Ponman3, Irini Sakelliou4 IRFU, CEA-Saclay, 2University of Hertfordshire, 3University of Birmingham, 4MPIA-Heidelberg, Germany 1 Radio g...
P_Hardee.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Helically Twisted Shocks in the M87 Jet Philip Hardee1, Andrei Lobanov2 & Jean Eilek3 The University of Alabama, Tuscaloosa, AL, USA 2 Max-Planck Institut fr Radioastronomie, Bonn, Germany 3 New Mexico Tech/NRAO, Socorro, NM, USA 1 RadioGals08, Camb...
M_Birkinshaw1.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Radio galaxies in the Chandra era AGN jet flows Mark Birkinshaw University of Bristol Radio galaxies in the Chandra era Outline 1. Critical questions 2. Low-power jets two case studies and some thoughts 3. High-power jets another case study with...
N_Soker.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Inflating Fat Bubbles in Clusters of Galaxies by Slow Wide Jets Assaf Sternberg Noam Soker (did the work) (speaker today) Technion, Israel Goal: To form \'Fat` Bubbles PERSEUS IN VISIBLE AND X-RAY From Fabian and collaborators Rayleigh-Taylor i...
finale.ppt
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: WHERE DO WE GO FROM HERE? Moderator: Mitch Begelman Panelists: Stefi Baum Katherine Blundell Greg Madejski Paul Nulsen Lukasz Stawarz X-RAYS FROM JETS/KNOTS WHERE HAVE WE BEEN? Close-in: relation to optical (HST), radio, IR (Spitzer!) Variabilit...
092_Saez.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: CONFIRMATION OF A CORRELATION BETWEEN THE X-RAY LUMINOSITY AND SPECTRAL SLOPE OF AGNs IN THE CHANDRA DEEP FIELDS. C. Saez (PSU), G. Chartas (PSU), W. N. Brandt (PSU), B. D. Lehmer (Durham), F. E. Bauer (Columbia), X. Dai (OSU), and G. P. Garmire (PSU...
053_Getman.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: X-ray flares, coronae and disks in Orion young stars K.V. Getman, E.D. Feigelson, P.S. Broos, G. P. Garmire (Penn State University) Pre-main sequence (PMS) stars are known to produce powerful X-ray flares which resemble magnetic reconnection solar fl...
055_Kashyap.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: #55 : 8 Years of Science with Chandra Symposium : 2007 Oct 22-25 Huntsville AL Detection of Short Timescale Variability in Capella Aur / HD 34029 / HR 1708 / SAO 40186 / 13 Aur Vinay Kashyap (SAO), Jennifer Posson-Brown (SAO) CAPELL...
074_Cavagnolo.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: The Entropy-Feedback Connection and Quantifying Cluster Virialization Kenneth W. Cavagnolo, Megan Donahue, G. Mark Voit, Ming Sun Michigan State University ABSTRACT Understanding the entropy of intracluster gas is the key to understanding 1) the feed...
099_Aarnio_ppt_pc.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Angular Momentum Loss Considerations in Large Scale T Tauri Flares A. N. Aarnio Abstract The Chandra Orion Ultradeep Project observed a number of T Tauri stars during highly energetic X-ray flare events. Favata et al. (2005) applied a uniform cooling...
101_Broos.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: 8 Years of Chandra Symposium Innovations in ACIS Imaging Data Analysis Patrick Broos, Leisa Townsley (ACIS Instrument Team, Penn State University) patb@astro.psu.edu Fields with thousands of X-ray point sources pose significant data analysis chall...
060_Tsujimoto.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: X-ray Imaging Study of RCW49 M. Tsujimoto , E. D. Feigelson , L. Townsley , P. Broos , K. V. Getman , J. Wang , 3 4 5 1 2 G. Garmire , D. Baba , T. Nagayama , M. Tamura , E. B. Churchwell 1 1 1 1 1 1 1 Pennsylvania State Univ., 2Nagoya Univ., 3 Kyot...
097_Kim.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: X-ray Luminosity Evolution in Normal Elliptical Galaxies with c-COSMOS Dong-Woo Kim (cfa), G. Fabbiano (cfa), M. Elvis (cfa), T. Aldcroft (cfa), H. Brunner (mpg), M. Brusa (mpg), N. Cappelluti (mpg), F. Civano (bo), A. Comastri (bo), A. Finoguenov (m...
094_Aldcroft.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Not just an Xray Extractor Tom Aldcroft, SAO/CXC http:/cxc.harvard.edu/contrib/yaxx Key Features: Yaxx is a Perl script that facilitates batch data processing using Perl open source tools and commonly available astronomical software (CIAO/Sherpa, SAS...
065_DeLaney.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Doppler Velocities of X-ray Knots and Filaments in the LMC SNR N132D Tracey DeLaney, Dan Dewey, Claude Canizares MIT Kavli Institute Dispersed Spectra: What\'s in this Supernova Remnant? ABSTRACT The oxygen-rich supernova remnant N132D in the Large Ma...
090_Mueller.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Toward a Handle on the Low-energy End of the Electron Distribution in Large-scale Jets: The Case of PKS 0637-752 Martin Mueller (KIPAC/SLAC), Dan Schwartz (SAO) Motivation: Unknown Behavior of the Electron Distribution at Low Energies The Uniqueness ...
076_Dupke.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Constraining the Age of Fossil Groups with Chandra Renato Dupke University of Michigan, Ann Arbor INTRO Fossil groups (FGs) are classically defined as systems dominated by a single giant elliptical galaxy and with a 2 magnitude difference between th...
