Classical novae from the POINT-AGAPE microlensing survey of M31 - II. Rate and statistical characteristics of the nova population

The POINT-AGAPE (Pixel-lensing Observations with the Isaac Newton Telescope-Andromeda Galaxy Amplified Pixels Experiment) survey is an optical search for gravitational microlensing events towards the Andromeda galaxy (M31). As well as microlensing, the survey is sensitive to many different classes of variable stars and transients. In our first paper of this series, we reported the detection of 20 classical novae (CNe) observed in Sloan r' and i' passbands.

POINT-AGAPE pixel lensing survey of M31 - Evidence for a MACHO contribution to galactic halos

The POINT-AGAPE collaboration is carrying out a search for gravitational microlensing toward M31 to reveal galactic dark matter in the form of MACHOs (Massive Astrophysical Compact Halo Objects) in the halos of the Milky Way and M31. A high-threshold analysis of 3 years of data yields 6 bright, short- duration microlensing events, which are confronted to a simulation of the observations and the analysis. The observed signal is much larger than expected from self lensing alone and we conclude, at the 95% confidence level, that at least 20% of the halo mass in the direction of M31 must be in the form of MACHOs if their average mass lies in the range 0.5-1 M-circle dot. This lower bound drops to 8% for MACHOs with masses similar to 0.01 M-circle dot. In addition, we discuss a likely binary microlensing candidate with caustic crossing. Its location, some 32' away from the centre of M31, supports our conclusion that we are detecting a MACHO signal in the direction of M31.

The POINT-AGAPE survey - II. An unrestricted search for microlensing events towards M31

An automated search is carried out for microlensing events using a catalogue of 44 554 variable superpixel light curves derived from our 3-yr monitoring programme of M31. Each step of our candidate selection is objective and reproducible by a computer. Our search is unrestricted, in the sense that it has no explicit time-scale cut. So, it must overcome the awkward problem of distinguishing long time-scale microlensing events from long-period stellar variables.

Classical novae from the POINT-AGAPE microlensing survey of M31 - I. The nova catalogue

The POINT-AGAPE (Pixel-lensing Observations with the Isaac Newton Telescope-Andromeda Galaxy Amplified Pixels Experiment) survey is an optical search for gravitational microlensing events towards the Andromeda galaxy (M31). As well as microlensing, the survey is sensitive to many different classes of variable stars and transients. Here we describe the automated detection and selection pipeline used to identify M31 classical novae (CNe) and we present the resulting catalogue of 20 CN candidates observed over three seasons. CNe are observed both in the bulge region as well as over a wide area of the M31 disc. Nine of the CNe are caught during the final rise phase and all are well sampled in at least two colours. The excellent light-curve coverage has allowed us to detect and classify CNe over a wide range of speed class, from very fast to very slow. Among the light curves is a moderately fast CN exhibiting entry into a deep transition minimum, followed by its final decline. We have also observed in detail a very slow CN which faded by only 0.01 mag d(-1) over a 150-d period. We detect other interesting variable objects, including one of the longest period and most luminous Mira variables. The CN catalogue constitutes a uniquely well-sampled and objectively-selected data set with which to study the statistical properties of CNe in M31, such as the global nova rate, the reliability of novae as standard-candle distance indicators and the dependence of the nova population on stellar environment. The findings of this statistical study will be reported in a follow-up paper.

The POINT-AGAPE survey - I. The variable stars in M31

For the purposes of identifying microlensing events, the POINT-AGAPE collaboration has been monitoring the Andromeda galaxy (M31) for three seasons (1999-2001) with the Wide Field Camera on the Isaac Newton Telescope. In each season, data are taken for one hour per night for roughly 60 nights during the six months that M31 is visible. The two 33 x 33 arcmin(2) fields of view straddle the central bulge, northwards and southwards. We have calculated the locations, periods and brightness of 35 414 variable stars in M31 as a by-product of the microlensing search. The variables are classified according to their period and brightness. Rough correspondences with classical types of variable star (such as Population I and II Cepheids, Miras and semiregular long-period variables) are established. The spatial distribution of Population I Cepheids is clearly associated with the spiral arms, while the central concentration of the Miras and long-period variables varies noticeably, the brighter and the shorter period Miras being much more centrally concentrated.

