#Magento Certified Developer in Dallas

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Magento Certified Developers in Dallas

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Adobe Commerce Magento Consulting Services | Houston A leader in Adobe commerce Cloud Professional Services. An Award-Winning Adobe Commerce (Magento) agency with 50+ certified developers with end-to-end solutions customized to meet your needs| Houston | Austin | Dallas | San Antonio - DESSS

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Fwd: Urgent requirements on Corp to Corp with one of Client.

New Post has been published on https://www.hireindian.in/fwd-urgent-requirements-on-corp-to-corp-with-one-of-client-4/

Fwd: Urgent requirements on Corp to Corp with one of Client.

Hello  

    Hope you are doing well!!

  This is Mike from Vinsys Information Technology. We have some opportunities on C2C with one of our client. Please go through the below mentioned Requirements and Please share your updated Resume to mike@vinsysinfo.com. Or please call me on 703-349-3271 to discuss more about this position.

    Sr. No

Job Title

Location

1

TM1 Developer

North Wales, PA

2

Technical writer Information Technology/ Information Security

San Antonio, TX

3

Sr TIBCO BW developer

Atlanta, GA

4

LSF Linux Admin

Austin, TX

5

Drupal Technical Lead

Fort Worth, TX

6

Wonderware Consultant

Hilmar, CA

7

Sr. developer – JDA TMS

Nashville, TN/ Remote

8

Adobe AEM Sr. Technical Lead

Rosemont, IL

9

Ecommerce Solution Architect

Rosemont, Chicago, IL

10

Senior Tandem Lead

Phoenix, Arizona (Tempe)

11

Lead-Peoplesoft, Alfresco ,ApI & Manual Testing

Rosemont, IL

12

Systems Analyst or Product Owner

Bellevue/Bothell, WA

13

AEM Developer

SFO, CA

14

AEM Senior developer/ Lead

SFO, CA

15

Devops and Build engineer

Bothell, Washington

16

BI Developer

Lansing, MI

17

Cust Exp Platform BA

Lansing, MI

18

Cust Exp Platform Developer

Lansing, MI

19

Digital Exp App Support Developer

Lansing, MI

20

Platform Administrator App Support Developer

Lansing, MI

21

Business Analyst

Lansing, MI

22

Document Management Scrum Master

Lansing, MI

23

BA CUM PROJECT MANAGER (10+ Years)

REDMOND, WA

24

Technical Product Owner with API/ Microservices

Atlanta, GA

25

ReactJS developer with Java

REDMOND, WA

26

Sr Springboot Developer

Bellevue, WA

27

Java Solution Architect

Bothell, Bellevue, WA

28

EDI developer

Rosemont, IL

29

UI Developer

San Diego, CA

30

Drupal Architect

Fort Worth, TX

31

Java Lead

San Diego, CA

32

Pega DSA

Kansas City, Kansas

33

NFT Architect

Celebration, FL

34

Technical Lead – Web methods

Framingham, MA

35

Commerce Architect

Philadelphia, PA

36

Informix DBA

Dallas TX

37

Magento Developer

Coppell , TX

38

Tech Lead – SSIS

Milford, CT

39

Simcorp Developer

Arlington, VA

40

HR Technical Resource with EBS (Oracle EBS with PL/SQL experience)

Arlington, VA

41

.Net Programmer

Nashville, TN

42

MS Dynamics

New York

43

BPC Developer

Universal City, CA

44

System Support Analyst

Sunnyvale, CA

45

Mulesoft and Jitter bit LEAD

SFO, CA

46

Sr TIBCO Business Analyst with WSDL, XSD, UML  

Atlanta, GA

47

MSBI DEVELOPER With Power BI (Junior)

Seattle, WA

48

Java Support Engineer

Framingham, MA

        Thanks & Regards,

  Mike Tye (Ravikant)

