UNIQ: Uniform Noise Injection for Non-Uniform Quantization of Neural
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The Different Unix Contexts
The different Unix contexts • User-level • Kernel “top half” - System call, page fault handler, kernel-only process, etc. • Software interrupt • Device interrupt • Timer interrupt (hardclock) • Context switch code Transitions between contexts • User ! top half: syscall, page fault • User/top half ! device/timer interrupt: hardware • Top half ! user/context switch: return • Top half ! context switch: sleep • Context switch ! user/top half Top/bottom half synchronization • Top half kernel procedures can mask interrupts int x = splhigh (); /* ... */ splx (x); • splhigh disables all interrupts, but also splnet, splbio, splsoftnet, . • Masking interrupts in hardware can be expensive - Optimistic implementation – set mask flag on splhigh, check interrupted flag on splx Kernel Synchronization • Need to relinquish CPU when waiting for events - Disk read, network packet arrival, pipe write, signal, etc. • int tsleep(void *ident, int priority, ...); - Switches to another process - ident is arbitrary pointer—e.g., buffer address - priority is priority at which to run when woken up - PCATCH, if ORed into priority, means wake up on signal - Returns 0 if awakened, or ERESTART/EINTR on signal • int wakeup(void *ident); - Awakens all processes sleeping on ident - Restores SPL a time they went to sleep (so fine to sleep at splhigh) Process scheduling • Goal: High throughput - Minimize context switches to avoid wasting CPU, TLB misses, cache misses, even page faults. • Goal: Low latency - People typing at editors want fast response - Network services can be latency-bound, not CPU-bound • BSD time quantum: 1=10 sec (since ∼1980) - Empirically longest tolerable latency - Computers now faster, but job queues also shorter Scheduling algorithms • Round-robin • Priority scheduling • Shortest process next (if you can estimate it) • Fair-Share Schedule (try to be fair at level of users, not processes) Multilevel feeedback queues (BSD) • Every runnable proc. -
Backup and Restore Cisco Prime Collaboration Provisioning
Backup and Restore Cisco Prime Collaboration Provisioning This section explains the following: • Perform Backup and Restore, page 1 • Back Up the Single-Machine Provisioning Database, page 2 • Restore the Single-Machine Provisioning Database, page 3 • Schedule Backup Using the Provisioning User Interface, page 5 Perform Backup and Restore Cisco Prime Collaboration Provisioning allows you to backup your data and restore it. You can schedule periodic backups using the Provisioning UI (Schedule Backup Using the Provisioning User Interface, on page 5). There are two backup and restore scenarios; select the set of procedures that matches your scenario: • Backup and restore on a single machine, with the same installation or a new installation. For this scenario, see Schedule Backup Using the Provisioning User Interface, on page 5. Note When backing up files, you should place the files on a different file server. Also, you should burn the backup data onto a CD. Cisco Prime Collaboration Provisioning allows you to back up system data and restore it on a different system in the event of total system failure. To restore the backup from another system, the following prerequisites must be met: • Ensure that the server to which data is restored has the same MAC address as that of the system that was backed up (the IP address and the hostname can be different). • If you are unable to assign the MAC address of the original system (the one that was backed up) to another system, contact the Engineering Team for information on a new license file (for a new MAC address). Cisco Prime Collaboration Provisioning Install and Upgrade Guide, 12.3 1 Backup and Restore Cisco Prime Collaboration Provisioning Back Up the Single-Machine Provisioning Database • The procedure to backup and restore data on a different system is the same as the procedure to backup and restore data on the same system. -
80842-Su | Cc/Led/27W/E26-E39/Mv/50K Corn Cob Sunlite
Item: 80842-SU CC/LED/27W/E26-E39/MV/50K CORN COB SUNLITE General Characteristics Bulb Corn Lamp Type Corn Cob Lamp Life Hours 50000 Hours Material Aluminium & Plastic LED Type LG5630 Base Medium (E26) Lumens Per Watt (LPW) 135.00 Life (based on 3hr/day) 45.7 Years Estimated Energy Cost $3.25 per Year Safety Rating UL Listed Ingress Protection IP64 Sunlite CC/LED/27W/E26-E39/MV/50K LED 27W (100W MHL/HPSW Electrical Characteristics Equivalent) Corn Bulb, Medium (E26), Watts 27 5000K Super White Volts 100-277 Equivalent Watts 100 LED Chip Manufacturer LG5630 Sunlite's super efficient LED corn lamps were created to Number of LEDs 84 replace the equivalent but power hungry metal halide and Power Factor 0.9 high-pressure sodium lamps. Capable of withstanding water sprays from any direction in thanks to its IP64 rating, these Temperature -40° To 140° bulbs will keep outdoor paths, back yards and many more locations illuminated for a significantly longer period of time Light Characteristics when compared to a high-pressure sodium lamp or a metal Brightness 3645 Lumens halide while also lowering your electrical usage. Color Accuracy (CRI) 85 Light Appearance Super White Color Temperature 5000K • This modern corn cob lamp produces an efficient 5000K Beam Angle 360° super white beam of 360° light at a powerful 3645 lumens • On average, this multi-volt LED corn cob lamp lasts up to Product Dimensions an astonishing 50,000 hours and features 84 energy MOL (in) 7.4 saving diodes Diameter (in) 3.65 • Ideal for all post lights, Street lights, security Lighting, high Package Dimensions (in) (W) 3.70 (H) 11.90 (D) 3.80 bay lights while also designed for indoor as well as Product Data outdoor usage. -
