SOPHIE velocimetry of Kepler transit candidates XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet

In this paper we report a new transiting warm giant planet: KOI-1257 b. It was first detected in photometry as a planet-candidate by the ${\it Kepler}$ space telescope and then validated thanks to a radial velocity follow-up with the SOPHIE spectrograph. It orbits its host star with a period of 86.647661 d $\pm$ 3 s and a high eccentricity of 0.772 $\pm$ 0.045. The planet transits the main star of a metal-rich, relatively old binary system with stars of mass of 0.99 $\pm$ 0.05 Msun and 0.70 $\pm$ 0.07 Msun for the primary and secondary, respectively. This binary system is constrained thanks to a self-consistent modelling of the ${\it Kepler}$ transit light curve, the SOPHIE radial velocities, line bisector and full-width half maximum (FWHM) variations, and the spectral energy distribution. However, future observations are needed to confirm it. The PASTIS fully-Bayesian software was used to validate the nature of the planet and to determine which star of the binary system is the transit host. By accounting for the dilution from the binary both in photometry and in radial velocity, we find that the planet has a mass of 1.45 $\pm$ 0.35 Mjup, and a radius of 0.94 $\pm$ 0.12 Rjup, and thus a bulk density of 2.1 $\pm$ 1.2 g.cm$^{-3}$. The planet has an equilibrium temperature of 511 $\pm$ 50 K, making it one of the few known members of the warm-jupiter population. The HARPS-N spectrograph was also used to observe a transit of KOI-1257 b, simultaneously with a joint amateur and professional photometric follow-up, with the aim of constraining the orbital obliquity of the planet. However, the Rossiter-McLaughlin effect was not clearly detected, resulting in poor constraints on the orbital obliquity of the planet.Comment: 39 pages, 17 figures, accepted for publication in Astronomy & Astrophysic

Rethinking “democratic backsliding” in Central and Eastern Europe – looking beyond Hungary and Poland

This essay introduces contributions to a special issue of East European Politics on “Rethinking democratic backsliding in Central and Eastern Europe”, which seeks to expand the study of democratic regression in CEE beyond the paradigmatic cases of Hungary and Poland. Reviewing these contributions, we identify several directions for research: 1) the need to critique “democratic backsliding”, not simply as a label, but also as an assumed regional trend; 2) a need to better integrate the role of illiberal socio-economic structures such as oligarchical structures or corrupt networks; and 3) a need to (re-)examine the trade-offs between democratic stability and democratic quality. We also note how insights developed researching post-communist regions such as Western Balkans or the post-Soviet space could usefully inform work on CEE backsliding. We conclude by calling for the study of CEE democracy to become more genuinely interdisciplinary, moving beyond some narrowly institutionalist comparative political science assumptions

WASP-113b and WASP-114b, two inflated hot Jupiters with contrasting densities

Aims. We present the discovery and characterisation of the exoplanets WASP-113b and WASP-114b by the WASP surveys, SOPHIE and CORALIE. Methods. The planetary nature of the systems was established by performing follow-up photometric and spectroscopic observations. The follow-up data were combined with the WASP-photometry and analysed with an MCMC code to obtain system parameters. Results. The host stars WASP-113 and WASP-114 are very similar. They are both early G-type stars with an effective temperature of ~5900 K, [Fe/H] ~ 0.12, and log g~ 4.1 dex. However, WASP-113 is older than WASP-114. Although the planetary companions have similar radii, WASP-114b is almost four times heavier than WASP-113b. WASP-113b has a mass of 0.48 MJup and an orbital period of ~4.5 days; WASP-114b has a mass of 1.77 MJup and an orbital period of ~1.5 days. Both planets have inflated radii, in particular WASP-113 with a radius anomaly of ℜ = 0.35. The high scale height of WASP-113b (~950 km) makes it a good target for follow-up atmospheric observations.Publisher PDFPeer reviewe

Spin-orbit inclinations of the exoplanetary systems HAT-P-8, HAT-P-9, HAT-P-16 and HAT-P-23

We report the measurement of the spin-orbit angle of the extra-solar planets HAT-P-8 b, HAT-P-9 b, HAT-P-16 b and HAT-P-23 b, thanks to spectroscopic observations performed at the Observatoire de Haute-Provence with the SOPHIE spectrograph on the 1.93-m telescope. Radial velocity measurements of the Rossiter-McLaughlin effect show the detection of an apparent prograde, aligned orbit for all systems. The projected spin-orbit angles are found to be lambda=-17 deg (+9.2,-11.5), -16 deg (8), -10 deg (16), +15 deg (22) for HAT-P-8, HAT-P-9, HAT-P-16 and HAT-P-23 respectively, with corresponding projected rotational velocities of 14.5 (0.8), 12.5 (1.8), 3.9 (0.8), and 7.8 (1.6) km/s. These new results increase to 37 the number of accurately measured spin-orbit angles in transiting extrasolar systems. We conclude by drawing a tentative picture of the global behaviour of orbital alignement, involving the complexity and diversity of possible mechanisms.Comment: accepted in A&

It’s Not the Left: Ideology and Protest Participation in Old and New Democracies

Multiple studies in political science consistently hold that left-wing ideology renders individuals more prone to protest behavior. However, the familiar association between left-wing ideology and protesting is not empirically corroborated in all democratic nations. Building on existing theoretical principles and applying them to diverse political contexts, this paper sheds light on puzzling variation in protest behavior across new and old democracies. It argues that it is not the left that engenders protest. Instead, we demonstrate that which political camp engages in protest behavior depends on its historical legacies and cultural liberalism. Historical legacies reflect the ideological configuration at democratization. Protesting tends to be more common in the ideological camp that opposed the pre-democratic political order. Simultaneously, it is culturally liberal individuals that more likely embrace protest participation, independent of their left-right identification. These theoretical expectations are supported through survey data analyses, explaining contrasting inter- and intra-regional variation in European democracies

Organizing for impact: International organizations and global pension policy

The internal dynamics and politics of international organizations influence how international policy agendas are set and how effectively they are pursued. International organizations are open systems which respond and adapt to the external policy environment in order to remain relevant to global policymaking. Through an analysis of the internal politics of the World Bank and International Labour Organization, the leading global agenda-setters for pension reform, this article shows that internal political battles and restructuring have a decisive influence on global pensions policy. Appointment of key personnel and internal reorganization can help make certain policy ideas prominent over others. Scholars should pay greater attention to processes of change within international organizations in order to better understand the international agenda setting process

Migrants’ Access to Social Protection in Romania

peer reviewedThis chapter examines to what extent the Romanian welfare system covers resident citizens compared to foreigners residing in Romania and Romanians living abroad. In doing so, we analyse existing social policies aiming to ensure their coverage against a variety of risks at different life-cycle stages, including unemployment, poverty, sickness and old-age. The main conclusion is that the Romanian welfare state is open to all residents, regardless of their nationality, thus providing everyone equal grounds for accessing social benefits. The criterion of residence on the Romanian soil is, however, prevalent. This implies that relatively few social provisions are extended for non-resident Romanians, which represent an increasingly sizeable community given the intensity of migration outflows in recent years. Furthermore, the Romanian social protection system has had relatively little impact on reducing the risk of poverty and income inequality in the country, despite regular amendments during the last years.Migration and transnational social protection in (post) crisis Europ