Talent Acquisition Team – North America

Vinsys Information Technology Inc

SBA 8(a) Certified, MBE/DBE/EDGE Certified

Virginia Department of Minority Business Enterprise(SWAM)

703-349-3271

mike@vinsysinfo.com

www.vinsysinfo.com

https://www.linkedin.com/in/ravikant-mike-tye-janawadkar-809181122/

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Search for Dar VPN router  k Matter Reveals First Hint of WIMP

www.inhandnetworks.com

The Cryogenic Dark Matter Search (CDMS) experiment is one of several major international collaborations that has been searching for dark matter since 2003. The experiment uses very sophisticated detector technology and advanced analysis techniques to enable cryogenically cooled (almost absolute zero temperature at -460 degrees F) germanium and silicon targets to search for the rare recoil of dark matter particles.

SuperCDMS researchers have for the first time observed a concrete hint of a weakly interacting massive particle (WIMP), the particle physicists belie industrial IoT router  ve to be behind dark matter.

College Station — An international collaboration whose search for dark matter is powered by detectors being fabricated at Texas A&M University has for the first time observed a concrete hint of what physicists believe to be the particle behind dark matter and therefore nearly a quarter of the universe — a WIMP, or weakly interacting massive particle.

Scientists with the international Super Cryogenic Dark Matter Search (SuperCDMS) experiment involving Texas A&M high-energy physicist Rupak Mahapatra are reporting a WIMP-like signal at the 3-sigma level, indicating a 99.8 percent chance — or, in high-energy parlance, a hint of the mysterious substance dark matter that is believed to hold the cosmos together but to date has never been directly observed.

“In high-energy physics, a discovery is only claimed at 5-sigma or better,” Mahapatra said. “So this is certainly very exciting, but not fully convincing by the standards. We just need more data to be sure. For now, we have to live with this tantalizing hint of one of the biggest puzzles of our time.”

SuperCDMS researchers are announcing their breakthrough result in talks around the nation, including one at noon today (Monday, April 15) by Mahapatra, a principal investigator in the collaboration and a member of the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy. Mahapatra’s public presentation will be held in the Stephen W. Hawking Auditorium within the Mitchell Institute and streamed live via TTVN. The collaboration has detailed its full results in a paper, Dark Matter Search Results Using the Silicon Detectors of CDMS II, published in arXiv that eventually will appear in Physical Review Letters.

Notoriously elusive, WIMPs rarely interact with normal matter and therefore are difficult to detect. Scientists believe they occasionally bounce off, or scatter like billiard balls from, atomic nuclei, leaving behind a small amount of energy capable of being tracked by detectors deep underground, particle colliders such as the Large Hadron Collider at CERN and even instruments in space like the Alpha Magnetic Spectrometer (AMS) mounted on the International Space Station (ISS).

The CDMS experiment, located a half-mile underground at the Soudan mine in northern Minnesota and managed by the United States Department of Energy’s Fermi National Accelerator Laboratory, has been searching for dark matter since 2003. The experiment uses very sophisticated detector technology and advanced analysis techniques to enable cryogenically cooled (almost absolute zero temperature at -460 degrees F) germanium and silicon targets to search for the rare recoil of dark matter particles.

Mahapatra says the latest analysis represents comprehensive data gleaned from the largest exposure with silicon detectors during the CDMS-II operation, an earlier phase of the overall experiment involving more than 50 scientists from 18 international institutions.

“This result is from data taken a few years ago using silicon detectors manufactured at Stanford that are now defunct,” Mahapatra said. “Increased interest in the low mass WIMP region motivated us to complete the analysis of the silicon-detector exposure, which is less sensitive than germanium for WIMP masses above 15 giga-electronvolts [one GeVa is equal to a billion electron volts] but more sensitive for lower masses. The analysis resulted in three events, and the estimated background is 0.7 events.”