The anomaly in the candidate microlensing event PA-99-N2

The light curve of PA-99-N2, one of the recently announced microlensing candidates toward M31, shows small deviations from the standard Paczynski form. We explore a number of possible explanations, including correlations with the seeing, the parallax effect, and a binary lens. We find that the observations are consistent with an unresolved red giant branch or asymptotic giant branch star in M31 being microlensed by a binary lens. We find that the best-fit binary lens mass ratio is similar to1.2x10(-2), which is one of the most extreme values found for a binary lens so far. If both the source and lens lie in the M31 disk, then the standard M31 model predicts the probable mass range of the system to be 0.02-3.6 M-circle dot (95% confidence limit). In this scenario, the mass of the secondary component is therefore likely to be below the hydrogen-burning limit. On the other hand, if a compact halo object in M31 is lensing a disk or spheroid source, then the total lens mass is likely to lie between 0.09 and 32 M-circle dot, which is consistent with the primary being a stellar remnant and the secondary being a low-mass star or brown dwarf. The optical depth (or, alternatively, the differential rate) along the line of sight toward the event indicates that a halo lens is more likely than a stellar lens, provided that dark compact objects comprise no less than 15% (or 5%) of halos.

Theory of pixel lensing toward M31. II. The velocity anisotropy and flattening of the MACHO distribution

The POINT-AGAPE collaboration is currently searching for massive compact halo objects (MACHOs) toward the Andromeda galaxy (M31). The survey aims to exploit the high inclination of the M31 disk, which causes an asymmetry in the spatial distribution of M31 MACHOs. Here, we investigate the effects of halo velocity anisotropy and flattening on the asymmetry signal using simple halo models. For a spherically symmetric and isotropic halo, we find that the underlying pixel lensing rate in far-disk M31 MACHOs is more than 5 times the rate of near-disk events. We find that the asymmetry is further increased by about 30% if the MACHOs occupy radial orbits rather than tangential orbits, but it is substantially reduced if the MACHOs lie in a flattened halo. However, even for halos with a minor- to major-axis ratio of q = 0.3, the number of M31 MACHOs in the far side outnumber those in the near side by a factor of similar to2. There is also a distance asymmetry, in that the events on the far side are typically farther from the major axis. We show that, if this positional information is exploited in addition to number counts, then the number of candidate events required to confirm asymmetry for a range of flattened and anisotropic halo models is achievable, even with significant contamination by variable stars and foreground microlensing events. For pixel lensing surveys that probe a representative portion of the M31 disk, a sample of around 50 candidates is likely to be sufficient to detect asymmetry within spherical halos, even if half the sample is contaminated, or to detect asymmetry in halos as flat as q = 0.3, provided less than a third of the sample comprises contaminants. We also argue that, provided its mass-to-light ratio is less than 100, the recently observed stellar stream around M31 is not problematic for the detection of asymmetry.

The POINT-AGAPE survey: 4 high signal-to-noise microlensing candidates detected towards M 31

We have carried out a survey of the Andromeda galaxy for unresolved microlensing (pixel lensing). We present a subset of four short timescale, high signal-to-noise microlensing candidates found by imposing severe selection criteria: the source flux variation exceeds the flux of an R = 21 magnitude star and the full width at half maximum timescale is less than 25 days. Remarkably, in three out of four cases, we have been able to measure or strongly constrain the Einstein crossing time of the event. One event, which lies projected on the M 31 bulge, is almost certainly due to a stellar lens in the bulge of M 31. The other three candidates can be explained either by stars in M 31 and M 32 or by MACHOs.

