et-gw.eu

physics.gla.ac.uk

University of Glasgow :: Schools :: School of Physics and Astronomy :: Institute for Gravitational Research - Speedmeter

http://www.physics.gla.ac.uk/igr/speedmeter

Skip to main content. School of Physics and Astronomy. Institute for Gravitational Research. Welcome to the ERC Sagnac Speed-Meter Project. This project has received funding from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no. 307245. This website is meant to provide information on the European Research Council. At the University of Glasgow. In this project we aim to answer questions like:. Or future upgrades to LIGO.

grawiton-gw.eu

Supervisory Board

http://www.grawiton-gw.eu/index.php/supervisoryboard

Jump to main navigation and login. Jump to additional information. GraWIToN Early Stage Researchers. ITN in FP7 Marie Curie Actions. Michele Punturo (Project Coordinator). Elena Cuoco (Scientific Coordinator). Eugenio Coccia (INFN) (LAS sub-programme Coordinator). Andreas Freise (UoB) (SIM sub-programme Coordinator). Sheila Rowan (UGLA) (OPT sub-programme Coordinator). Benno Willke (LUH) (HPL sub-programme Coordinator). Erika Morucci (EGO Secretariat). Second GW signal detected! Yes, we did it again!

fiontar.co.uk

Technical Notes | Fiontar

http://www.fiontar.co.uk/archives/1401

Technical Consulting; Antique Scientific Instruments; Sundials. The technical world is abuzz with the plethora of large scale telescopes coming over the horizon in the wake of the Hubble Space Telescope’s success (once the right unit system was in use). The Giant Magellan Telescope ( GMT. Is scheduled to be fully up and working in Chile’s Atacama Desert by 2024 and will be the world’s largest optical telescope. The even larger proposed $1.4bn optical Thirty Metre Telescope ( TMT. Australia used in the se...

edgeofphysics.com

News from the Frontiers of Cosmology: A companion to the book The Edge of Physics — The Edge of Physics Blog

http://edgeofphysics.com/blog

The Edge of Physics Blog. News from the Frontiers of Cosmology: A companion to the book The Edge of Physics. Want to go underground to build a sensitive observatory capable of detecting gravitational waves that are thought be generated when black holes merge. The “Einstein Observatory” will 100 times more sensitive than existing detectors, and will likely be able to detect gravitational waves generated just after the Big Bang. Already, the next generation of detectors, such as Advanced LIGO. If such an i...

gw-models.org

GW-models

http://www.gw-models.org/links/index.php

Software and Data for Modeling and Analysing Gravitational Waveforms from Compact Binaries. Our phenomenological waveform models are used for analysing data of the LIGO. Detectors, and for the design of future detectors like ET. Numerical INJection Analysis (NINJA) Project. Addressing the spin question. Modeling waveforms of compact binary coalescences. Tracking the precession of binary black holes. The NINJA2 Waveform Model Data Set.

gwic.ligo.org

GWIC - The Gravitational Wave International Committee

https://gwic.ligo.org/members

Member Projects and Representatives. Sheila Rowan, University of Glasgow, (GWIC, 2009- , Chair 2015- ). Bram Slagmolen, Australian National University, 2015-. Massimo Cerdonio, University of Padua and. Michele Punturo, INFN-Perugia, 2009-. European Pulsar Timing Array (EPTA). Michael Kramer, Max-Planck-Institut für Radioastronomie and Jodrell Bank Centre for Astrophysics (University of Manchester), 2009-. Karsten Danzmann, Albert-Einstein-Institut fur Gravitationsphysik and University of Hannover, 1997-.

geo600.org

Links | GEO 600 Portal

http://www.geo600.org/6400/Links

Skip to navigation (Press Enter). Skip to main content (Press Enter). GEO High Frequency and Squeezing. Press and Public Outreach. Science for the public. Other existing or planned laser interferometric gravitational wave detectors. The US project: 4 km, two detectors. The French-Italian project: 3 km. Evolved Laser Interferometer Space Antenna. The LISA International Science Community. The planned cryogenic Japanese detector (l = 3 km), located in the Kamioka mine. The Rome Gravitational Wave Group.

coirich.com

Charmant Project | CoIRICH – Consortium of Italian Research Infrastructure for Cultural Heritage

http://www.coirich.com/index.php/charmant-project

The former, a Roman age villa, is recognized as a key site for a thorough cultural understanding of the ancient world, mostly due to its wide library. The latter, and most demanding site, is the key to solve, by archaeo-DNA retrieval and analysis, the still unanswered question on the origin of the Sumerian population. The CHARMANT Synergistic Team. ORNL UT Batelle, US). SNS, ORNL UT Batelle, US). Università di Roma Tre). ISIS Pulsed Neutron Source, UK). Archeologica del Lazio), F. D’Agostino. K L Kvamme,.

grawiton-gw.eu

Job Opportunities

http://www.grawiton-gw.eu/index.php/jobopportunities

Jump to main navigation and login. Jump to additional information. GraWIToN Early Stage Researchers. ITN in FP7 Marie Curie Actions. Deadlines: closed for all positions. Project Recruitment Advertisement materials (Archive):. Download the recruitment poster here. Some websites where Beneficiaries published their vacancies:. Http:/ ec.europa.eu/euraxess/index.cfm/jobs/index. Http:/ www.findaphd.com/. Http:/ www.iop.org/. Http:/ www.jobs.ac.uk/. Second GW signal detected! Yes, we did it again!

grawiton-gw.eu

Image Collections

http://www.grawiton-gw.eu/index.php/imagecollections

Jump to main navigation and login. Jump to additional information. GraWIToN Early Stage Researchers. 1st Basic School Pictures. Images of the 2nd SB meeting (Birmingham, 2014). GSSI Academic year inauguration (L'Aquila, 2014). Solar eclipse seen from GSSI (L'Aquila, 2015). Outreach: La scienza è donna (Pisa, June 2015). 2nd GraWIToN School Pictures. Third GraWIToN School pictures. President of the Council of ministers of the Italian Republic, Matteo Renzi, visits GSSI (L'Aquila - February 22, 2016).