High-precision transit observations of the exoplanet WASP-13b with the RISE instrument

WASP-13b is a sub-Jupiter mass exoplanet orbiting a G1V type star with a period of 4.35 d.The current uncertainty in its impact parameter (0 < b < 0.46) results in poorly definedstellar and planetary radii. To better constrain the impact parameter, we have obtained highprecisiontransit observations with the rapid imager to search for exoplanets (RISE) instrumentmounted on 2.0-m Liverpool Telescope. We present four new transits which are fitted witha Markov chain Monte Carlo routine to derive accurate system parameters. We found anorbital inclination of 85. ◦ 2 ± 0. ◦ 3 resulting in stellar and planetary radii of 1.56 ± 0.04 Rand 1.39 ± 0.05RJup, respectively. This suggests that the host star has evolved off the mainsequence and is in the hydrogen-shell-burning phase.We also discuss how the limb darkeningaffects the derived system parameters.With a density of 0.17ρJ,WASP-13b joins the group oflow-density planets whose radii are too large to be explained by standard irradiation models.We derive a new ephemeris for the system, T0 = 245 5575.5136 ± 0.0016 (HJD) and P =4.353 011 ± 0.000 013 d. The planet equilibrium temperature (Tequ = 1500 K) and the brighthost star (V = 10.4mag) make it a good candidate for follow-up atmospheric studies.

The Next Generation Transit Survey (NGTS)

The Next Generation Transit Survey (NGTS) is a new ground-based sky survey designed to find transiting Neptunes and super-Earths. By covering at least sixteen times the sky area of Kepler we will find small planets around stars that are sufficiently bright for radial velocity confirmation, mass determination and atmospheric characterisation. The NGTS instrument will consist of an array of twelve independently pointed 20cm telescopes fitted with red-sensitive CCD cameras. It will be constructed at the ESO Paranal Observatory, thereby benefiting from the very best photometric conditions as well as follow up synergy with the VLT and E-ELT. Our design has been verified through the operation of two prototype instruments, demonstrating white noise characteristics to sub-mmag photometric precision. Detailed simulations show that about thirty bright super-Earths and up to two hundred Neptunes could be discovered. Our science operations are due to begin in 2014.

Transit timing variations in WASP-10b induced by stellar activity

The hot-JupiterWASP-10bwas reported by Maciejewski et al. to showtransit timing variations (TTVs) with an amplitude of ~3.5 min. These authors proposed that the observed TTVs were caused by a 0.1M_Jup perturbing companion with an orbital period of ~5.23 d, and hence, close to the outer 5:3 mean-motion resonance with WASP-10b. To test this scenario, we present eight new transit light curves of WASP-10b obtained with the Faulkes Telescope North and the Liverpool Telescope. The new light curves, together with 22 previously published ones, were modelled with a Markov Chain Monte Carlo transit fitting code. Transit depth differences reported forWASP-10b are thought to be due to starspot-induced brightness modulation of the host star. Assuming the star is brighter at the activity minimum, we favour a small planetary radius. We find Rp = 1.039^+0.043 _-0.049R_Jup in agreement with Johnson et al. and Maciejewski et al. Recent studies find no evidence for a significant eccentricity in this system. We present consistent system parameters for a circular orbit and refine the orbital ephemeris ofWASP-10b. Our homogeneously derived transit times do not support the previous claimed TTV signal, which was strongly dependent on two previously published transits that have been incorrectly normalized. Nevertheless, a linear ephemeris is not a statistically good fit to the transit times of WASP-10b. We show that the observed transit time variations are due to spot occultation features or systematics. We discuss and exemplify the effects of occultation spot features in the measured transit times and show that despite spot occultation during egress and ingress being difficult to distinguish in the transit light curves, they have a significant effect in the measured transit times. We conclude that if we account for spot features, the transit times of WASP-10b are consistent with a linear ephemeris with the exception of one transit (epoch 143) which is a partial transit. Therefore, there is currently no evidence for the existence of a companion to WASP-10b. Our results support the lack of TTVs of hot-Jupiters reported for the Kepler sample. 