A candidate M31/M32 intergalactic microlensing event

We report the discovery of a microlensing candidate projected 2'54

Débattre : pratique de l'argumentation et inscription de l'identité dans une perspective textuelle et interactionnelle

L'objectif de la thèse est de rendre compte d'une pratique langagière particulière, le débat, et d'opérer ce travail à la fois à un niveau théorique - en tant qu'analyser la pratique du débat pose certaines questions aux sciences du langage - et à un niveau pratique - dans la mesure où la spécificité du débat repose sur certains observables qu'il s'agit d'identifier et de décrire et qui permettent à chacun de distinguer le débat d'autres formes de comportement, telles que l'anecdote, la dispute ou encore la réunion de travail.¦La thèse part du constat que la pratique du débat constitue un fait social attesté et reconnaissable comme tel, et ce aussi bien par les agents qui s'engagent dans son accomplissement que par un observateur externe. Le fait qu'aucune règle ne vienne pour autant décrire «ce qui fait débat» plaide pour l'adoption d'une perspective ethnométhodologique, sensible à la manière dont les agents pourvoient eux-mêmes, en agissant de façon méthodique et routinière, à la reconnaissabilité (accountability) des pratiques dans lesquelles ils s'engagent.¦La thèse questionne le caractère reconnaissable de la pratique du débat à partir de données originales. Le corpus est constitué de huit événements publics s'étant déroulés à l'Université de Lausanne et ayant été vidéo-enregistrés pour l'occasion. Ces rencontres ne relèvent donc pas d'événements télédiffusés, par exemple des débats de sociétés organisés par des chaînes de télévision. Il s'agit de confrontations verbales (de types « débats publics » ou « conférence-discussion ») où tous les participants, public compris, sont réunis en un même lieu et dans une même tranche temporelle.¦La thèse organise la réflexion en trois parties. Intitulée la parole en interaction médiatisée, la première partie est consacrée à la présentation et à la problématisation, grâce à divers extraits du corpus, des différentes dimensions analytiques mobilisées. Par l'articulation d'acquis en linguistique textuelle et énonciative et en analyse conversationnelle, il s'agit d'étudier la matérialité signifiante des actions verbales en lien avec les dynamiques discursives et interactionnelles dans lesquelles cette matérialité s'inscrit et prend sens. En d'autres termes, on considère la manière dont les unités linguistiques participent à l'accomplissement d'activités pratiques et les pressions que ces activités pratiques sont susceptibles d'exercer sur l'usage de ces unités. L'analyse du débat est en outre inscrite dans une approche multimodale des pratiques, qui entend dépasser l'analyse de la seule verbalité pour donner une place aux ressources corporelles, qu'il s'agisse de gestes, de mimiques ou de la répartition des participants dans l'espace.¦Une fois les différentes dimensions analytiques posées, les deux autres parties examinent chacune une composante - autrement dit un observable - qui spécifie le débat en tant que pratique langagière particulière. Mobilisant une approche dialogale de la pratique de l 'argumentation, la deuxième partie entend montrer que le débat gagne à être abordé comme un mode particulier de gestion du désaccord, fondé sur l'usage de ressources argumentatives. La troisième partie s'intéresse finalement à la problématique de l'inscription de l'identité dans le langage et dans l'interaction et considère la manière dont les traits identitaires que les agents s'attribuent, respectivement ou réciproquement, lorsqu'ils s'engagent dans un débat, participent à assurer le caractère reconnaissable de cette pratique.

Revue rétrospective ou Archives secrètes du dernier gouvernement : 1830-1848 : recueil non périodique / [publié par Jules Taschereau]

1848.

Guide général dans Paris

Collection : Guides illustrés à 1 franc

Revue rétrospective ou Archives secrètes du dernier gouvernement : 1830-1848 : recueil non périodique / [publié par Jules Taschereau]

Etat de collection : N° 1-32/33 (1848)

« Le Jeu des eschez amoureux, translaté de rithme en prose et exposé ».

Contient : « Pour ce que la matière d'amours est délictable en soy... » ; « ... et qui seroient belles à déclairer, maiz pour certaine cause je m'en tairay à tant quant à présent. » — Le texte est suivi d'un petit épilogue en 8 vers (fol. 289) : « Je lairray donc ceste matière, Tant soit elle de grant mistère... » ; « Tabula hujus libri. De comparatione ludi scacorum... »