FIFI-LS Highlights Robert Minchin FIFI-LS Highlights
FIFI-LS Highlights Robert Minchin FIFI-LS Highlights • Nice face-on galaxies where [CII] traces star formation [CII] traces star formation in M51 Pineda et al. 2018 [CII] in NGC 6946 Bigiel et al. 2020 [CII] particularly important as H2 & SFR tracer in inter-arm regions FIFI-LS Highlights • Nice face-on galaxies where [CII] traces star formation • Galaxies where [CII] doesn’t trace star formation [CII] from shocks & turbulence in NGC 4258 • [CII] seen along X-ray/radio ‘arms’ of NGC 4258, associated with past or present jet activity • [CII] excited by shocks and turbulence associated with the jet impacting the disk • NOT star formation Appleton et al. 2018 Excess [CII] in HE 1353-1917 1011 HE 1353-1917 1% MUSE RGB Images: 0.1 % • HE 1353-1917 1010 iband[OIII] Hα 0.02 % has a large 109 excess in HE 0433-1028 L[CII]/LFIR 8 10 excess 1σ 10 × 2σ /L 3C 326 3σ HE 1029-1831 • AGN ionization [CII] 7 10 HE 1108-2813 L cone intercepts HE 2211-3903 106 the cold SOFIA AGN Hosts galactic disk AGN Hosts High z 105 LINERs [Brisbin+15] Normal Galaxies LIRGs ULIRGs [Decarli+18] 104 108 109 1010 1011 1012 1013 1014 L /L Smirnova-Pinchukova et al. 2019 FIR Shock-excited [CII] in NGC 2445 [CII] in the ring of NGC 2445 is enhanced compared to PAHs, showing a shock excitement origin rather than star formation Fadda & Appleton, 2020, AAS Meeting 235 FIFI-LS Highlights • Nice face-on galaxies where [CII] traces star formation • Galaxies where [CII] doesn’t trace star formation • Galaxies with gas away from the plane Extraplanar [CII] in edge-on galaxies • Edge-on galaxies NGC 891 & NGC 5907 observed by Reach et al. -
Unix Security Overview: 1
CIS/CSE 643: Computer Security (Syracuse University) Unix Security Overview: 1 Unix Security Overview 1 User and Group • Users – root: super user (uid = 0) – daemon: handle networks. – nobody: owns no files, used as a default user for unprivileged operations. ∗ Web browser can run with this mode. – User needs to log in with a password. The encrypted password is stored in /etc/shadow. – User information is stored in /etc/passwd, the place that was used to store passwords (not anymore). The following is an example of an entry in this file. john:x:30000:40000:John Doe:/home/john:/usr/local/bin/tcsh • Groups – Sometimes, it is more convenient if we can assign permissions to a group of users, i.e. we would like to assign permission based on groups. – A user has a primary group (listed in /etc/passwd), and this is the one associated to the files the user created. – Any user can be a member of multiple groups. – Group member information is stored in /etc/group % groups uid (display the groups that uid belongs to) – For systems that use NIS (Network Information Service), originally called Yellow Page (YP), we can get the group information using the command ypcat. % ypcat group (can display all the groups and their members) 2 File Permissions • File Permissions – The meaning of the permission bits in Unix. ∗ Owner (u), Group (g), and Others (o). ∗ Readable (r), Writable (w), and Executable (x). ∗ Example: -rwxrwxrwx (777) • Permissions on Directories: – r: the directory can be listed. – w: can create/delete a file or a directory within the directory. -
Sleep 2.1 Manual
Sleep 2.1 Manual "If you put a million monkeys at a million keyboards, one of them will eventually write a Java program. The rest of them will write Perl programs." -- Anonymous Raphael Mudge Sleep 2.1 Manual Revision: 06.02.08 Released under a Creative Commons Attribution-ShareAlike 3.0 License (see http://creativecommons.org/licenses/by-sa/3.0/us/) You are free: • to Share -- to copy, distribute, display, and perform the work • to Remix -- to make derivative works Under the following conditions: Attribution. You must attribute this work to Raphael Mudge with a link to http://sleep.dashnine.org/ Share Alike. If you alter, transform, or build upon this work, you may distribute the resulting work only under the same, similar or a compatible license. • For any reuse or distribution, you must make clear to others the license terms of this work. The best way to do this is with a link to the license. • Any of the above conditions can be waived if you get permission from the copyright holder. • Apart from the remix rights granted under this license, nothing in this license impairs or restricts the author's moral rights. Your fair use and other rights are in no way affected by the above. Table of Contents Introduction................................................................................................. 1 I. What is Sleep?...................................................................................................1 II. Manual Conventions......................................................................................2 III. -