063_Allen.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: The High-Energy X-Ray Spectrum of Cas A: Nonthermal Brem. v. Synchrotron Radiation Allen, G. 1, E. Stage, M. 1 2, D. and Houck, J. 1 C. MIT, 2U. Mass. E [keV] 0.1 0.3 1 3 10 30 Abstract We performed a spectral analysis of some Chandra ACIS and ...
062_Airhart.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Spectral and Temporal Monitoring of the Abstract C. Airhart (Dynetics, Inc.); P.M. Woods (Dynetics, Inc., National Space Science and Technology Center); V. Zavlin (National Space Science and Technology Center, Marshall Space Flight Center); M.H. Fin...
098_Tuellmann.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: The Chandra ACIS Survey of M33 (ChASeM33): Investigating the Hot Ionized Medium of NGC604 R. Tllmann , T. J. Gaetz , P. P. Plucinsky , P. Ghavamian , D. Breitschwerdt , M. Avillez , u 2 5 6 7 W. P. Blair , K. S. Long , T. G. Pannuti , P. Frank Winkle...
104_Xiang.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Probing the 4U 1624-490 Ionized Gas and Dust distribution along the LOS Jingen Xiang , Julia. C. Lee (Harvard University) and Michael. A. Nowak , Norbert S Schulz (MIT) 1. jxiang@cfa.harvard.edu 2. jclee@cfa.harvard.edu 3. mnowak@space.mit.edu 4. nss...
050_Wolk_ppt_pc.pdf
Path: Harvard >> SYMPOSIUM >> 2007 Fall, 2009
Description: Chandra\'s Close Encounter with the Disintegrating Comet SW3/73P- Fragment B S. J. Wolk (CfA), C.M. Lisse (APL), D. Bodewits (KVI), D. J. Christian (UQB) & K. Dennerl (MPE) On May 23, 2006 we used the ACIS-S instrument on Chandra to study the X-ray em...
Darcangelo_Francesca.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Rapid Multiwavelength Polarization Correlation in OJ287 and Other Blazars F. D. DArcangelo, A. P. Marscher, S. G. Jorstad, P. S. Smith, V. M. Larionov, V. A. Hagen-Thorn, G. G. Williams, D. P. Clemens Boston University, University of Arizona, St. Pet...
M_Sobolewska.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: What can we learn about AGN from OX measurements in GBHs? Malgosia Sobolewska (FORTH, Crete, Greece) with Marek Gierlinski (University of Durham, UK) Aneta Siemiginowska (SAO, Cambridge, USA) Radio Galaxies in the Chandra Era, 2008 Malgosia Sobole...
T_Ergin.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: OBSERVATIONS OF VERY HIGH ENERGY GAMMA RAYS FROM M87 BY VERITAS Tln Ergin (U. of Massachusetts Amherst, MA) on behalf of the VERITAS Collaboration (http:/veritas.sao.arizona.edu) 1 APOD , 2004 December 11 T.Ergin ...
P_Kharb.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Pc-scale rotation measures across radio galaxy jets Department of Physics, Purdue University, IN D. C. Gabuzda (UCC, Cork) C. P. O\' Dea (RIT, Rochester, NY) P. Shastri (IIA, Bangalore) S. A. Baum (RIT, Rochester, NY) P. Kharb Faraday Rotation Rotat...
R_Laing.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Precision Jet Physics Low-power radio galaxies and their environments Robert Laing (ESO) Deep, multiconfiguration VLA observations Spectra High-resolution IQU, corrected for Faraday rotation Kinematic models of jets Faraday rotation images Optic...
S_Willner.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: High Redshift 3CR Sources: Spitzer Mid-infrared SEDs Steve Willner, Matt Ashby, Rolf Chini, Giovanni Fazio, Martin Haas, Frank Heymann, Ralf Siebenmorgan, Belinda Wilkes Related posters: Christian Leipski: Spitzer Mid-infrared Spectra Belinda Wil...
Miller_Brendan.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: Chandra Observations of Hybrid Morphology Radio Sources B. P. Miller, W. N. Brandt (Pennsylvania State University) Overview The classification scheme devised by Fanaroff & Riley (1974) identifies FR I sources as core brightened and the more luminous...
OSullivan_Ewan.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: A Combined X-ray/Low-Frequency Radio Survey of Feedback in Galaxy Groups E. OSullivan , S. Giacintucci , S. Raychaudhury , J.M. Vrtilek , L.P. David 1 1 2 1 [1] Harvard-Smithsonian Center for Astrophysics (USA) [2] University of Birmingham (UK) Motiv...
Hogan_Brandon.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: X-ray Jets in Superluminal Blazars Brandon Hogan (Purdue University), Matthew Lister (Purdue University), Herman Marshall (MIT), Preeti Kharb (Purdue University) We are currently investigating a complete sample of 32 sources selected from the MOJAVE ...
Massaro_Francesco.pdf
Path: Harvard >> RADIOGALS >> 08 Fall, 2009
Description: The Chandra 3C Snapshot Survey for Sources with z < 0.3 F. Massaro1, D. E. Harris1, D. Axon2, S. A. Baum3, A.Capetti4, M. Chiaberge5, R. Gilli6, G. Giovannini7, P. Grandi8, F. D. Macchetto5, C. P. O\'Dea2, G. Risaliti9, W. Sparks5. 1 Harvard, Smithso...