Aristarchos RISE2: A Wide-Field Fast Imager for Exoplanet Transit Timing

The detection of exoplanets is currently of great topical interest in astronomy. The Rapid Imager for Surveys of Exoplanets 2 (RISE2) camera will be built for exoplanet studies and in particular for detection of transit timing variations (TTV) induced by the presence of a third body in the system. It will be identical to RISE which has been running successfully on the 2m Liverpool Telescope since 2008 but modified for the 2.3m ARISTARCHOS telescope. For TTV work the RISE/LT combination is regularly producing timings with accuracy <10 seconds making it the best suited instrument for this work. Furthermore, RISE2/AT has the added benefit of being located at a significantly different longitude to the LT/RISE on La Palma, hence extending the transit coverage.

Transit Observations of the Hot Jupiter HD 189733b at X-Ray Wavelengths

We present new X-ray observations obtained with Chandra ACIS-S of the HD 189733 system, consisting of a K-type star orbited by a transiting Hot Jupiter and an M-type stellar companion. We report a detection of the planetary transit in soft X-rays with a significantly deeper transit depth than observed in the optical. The X-ray data favor a transit depth of 6%-8%, versus a broadband optical transit depth of 2.41%. While we are able to exclude several possible stellar origins for this deep transit, additional observations will be necessary to fully exclude the possibility that coronal inhomogeneities influence the result. From the available data, we interpret the deep X-ray transit to be caused by a thin outer planetary atmosphere which is transparent at optical wavelengths, but dense enough to be opaque to X-rays. The X-ray radius appears to be larger than the radius observed at far-UV wavelengths, most likely due to high temperatures in the outer atmosphere at which hydrogen is mostly ionized. We furthermore detect the stellar companion HD 189733B in X-rays for the first time with an X-ray luminosity of log LX = 26.67 erg s-1. We show that the magnetic activity level of the companion is at odds with the activity level observed for the planet-hosting primary. The discrepancy may be caused by tidal interaction between the Hot Jupiter and its host star.

Spatial distribution of plastic pollutants in a transit from Puget Sound to outside Nootka Sound Canada

Senior thesis written for Oceanography 445

An accessibility planning tool for network transit oriented development : SNAP

In the academic debate regarding the influences between urban form, built environment and travel patterns, a specific idea that has taken hold is that more compact urban development around railway stations, often referred to as Transit Oriented Development (TOD), contributes to the control of vehicle travel and to more sustainable metropolitan systems. According to this general principle this work proposes a GIS accessibility tool for the design of polycentric transit oriented scenario: SNAP - Station Network Accessibility Planning tool. In the first part the state of the art on Transit Oriented Development policies in Europe is presented with a focus on three study cases. In the second part the SNAP tool is described, with remarks to the approach, the methodology and the used indicators. Furthermore the paper discusses an application to the metropolitan area of Naples.

A minor theory of the transit of materiality into discourse, Via Campesina.

In this thesis I explore how the material properties of plant seed enter the political discourses of the international peasant coalition the Via Campesina and coalition member the National Fanners Union of Canada (NFU), querying how this process might be employed as a resource for a transformative eco-social politics. I employ several post-structural theoretical constructs, configuring them together as a "minor theory". This minor theory provides the basis for a "minor" reading of three sets of Via Campesina and NFU texts. The aim of these readings is to track the movement of seed from a local agricultural concern to a transitive political one, across both the material and discursive registers. In surfacing the presence of the seed's physical properties in the three texts, I highlight the distinctions between the constraining seed of corporate industrial agriculture, and the social and agroecological opportunities resulting from what I call a "Seed Event".

Personal soundtracks on public transit : personal listening devices and socio-spatial negotiations of students' bus journeys

One way of exploring the power of sound in the experience and constitution of space is through the phenomenon of personal listening devices (PLDs) in public environments. In this thesis, I draw from in-depth interviews with eleven Brock University students in S1. Catharines, Ontario, to show how PLDs (such as MP3 players like the iPod) are used to create personalized soundscapes and mediate their public transit journeys. I discuss how my interview participants experience the space-time of public transit, and show how PLDs are used to mediate these experiences in acoustic and non-acoustic ways. PLD use demonstrates that acoustic and environmental experiences are co-constitutive, which highlights a kinaesthetic quality of the transit-space. My empirical findings show that PLDs transform space, particularly by overlapping public and private appropriations of the bus. I use these empirical findings to discuss the PLD phenomenon in the theoretical context of spatiality, and more specifically, acoustic space. J develop the ontological notion of acoustic space, stating that space shares many of the properties of sound, and argue that sound is a rich epistemological tool for understanding and explaining our everyday experiences.