Lab Intro to Console Commands
New Lab Intro to KDE Terminal Konsole After completing this lab activity the student will be able to; Access the KDE Terminal Konsole and enter basic commands. Enter commands using a typical command line interface (CLI). Explain the use of the following commands, ls, ls –al, dir, mkdir, whoami, Explain the directory structure of a typical user. This lab activity will introduce you to one of the many command line interfaces available in Linux/UNIX operating systems and a few of the most basic commands. The command line interface you will be using for this lab activity is the console called the Konsole and is also referred to as Terminal. Note: As you notice, in the KDE system many features are written with the capital letter “K” in place of the first letter or the utility to reflect the fact it was modified for the KDE system. The original UNIX system did not use a graphical user interface GUI but rather was a command line interface (CLI) similar to the command prompt in Windows operating systems. The command line interface is referred to as a shell. Even today the command line interface (the shell) is used to issue commands on a Linux server to minimize system resources. For example, there is no need to start the GUI on the server to add a new user to an existing system. Starting the GUI will reduce the system performance because it requires RAM to run the GUI. A GUI will affect the overall performance of the server when it is supporting many users (clients). -
Parallel Processing Here at the School of Statistics
Parallel Processing here at the School of Statistics Charles J. Geyer School of Statistics University of Minnesota http://www.stat.umn.edu/~charlie/parallel/ 1 • batch processing • R package multicore • R package rlecuyer • R package snow • grid engine (CLA) • clusters (MSI) 2 Batch Processing This is really old stuff (from 1975). But not everyone knows it. If you do the following at a unix prompt nohup nice -n 19 some job & where \some job" is replaced by an actual job, then • the job will run in background (because of &). • the job will not be killed when you log out (because of nohup). • the job will have low priority (because of nice -n 19). 3 Batch Processing (cont.) For example, if foo.R is a plain text file containing R commands, then nohup nice -n 19 R CMD BATCH --vanilla foo.R & executes the commands and puts the printout in the file foo.Rout. And nohup nice -n 19 R CMD BATCH --no-restore foo.R & executes the commands, puts the printout in the file foo.Rout, and saves all created R objects in the file .RData. 4 Batch Processing (cont.) nohup nice -n 19 R CMD BATCH foo.R & is a really bad idea! It reads in all the objects in the file .RData (if one is present) at the beginning. So you have no idea whether the results are reproducible. Always use --vanilla or --no-restore except when debugging. 5 Batch Processing (cont.) This idiom has nothing to do with R. If foo is a compiled C or C++ or Fortran main program that doesn't have command line arguments (or a shell, Perl, Python, or Ruby script), then nohup nice -n 19 foo & runs it. -
Open Data/Open Source: Seismic Unix Scripts to Process a 2D Land Line
Open Data/Open Source: Seismic Unix scripts to process a 2D land line Karl Schleicher k [email protected] John A. and Katherine G. Jackson School of Geosciences The University of Texas at Austin University Station, Box X Austin, TX 78713-8924 (January 29, 2012) Running head: Alaska ABSTRACT This paper describes how to process an internet downloadable 2D land line data set though a very basic processing sequence using Seismic Unix. The data from the Alaska North Slope has good signal, although it may be suitable for testing ground-roll and noise burst attenuation programs. The detailed steps to download the dataset from the Internet and process it are described. You should be able to follow these steps and recreate my results. I hope this will accelerate the testing and validation of programs developed in different research groups. The paper starts with background information such as data downloading, region overview, data acquisition, and previous processing. The scripts and custom programs for Seismic Unix translation, header load, qc, shotrecord velocity filter, deconvolution, CDP gather, velocity analysis, residual statics, stack, and post stack migration can be downloaded to 1 your computer. Header loading is not well described in other Seismic Unix documentation or papers. One approach to header loading is described here. The velocity analysis script is more advanced than what I found in previous publications. This paper is the beginning of an effort to build an open data/open source library for research, software testing, demonstrations, and user training. I encourage you to use these scripts and improve on my results. -
