Prospectus, August 30, 1983

NEW PARK-LAND APARTMENTS FILL EMPTY FIELD SOUTH OF PARKLAND; Survival hints for Parkland; News Digest; President Staerkel welcomes new students to Parkland; September 1983 Parkland College Calendar; Is your class cancelled?; Bookstore supplies more than books; Everyone is welcome to enjoy Fall-In \u2783; StuGo welcomes all; New addition takes care of classroom needs; Choose your movies; Lindstrand awards six films as best summer flics; Chase has bad vacation--produces funny flic; Keaton and Garr star in Mr. Mom ; Greatest Show returns to Assembly Hall; New Doctor Who to be televised; Reviewing summer\u27s top music hits; Skylines; Parkland employees honored; Neal retires; Classified; Guard goes north for summer camp; Police fingerprint children; Beginning Again program for bereaved; Improve bowling skills--join Bowling Club; Woods Words: Stadium to celebrate its 60th yearhttps://spark.parkland.edu/prospectus_1983/1013/thumbnail.jp

Prospectus, December 14, 1983

MERRY CHRISTMAS TO ALL; Memories recalled from Christmases past; 32 are named in Who\u27s Who; News Digest; Parkland student talks with Santa; Simpson keeps position; Illinois joins no-fault divorce movement; PC Happenings: Second blood drive is success; German club goes to Chicago; Rotary scholarships available; Camera ban lifted; Final Exam Schedule; Looking forward to a winter like last year\u27s!; Parkland publishes annual magazine--Intercom; Zamary decorates cakes; Letter to the editor; Christmas carols are important part of world history; Letter to the editor; Question: When did you stop believing in Santa?; Question: What was the best Christmas gift you ever received?; Question: What is your best Christmas memory or tradition?; Christmas--ancient celebration of the birth of Christ; Spring brings more of an abundance of Cabbage Patches; The brighter side of Christmas; Make holiday cleaning easy; Tips for easier Holiday Baking; Tree trimming is art; Christmas cards originate in England; Recipes for Christmas and New Years; Christmas of yesteryear at the Lake of the Woods; Parkland before the brown brick campus; Photographer captures old-fashioned Christmas; Wham Bam it\u27s Tieken man and U.R.S.A..; Pulitzer winner at Krannert; WILL--most varied holiday line-up; Variety of films hits the 1983 Christmas season; Dylan is back again; \u27Stones\u27 come back to life; January Krannert Schedule; Classifieds; Tips on how to stay out of an accident on icy days; 1984 Bowl game schedule; Cobra volleyball players feted; Composite Athletic Schedule; I.M. News...; Women win; Track tream ready for season; Fire hazard safety tips; Local search for Opryland talent; President\u27s Christmas messagehttps://spark.parkland.edu/prospectus_1983/1000/thumbnail.jp

The Science Case for an Extended Spitzer Mission

Although the final observations of the Spitzer Warm Mission are currently scheduled for March 2019, it can continue operations through the end of the decade with no loss of photometric precision. As we will show, there is a strong science case for extending the current Warm Mission to December 2020. Spitzer has already made major impacts in the fields of exoplanets (including microlensing events), characterizing near Earth objects, enhancing our knowledge of nearby stars and brown dwarfs, understanding the properties and structure of our Milky Way galaxy, and deep wide-field extragalactic surveys to study galaxy birth and evolution. By extending Spitzer through 2020, it can continue to make ground-breaking discoveries in those fields, and provide crucial support to the NASA flagship missions JWST and WFIRST, as well as the upcoming TESS mission, and it will complement ground-based observations by LSST and the new large telescopes of the next decade. This scientific program addresses NASA's Science Mission Directive's objectives in astrophysics, which include discovering how the universe works, exploring how it began and evolved, and searching for life on planets around other stars.Comment: 75 pages. See page 3 for Table of Contents and page 4 for Executive Summar

