Becoming-Artwork: Rethinking Agency and Performativity Through the Conservation History of Rembrandt's The Night Watch (1642)

This thesis stems from the mainstream notion that art conservation is a practice that stabilizes objects with well-defined properties, and it argues that idea is complexified when conservation practices are studied attentively. By considering concepts from new materialism – specifically becoming, agency and performativity – this analysis looks closely at the long conservation history of Rembrandt van Rijn’s canonical painting The Night Watch (1642), to center on the ontological tensions between states of change and permanency in which the painting comes to be. With a focus on process and materiality, this thesis begins with a historiographical exploration of the object in conservation theories, ranging from a positivist understanding of the work of art as a single object with defined physical properties, to a more constructivist definition, where the art object is understood as a multiplicity of forces. The text proceeds to introduce The Night Watch as an entity that transits between temporal ontologies of change and permanency, thus destabilizing its identity as a single artwork, positing it, rather, as an entity in transition, a becoming-object. Framing Rembrandt’s painting as process poses the question of who and what agents co-produce this process. Agency is demonstrated to be distributed amongst the artist, the materials of the painting itself, the conservators, and the technologies used in preservation practices: all forces that interact and mobilize one another in the process of materialization of The Night Watch. Accounting for the boundaries of The Night Watch not as fixed, but as being materialized, forces us to account for the practices – repetitions of doings – that perform those boundaries in the first place. The research and conservation project of the painting, Operation Night Watch, currently ongoing at the Rijksmuseum, displays all these agencies at play at the museum’s gallery. Understanding artworks as process ultimately has consequences not only for how an artwork is perceived, as fixed and eternal, but also for conservation ethics

The Structure and Star-Formation History of NGC 5461

We compute photoionization models for the giant extragalactic H II region NGC 5461, and compare their predictions to several observational constraints. Since we aim at reproducing not only the global properties of the region, but its local structure also, the models are constrained to reproduce the observed density profile, and our analysis takes into consideration the bias introduced by the shapes and sizes of the slits used by different observers. We find that an asymmetric nebula with a gaussian density distribution, powered by a young burst of 3.1 Myr, satisfactorily reproduces most of the constraints, and that the star-formation efficiency inferred from the model agrees with current estimates. Our results strongly depend on the assumed density law, since constant density models overestimate the hardness of the ionizing field, affecting the deduced properties of the central stellar cluster. We illustrate the features of our best model, and discuss the possible sources of errors and uncertainties affecting the outcome of this type of studies.Comment: 33 pages (LaTeX), 3 .eps figures. to be published in ApJ, May 200

Bright Stars and Recent Star Formation in the Irregular Magellanic Galaxy NGC2366

The stellar content of the Im galaxy NGC 2366 is discussed on the basis of CCD BVR photometry. The three brightest blue and red stars have been used to estimate its distance, obtaining a balue of 2.9 Mpc. The spatial distribution of the young stellar population is discussed in the light of the integrated color indices and the color-magnitude diagrams of different zones of the galaxy. A generalized star formation burst seems to have taken place about 50 Myr ago. The youngest stars are preferentially formed in the South-West part of the bar, where the giant HII complex NGC 2363 is located, being younger and bluer. The bar seems to play a role favouring star formation in one of its extremes. Self-propagation however, does not seem to be triggering star formation at large scale. A small region, populated by very young stars has also been found at the East of the galaxy.Comment: Astronomical Journal, accepted. This is a uuencoded, compressed, tar file (102 Kbytes) of 1 text, 1 table postscript files. Figures are retrieved as a separate file. One single file with all figures and tables (552Kb) also available from http://www.ast.cam.ac.uk/~etelles/astronomy.htm

Estudio teórico y experimental del sistema 9 Be + 51 V y sistemas similares

En este trabajo de tesis se presenta el estudio sistemático de los sistemas 7Li + 51V, 9Be + 51V y 8B + 58Ni. Para los sistemas ( 7Li, 9 Be) + 51V se midieron las secciones eficaces de fusión a energías cercanas a la barrera Coulombiana (EB,lab=11.75 y 16.16 MeV, respectivamente) empleando la técnica de rayos γ. El experimento para medir la fusión se llevó a cabo en el Laboratorio del Acelerador Tan- dem, del Instituto Nacional de Investigaciones Nucleares (ININ), siendo éstas las primeras mediciones realizadas para estos proyectiles a las energías consideradas. De forma simultánea, se hizo el análisis de los posibles núcleos residuales usando los códigos computacionales de fusión-evaporación PACE2, LILITA y CASCADE. Los resultados obtenidos fueron comparados con los datos experimentales me- didos. De forma preliminar, para el sistema 7Li + 51V, se hicieron cálculos usando la teoría de canales acoplados de reacción para estimar la contribución de la sección eficaz de transferencia de un protón a la producción del núcleo residual 52Cr. Para el sistema 8B + 58Ni, se hizo un análisis teórico de canales acoplados con el continuo discretizado y canales acoplados de reacción para estudiar los procesos de rompimiento y de transfe- rencia de un protón, 58Ni(8B,7Be)59Cu, a energías alrededor de la barrera Coulombiana (EB,lab=22.95 MeV). Para calcular las secciones eficaces correspondientes se usó un potencial de Modelo Óptico se- mimicroscópico, el cual combina un potencial real de doble convolución, un potencial de polarización y un potencial imaginario tipo Woods-Saxon. A partir de la comparación de nuestros cálculos con datos experimentales se determinaron los factores espectroscópicos Sexpt y astrofísicos S17(0) del protón en la interacción 8B → 7Be+p

Constraints on the χ_(c1) versus χ_(c2) polarizations in proton-proton collisions at √s = 8 TeV

The polarizations of promptly produced χ_(c1) and χ_(c2) mesons are studied using data collected by the CMS experiment at the LHC, in proton-proton collisions at √s=8  TeV. The χ_c states are reconstructed via their radiative decays χ_c → J/ψγ, with the photons being measured through conversions to e⁺e⁻, which allows the two states to be well resolved. The polarizations are measured in the helicity frame, through the analysis of the χ_(c2) to χ_(c1) yield ratio as a function of the polar or azimuthal angle of the positive muon emitted in the J/ψ → μ⁺μ⁻ decay, in three bins of J/ψ transverse momentum. While no differences are seen between the two states in terms of azimuthal decay angle distributions, they are observed to have significantly different polar anisotropies. The measurement favors a scenario where at least one of the two states is strongly polarized along the helicity quantization axis, in agreement with nonrelativistic quantum chromodynamics predictions. This is the first measurement of significantly polarized quarkonia produced at high transverse momentum