In addition to being heavily involved in the data analysis, Mahapatra says the Texas A&M group performed the crucial calibration of the silicon detectors, guaranteeing that the signal would look the same, regardless in which of the eight detectors located within the mine it might appear.

While Mahapatra says Monte Carlo simulations weren’t able to rule out statistical fluctuations as the cause of the backgrounds, the team believes said fluctuations would rarely produce a similar energy distribution, which they interpret instead as spin-independent scattering of WIMPs. And although he says the result is certainly encouraging and worthy of further investigation, he cautions it should not be considered a discovery.

“We are only 99.8 percent sure, and we want to be 99.9999 percent sure,” Mahapatra said. “At 3-sigma, you have a hint of something. At 4-sigma, you have evidence. At 5-sigma, you have a discovery.

“In medicine, you can say you are curing 99.8 percent of the cases, and that’s OK. When you say you’ve made a fundamental discovery in high-energy physics, you can’t be wrong. Given the money involved — $30 million in this case — it has to be extremely precise. With a 99.8 percent chance, that means if you repeated the same experiment a few hundred times, there is one chance it can go wrong. We want one out of a million instead.”

Using germanium detectors, the collaboration previously in 2010 reported detection of two events in the signal region and an estimated background of 0.9 events. They eventually concluded these events more likely were attributable to leakage of surface electrons rather than actual nuclear recoils.

6-inch detectors also being test-fabricated in Mahapatra’s lab for the Generation 3 (G3) experiments expected in a few years. These novel silicon detectors represent a world-first in cryogenic detection and are approximately 30 times more sensitive than the individual silicon detectors behind the SuperCDMS collaboration’s latest result.

For the past four years, Mahapatra and his Texas A&M team — which includes his Department of Physics and Astronomy-based research group as well as collaborator Rusty Harris in the Department of Electrical Engineering — have been developing the larger, more advanced detectors needed for the project’s current phases, from SuperCDMS to the even more sophisticated GEODM (Germanium Observatory for Dark Matter) experiments. They are developing both germanium and silicon detectors to create dual-threat devices that are much bigger, better and cheaper. He notes his laboratory’s new 6-inch diameter silicon detectors represent a world-first in cryogenic detection and are approximately 30 times more sensitive than the individual silicon detectors behind this latest result.

“The industrial manufacturing and fabrication facility we have set up here at Texas A&M has enabled us to bring down the cost from $350,000 per kilogram to about $40,000 per kilogram,” Mahapatra said. “We also have a 90 percent success rate, versus the previous 20 percent rate for the original silicon and germanium devices.”

Mahapatra says the collaboration will continue to probe this WIMP  Vending Telemeter  sector using the SuperCDMS Soudan experiment’s operating germanium detectors and is considering using silicon detectors in future experiments.

The collaboration’s work — beginning with CDMS and CDMS-II and continuing with SuperCDMS and GEODM — is funded by the DOE and the National Science Foundation as well as the Natural Sciences and Engineering Research Council of Canada (NSERC).

“In addition to NSF funding and an early career research award from the DOE, this work would not have been possible without start-up support from Texas A&M University and the College of Science and roughly $2 million in equipment from Maximum Integrated Products, Inc. (NASDAQ: MXIM) in Dallas,&rdqu touchscreen vending  o; Mahapatra said. “Additionally, the Mitchell Institute funds the postdoctoral fellow, Joel Sander, who is spearheading the effort to develop alternate next-generation detectors that are not only another order of magnitude cheaper and but can also run at easier cryogenic temperature, which is ideal for a ton-scale experiment on budget. The goal of this funding was to take up high-risk, high-return research that normally does not get supported by traditional funding from federal funding agencies like DOE and NSF.”

For more information on the Super Cryogenic Dark Matter Search Experiment, go to .

Paper: Dark Matter Search Results Using the Silicon Detectors of CDMS II Paper: Silicon Detector Results from the First Five-Tower Run of CDMS II

Image: Texas A&M University

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