The Vehicle, 1965, Vol. 7

Vol. 7 Table of Contents CommentaryElaine Lancepage 3 Lost Island and The Unseen SeaDaun Alan Leggpage 5 ElegyWilliam Mosierpage 6 AwayDavid Dixpage 7 DulceyRoberta Mathewspage 8 Alarum Tuam JonneDavid Walkerpage 11 Little BrotherSteve Gibbspage 13 River RunningDaun Alan Leggpage 15 PortraitRobert D. Thomaspage 16 The RockRoger Lewis Hudsonpage 17 Jarman HospitalElaine Lancepage 18 Of Domes and DiamondsDwight Ashbypage 19 Friday NightRoger J. Barrypage 20 MurderHelen Coxpage 23 Vigil SongDaun Alan Leggpage 24 Had You But Been the OneDavid Helmpage 25 To A Useless WeaponDarlene Brewerpage 25 Out of the NightPat Hartpage 26 La MortAdrian Beardpage 28 Mrs. Milton\u27s LamentBob Millerpage 30 Cockle CoveSusan McCabepage 31 Loss of VirtueJim Rinnertpage 32 The KeepsakeDwight Ashbypage 33 The RuinsRoger Lewis Hudsonpage 35 Ante Major OdysseyDaun Alan Leggpage 38 ReligionAnthony Barrettepage 39 All JoyJim Rinnertpage 40 SesameElaine Lancepage 40 CenterpieceDwight Ashbypage 41 A Great White WaveJohn Rhodespage 42 QueryElaine Lancepage 44 PistachioRita Salyerspage 45 FacadeKathleen McCormackpage 46 Winter Wisp AwaySteve Gibbspage 46 ScenarioDavid Dixpage 47 Damn-GodSteve Gibbspage 48 AccidentElaine Lancepage 48https://thekeep.eiu.edu/vehicle/1013/thumbnail.jp

VEGFR2 promotes central endothelial activation and the spread of pain in inflammatory arthritis

Chronic pain can develop in response to conditions such as inflammatory arthritis. The central mechanisms underlying the development and maintenance of chronic pain in humans are not well elucidated although there is evidence for a role of microglia and astrocytes. However in pre-clinical models of pain, including models of inflammatory arthritis, there is a wealth of evidence indicating roles for pathological glial reactivity within the CNS. In the spinal dorsal horn of rats with painful inflammatory arthritis we found both a significant increase in CD11b+ microglia-like cells and GFAP+ astrocytes associated with blood vessels, and the number of activated blood vessels expressing the adhesion molecule ICAM-1, indicating potential glio-vascular activation. Using pharmacological interventions targeting VEGFR2 in arthritic rats, to inhibit endothelial cell activation, the number of dorsal horn ICAM-1+ blood vessels, CD11b+ microglia and the development of secondary mechanical allodynia, an indicator of central sensitization, were all prevented. Targeting endothelial VEGFR2 by inducible Tie2-specific VEGFR2 knock-out also prevented secondary allodynia in mice and glio-vascular activation in the dorsal horn in response to inflammatory arthritis. Inhibition of VEGFR2 in vitro significantly blocked ICAM-1-dependent monocyte adhesion to brain microvascular endothelial cells, when stimulated with inflammatory mediators TNFa and VEGF-A165a. Taken together our findings suggest that a novel VEGFR2-mediated spinal cord gliovascular mechanism may promote peripheral CD11b+ circulating cell transmigration into the CNS parenchyma and contribute to the development of chronic pain in inflammatory arthritis. We hypothesise that preventing this glio-vascular activation and circulating cell translocation into the spinal cord could be a new therapeutic strategy for pain caused by rheumatoid arthritis

The ABC130 barrel module prototyping programme for the ATLAS strip tracker

For the Phase-II Upgrade of the ATLAS Detector, its Inner Detector, consisting of silicon pixel, silicon strip and transition radiation sub-detectors, will be replaced with an all new 100 % silicon tracker, composed of a pixel tracker at inner radii and a strip tracker at outer radii. The future ATLAS strip tracker will include 11,000 silicon sensor modules in the central region (barrel) and 7,000 modules in the forward region (end-caps), which are foreseen to be constructed over a period of 3.5 years. The construction of each module consists of a series of assembly and quality control steps, which were engineered to be identical for all production sites. In order to develop the tooling and procedures for assembly and testing of these modules, two series of major prototyping programs were conducted: an early program using readout chips designed using a 250 nm fabrication process (ABCN-25) and a subsequent program using a follow-up chip set made using 130 nm processing (ABC130 and HCC130 chips). This second generation of readout chips was used for an extensive prototyping program that produced around 100 barrel-type modules and contributed significantly to the development of the final module layout. This paper gives an overview of the components used in ABC130 barrel modules, their assembly procedure and findings resulting from their tests.Comment: 82 pages, 66 figure