Unix Quickref.Dvi
Summary of UNIX commands Table of Contents df [dirname] display free disk space. If dirname is omitted, 1. Directory and file commands 1994,1995,1996 Budi Rahardjo ([email protected]) display all available disks. The output maybe This is a summary of UNIX commands available 2. Print-related commands in blocks or in Kbytes. Use df -k in Solaris. on most UNIX systems. Depending on the config- uration, some of the commands may be unavailable 3. Miscellaneous commands du [dirname] on your site. These commands may be a commer- display disk usage. cial program, freeware or public domain program that 4. Process management must be installed separately, or probably just not in less filename your search path. Check your local documentation or 5. File archive and compression display filename one screenful. A pager similar manual pages for more details (e.g. man program- to (better than) more. 6. Text editors name). This reference card, obviously, cannot de- ls [dirname] scribe all UNIX commands in details, but instead I 7. Mail programs picked commands that are useful and interesting from list the content of directory dirname. Options: a user's point of view. 8. Usnet news -a display hidden files, -l display in long format 9. File transfer and remote access mkdir dirname Disclaimer make directory dirname The author makes no warranty of any kind, expressed 10. X window or implied, including the warranties of merchantabil- more filename 11. Graph, Plot, Image processing tools ity or fitness for a particular purpose, with regard to view file filename one screenfull at a time the use of commands contained in this reference card. -
User Accounts User Accounts User Info /Etc/Passwd User Info /Etc
User Accounts Even a single-user workstation (Desktop Computer) uses multiple accounts. Such a computer may have just one user account, but several system accounts help keep the computer running. Accounts enable multiple users to share a single computer without causing each other too much trouble. User Accounts The Users in a Linux system are stored in the /etc/passwd file. If you are on your own VM - somewhere near the bottom you should see yourself and joe. On a brand new install you will see many users listed. Of course if you recall, we only added ourselves and joe. So what are all these other users for? These users are added because we don’t want to give sudo power to all of our programs. So each program installed gets its own user with its own limited permissions. This is a protection for our computer. User Info /etc/passwd Examine the /etc/passwd file using cat or less . Here is what we are seeing: It is colon : separated. So each : denotes a new column. username password The x is just a place-holder. The password is not really in this file User ID (UID) Just like every computer needs a unique ip address, every user needs a unique id. User Info /etc/passwd Group ID (GID) Every user belongs to its own group, with its own group id Comment field This is the Full name, phone number, office number, etc. It is okay if it is blank. Home Directory This is the location of the users home directory - This is how we can know the full path of any users home directory - /home/smorgan vs /home/s/smorgan. -
Transcript of Interviews
UNIVERSITY OF OXFORD ANNUAL REVIEW 2013/14 REALISING THE POTENTIAL The UNIQ scheme allows academically able students from state schools to experience student life at a top research-led university Transcript of interviews Alistair (mentor): UNIQ’s been running five years now and I was a student The Humanities UNIQ course and other themed courses on the very first year. I’ve now been a mentor for two allow students to dip into history and English and whatever years. There are lots of lectures, which are a bit like the they want. Or general science UNIQ courses, where ones you would have in Oxford as an undergraduate; lab they can actually spend a week deciding which of these work as well, with similar experiments; and a lot of social disciplines suits them most, or maybe they want to do a activities as well with the other students. joint or combined honours course. Fiona (mentor): Fiona: The summer school was in fact way more packed into When I was 17 doing UNIQ I thought the 21-year-olds a week than I actually find myself doing in a week at running the course, assisting on the course, were so old. Oxford. I thought they’d got everything together, they were so mature, they were all going to go and have jobs. It’s quite Selina Todd, lecturer in history: nice that they must see me in the same way, as someone The culmination of the week was finishing and handing who’s been through it, and got their act together. I think the in – and having marked – your first Oxford history essay.