OA platinum, Projektname: NoVaMigra - Norms and Values in the European Migration and Refugee Crisis
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doi: 10.5445/ir/1000075998 , 10.48550/arxiv.1710.05833 , 10.18154/rwth-2017-10115 , 10.5445/ir/1000075998#verlagsausgabe , 10.18154/rwth-2017-10236 , 10.3204/pubdb-2017-12237
handle: 2318/1653088 , 1854/LU-8620611 , 20.500.11767/115369 , 20.500.11769/316953 , 1871.1/bca5efec-b61f-4887-b4f2-52213171a5a3 , 11585/618379 , 11587/417079 , 11391/1420862 , 11589/116039 , 11570/3210319 , 11591/464238 , 11311/1042230 , 11568/887847 , 11567/886113 , 11392/2495371 , 11581/405220 , 11584/370053 , 11573/1073679 , 11386/4720763 , 11368/2921588 , 11577/3268750 , 11576/2650552 , 20.500.11820/563466b8-dd95-441f-991a-57f2dda0430b , 21.11116/0000-0000-6274-F , 21.11116/0000-0000-6276-D , 21.11116/0000-0002-6398-3 , 21.11116/0000-0002-639A-1 , 11365/1073284 , 2434/533899
doi: 10.5445/ir/1000075998 , 10.48550/arxiv.1710.05833 , 10.18154/rwth-2017-10115 , 10.5445/ir/1000075998#verlagsausgabe , 10.18154/rwth-2017-10236 , 10.3204/pubdb-2017-12237
handle: 2318/1653088 , 1854/LU-8620611 , 20.500.11767/115369 , 20.500.11769/316953 , 1871.1/bca5efec-b61f-4887-b4f2-52213171a5a3 , 11585/618379 , 11587/417079 , 11391/1420862 , 11589/116039 , 11570/3210319 , 11591/464238 , 11311/1042230 , 11568/887847 , 11567/886113 , 11392/2495371 , 11581/405220 , 11584/370053 , 11573/1073679 , 11386/4720763 , 11368/2921588 , 11577/3268750 , 11576/2650552 , 20.500.11820/563466b8-dd95-441f-991a-57f2dda0430b , 21.11116/0000-0000-6274-F , 21.11116/0000-0000-6276-D , 21.11116/0000-0002-6398-3 , 21.11116/0000-0002-639A-1 , 11365/1073284 , 2434/533899
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim$1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg$^2$ at a luminosity distance of $40^{+8}_{-8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Msun. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim$40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over $\sim$10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position $\sim$9 and $\sim$16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. (Abridged) The astrophysical journal / 2 848(2), L12 (2017). doi:10.3847/2041-8213/aa91c9 Published by IOP Publ., London
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Fieldwork was conducted in selected migration arrival ports in Greece, Italy, Spain, France, South Africa, and Canada to explore the role of the notion of vulnerability in the field level governance of international protection. Specifically, we explored how key actors and stakeholders in the selected field sites 1) understood and applied notions of vulnerability, and 2) collaborated to address and reduce vulnerabilities.
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Olioso A., Gallego-Elvira B., Bahir M., Boulet G., Weiss M., Mira M., Castillo-Reyes S., 2015. EVASPA : EVapotranspiration Assessment from SPAce. Workshop modélisation de surface, 30 nov-1 dec 2015, CESBIO (salle de conférence du CESBIO), Toulouse. [Présentation orale par A. Olioso]. National audience
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doi: 10.18154/rwth-2017-07572 , 10.18154/rwth-2016-08778 , 10.48550/arxiv.1602.08772 , 10.5445/ir/1000059701
handle: 2318/1639269 , 1854/LU-8523193 , 2158/1115254 , 11585/593440 , 11384/66510 , 11391/1404531 , 11568/840776 , 11567/840036 , 11584/289379 , 11573/899029 , 11577/3239738 , 11449/165260 , 10067/1392540151162165141 , 10446/142678 , 10281/153147
doi: 10.18154/rwth-2017-07572 , 10.18154/rwth-2016-08778 , 10.48550/arxiv.1602.08772 , 10.5445/ir/1000059701
handle: 2318/1639269 , 1854/LU-8523193 , 2158/1115254 , 11585/593440 , 11384/66510 , 11391/1404531 , 11568/840776 , 11567/840036 , 11584/289379 , 11573/899029 , 11577/3239738 , 11449/165260 , 10067/1392540151162165141 , 10446/142678 , 10281/153147
Results are reported from a search for supersymmetry with gauge-mediated supersymmetry breaking in electroweak production. Final states with photons and large missing transverse energy ($E_{\mathrm{T}}^{\text{miss}}$) were examined. The data sample was collected in pp collisions at $\sqrt{s} = $ 8 TeV with the CMS detector at the LHC and corresponds to 7.4 fb$^{-1}$. The analysis focuses on scenarios in which the lightest neutralino has bino- or wino-like components, resulting in decays to photons and gravitinos, where the gravitinos escape undetected. The data were obtained using a specially designed trigger with dedicated low thresholds, providing good sensitivity to signatures with photons, $E_{\mathrm{T}}^{\text{miss}}$, and low hadronic energy. No excess of events over the standard model expectation is observed. The results are interpreted using the model of general gauge mediation. With the wino mass fixed at 10 GeV above that of the bino, wino masses below 710 GeV are excluded at 95% confidence level. Constraints are also set in the context of two simplified models, for which the analysis sets the lowest cross section limits on the electroweak production of supersymmetric particles. Results are reported from a search for supersymmetry with gauge-mediated supersymmetry breaking in electroweak production. Final states with photons and large missing transverse energy (MET) were examined. The data sample was collected in pp collisions at sqrt(s) = 8 TeV with the CMS detector at the LHC and corresponds to 7.4 inverse femtobarns. The analysis focuses on scenarios in which the lightest neutralino has bino- or wino-like components, resulting in decays to photons and gravitinos, where the gravitinos escape undetected. The data were obtained using a specially designed trigger with dedicated low thresholds, providing good sensitivity to signatures with photons, MET, and low hadronic energy. No excess of events over the standard model expectation is observed. The results are interpreted using the model of general gauge mediation. With the wino mass fixed at 10 GeV above that of the bino, wino masses below 710 GeV are excluded at 95% confidence level. Constraints are also set in the context of two simplified models, for which the analysis sets the lowest cross section limits on the electroweak production of supersymmetric particles. Results are reported from a search for supersymmetry with gauge-mediated supersymmetry breaking in electroweak production. Final states with photons and large missing transverse energy ( ETmiss ) were examined. The data sample was collected in pp collisions at s=8TeV with the CMS detector at the LHC and corresponds to 7.4 fb−1 . The analysis focuses on scenarios in which the lightest neutralino has bino- or wino-like components, resulting in decays to photons and gravitinos, where the gravitinos escape undetected. The data were obtained using a specially designed trigger with dedicated low thresholds, providing good sensitivity to signatures with photons, ETmiss , and low hadronic energy. No excess of events over the standard model expectation is observed. The results are interpreted using the model of general gauge mediation. With the wino mass fixed at 10 GeV above that of the bino, wino masses below 710 GeV are excluded at 95% confidence level. Constraints are also set in the context of two simplified models, for which the analysis sets the lowest cross section limits on the electroweak production of supersymmetric particles.
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Physics letters / B 829, 137062 (2022). doi:10.1016/j.physletb.2022.137062 Published by North-Holland Publ., Amsterdam