Alignment of the CMS silicon tracker during commissioning with cosmic rays

This is the Pre-print version of the Article. The official published version of the Paper can be accessed from the link below - Copyright @ 2010 IOPThe CMS silicon tracker, consisting of 1440 silicon pixel and 15 148 silicon strip detector modules, has been aligned using more than three million cosmic ray charged particles, with additional information from optical surveys. The positions of the modules were determined with respect to cosmic ray trajectories to an average precision of 3–4 microns RMS in the barrel and 3–14 microns RMS in the endcap in the most sensitive coordinate. The results have been validated by several studies, including laser beam cross-checks, track fit self-consistency, track residuals in overlapping module regions, and track parameter resolution, and are compared with predictions obtained from simulation. Correlated systematic effects have been investigated. The track parameter resolutions obtained with this alignment are close to the design performance.This work is supported by FMSR (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP (Brazil); MES (Bulgaria); CERN; CAS, MoST, and NSFC (China); COLCIENCIAS (Colombia); MSES (Croatia); RPF (Cyprus); Academy of Sciences and NICPB (Estonia); Academy of Finland, ME, and HIP (Finland); CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece); OTKA and NKTH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); NRF (Korea); LAS (Lithuania); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); PAEC (Pakistan); SCSR (Poland); FCT (Portugal); JINR (Armenia, Belarus, Georgia, Ukraine, Uzbekistan); MST and MAE (Russia); MSTDS (Serbia); MICINN and CPAN (Spain); Swiss Funding Agencies (Switzerland); NSC (Taipei); TUBITAK and TAEK (Turkey); STFC (United Kingdom); DOE and NSF (USA)

Commissioning and performance of the CMS pixel tracker with cosmic ray muons

This is the Pre-print version of the Article. The official published verion of the Paper can be accessed from the link below - Copyright @ 2010 IOPThe pixel detector of the Compact Muon Solenoid experiment consists of three barrel layers and two disks for each endcap. The detector was installed in summer 2008, commissioned with charge injections, and operated in the 3.8 T magnetic field during cosmic ray data taking. This paper reports on the first running experience and presents results on the pixel tracker performance, which are found to be in line with the design specifications of this detector. The transverse impact parameter resolution measured in a sample of high momentum muons is 18 microns.This work is supported by FMSR (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP (Brazil); MES (Bulgaria); CERN; CAS, MoST, and NSFC (China); COLCIENCIAS (Colombia); MSES (Croatia); RPF (Cyprus); Academy of Sciences and NICPB (Estonia); Academy of Finland, ME, and HIP (Finland); CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece); OTKA and NKTH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); NRF (Korea); LAS (Lithuania); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); PAEC (Pakistan); SCSR (Poland); FCT (Portugal); JINR (Armenia, Belarus, Georgia, Ukraine, Uzbekistan); MST and MAE (Russia); MSTDS (Serbia); MICINN and CPAN (Spain); Swiss Funding Agencies (Switzerland); NSC (Taipei); TUBITAK and TAEK (Turkey); STFC (United Kingdom); DOE and NSF (USA)

Performance of the CMS drift-tube chamber local trigger with cosmic rays

The performance of the Local Trigger based on the drift-tube system of the CMS experiment has been studied using muons from cosmic ray events collected during the commissioning of the detector in 2008. The properties of the system are extensively tested and compared with the simulation. The effect of the random arrival time of the cosmic rays on the trigger performance is reported, and the results are compared with the design expectations for proton-proton collisions and with previous measurements obtained with muon beams