Models and algorithms for transit network planning.

Tesis (Doctor en Ingeniería con Especialidad en Ingeniería de Sistemas) UANL, 2012.

Décliner la frontière : transit et contagion de la violence dans la fiction sacrificielle de Bernard-Marie Koltès

Ce mémoire de maîtrise traite de quatre pièces de l’auteur français Bernard-Marie Koltès. Résolument axé sur l’étude du texte écrit, il vise dans un premier temps l’analyse d’un ensemble de désajustements et d’une culture de l’équivoque dans le traitement du lieu, du temps et de l’identité. Le premier but de ces analyses est l’approfondissement de certaines avenues déjà investies par la critique (marginalité des lieux et des personnages, présence constante de la violence et de la mort, etc.), dans la recherche d’une signification globale à un ensemble de pratiques textuelles liées à la notion de limite ou de frontière. Opérant un changement de perspective, la seconde partie de l’étude s’attarde à la violence ainsi qu’aux modalités et implications de sa mise en texte dans une étude croisée de l’acte créateur et de la pratique de lecture. À partir de la théorie du sacrifice élaborée par René Girard dans La violence et le sacré, et faisant dialoguer certains textes importants d’auteurs divers (Aristote, Nietzsche, Artaud, Foucault, Derrida et Adorno), l’analyse vise à inscrire la littérarité du texte koltésien dans une entreprise plus vaste ayant à voir avec la violence, sa régulation et sa diffusion. Au carrefour des études théâtrales, de la littérature et de la philosophie, cette réflexion cherche à concevoir le théâtre de Koltès (particulièrement Roberto Zucco) comme un sacrifice rituel, afin de mieux en comprendre le rapport au réel et certaines de ses particularités du point de vue du mécanisme cathartique.

Assessing the impact of the Canadian tax credit for public transit passes.

Rapport de recherche présenté à la Faculté des arts et des sciences en vue de l'obtention du grade de Maîtrise en sciences économiques.

Standardisation de l’aménagement d’une unité d’endoscopie : Aires de transit des équipements biomédicaux

Rapport de projet

La planification métropolitaine et le transit-oriented development (TOD) : les nouveaux instruments de la gouvernance du Grand Montréal

Cette thèse croise les concepts de planification, de gouvernance et de transit-oriented development (TOD) par une étude de la production, de la mise en débat et de l'adoption du plan métropolitain d'aménagement et de développement (PMAD) de la Communauté métropolitaine de Montréal (CMM). Elle expose les résultats de quatre années de recherche qualitative sur les impacts de l'épisode du PMAD et de la stratégie TOD de la CMM sur les pratiques planificatrices et les processus décisionnels du Grand Montréal à l'échelle métropolitaine. Elle révèle que la planification métropolitaine et l'objectif de coordination du transport et de l'aménagement en général ainsi que le PMAD et le concept de TOD en particulier y sont des instruments de gouvernance. Les chapitres 2, 3 et 4 présentent la problématique, le terrain d'enquête et la démarche méthodologique de cette recherche. Le chapitre 5 relate l'épisode du PMAD en analysant son contenu, les procédures par lesquelles la CMM l'a produit, mis en débat et adopté, les réactions des parties prenantes de la région quant à ces aspects et la façon dont elles comptent assurer le suivi de sa mise en œuvre. Le chapitre 6 illustre comment cet épisode a fait du PMAD un instrument de gouvernance pour le Grand Montréal en décortiquant le rôle de la participation publique, des médias, des acteurs des milieux régional et local, des élus, de la CMM et de la société civile de la région au sein de ce processus de changement de registre de la planification et de la gouvernance les déployant sur des bases plus stratégiques et collaboratives. Le chapitre 7 montre que cet épisode a aussi fait du TOD un instrument de gouvernance pour le Grand Montréal en détaillant les tenants et aboutissants du processus d'appropriation, de marchand(is)age et d'instrumentalisation du concept par les élites politiques et techniques à des fins de marketing territorial et de construction de capital politique ouvrant la voie à la stabilisation d'une gouvernance en matière d'aménagement métropolitain. Il se dégage de cette thèse que ces profondes transformations que subissent actuellement la planification et la gouvernance exacerbent le caractère symbiotique de la relation qui les unit.