79 research outputs found
Dealing with adversity: religiosity or science? Evidence from the great influenza pandemic
How do societies respond to adversity? After a negative shock, separate strands of research document either an increase in religiosity or a boost in innovation efforts. In this paper, we show that both reactions can occur at the same time, driven by different individuals within society. The setting of our study is the 1918-1919 influenza pandemic in the United States. To measure religiosity, we construct a novel indicator based on naming patterns of newborns. We measure innovation through the universe of granted patents. Exploiting plausibly exogenous county-level variation in exposure to the pandemic, we provide evidence that more-affected counties become both more religious and more innovative. Looking within counties, we uncover heterogeneous responses: individuals from more religious backgrounds further embrace religion, while those from less religious backgrounds become more likely to choose a scientific occupation. Facing adversity widens the distance in religiosity between science-oriented individuals and the rest of the population, and it increases the polarization of religious beliefs
An imaged 15Mjup companion within a hierarchical quadruple system
Since 2019, the direct imaging B-star Exoplanet Abundance Study (BEAST) at
SPHERE@VLT has been scanning the surroundings of young B-type stars in order to
ascertain the ultimate frontiers of giant planet formation. Recently, the
Myr HIP 81208 was found to host a close-in (~50 au) brown dwarf
and a wider (~230 au) late M star around the central 2.6Msun primary. Alongside
the continuation of the survey, we are undertaking a complete reanalysis of
archival data aimed at improving detection performances so as to uncover
additional low-mass companions. We present here a new reduction of the
observations of HIP 81208 using PACO ASDI, a recent and powerful algorithm
dedicated to processing high-contrast imaging datasets, as well as more
classical algorithms and a dedicated PSF-subtraction approach. The combination
of different techniques allowed for a reliable extraction of astrometric and
photometric parameters. A previously undetected source was recovered at a short
separation from the C component of the system. Proper motion analysis provided
robust evidence for the gravitational bond of the object to HIP 81208 C.
Orbiting C at a distance of ~20 au, this 15Mjup brown dwarf becomes the fourth
object of the hierarchical HIP 81208 system. Among the several BEAST stars
which are being found to host substellar companions, HIP 81208 stands out as a
particularly striking system. As the first stellar binary system with
substellar companions around each component ever found by direct imaging, it
yields exquisite opportunities for thorough formation and dynamical follow-up
studies.Comment: 12 pages, 9 figures, 5 tables. Accepted for publication as a Letter
in Astronomy and Astrophysics, section 1. Letters to the Edito
The high-albedo, low polarization disk around HD 114082 harbouring a Jupiter-sized transiting planet
We present new optical and near-IR images of debris disk around the F-type
star HD 114082. We obtained direct imaging observations and analysed the TESS
photometric time series data of this target with a goal to search for planetary
companions and to characterise the morphology of the debris disk and the
scattering properties of dust particles. HD 114082 was observed with the
VLT/SPHERE instrument: the IRDIS camera in the K band together with the IFS in
the Y, J and H band using the ADI technique as well as IRDIS in the H band and
ZIMPOL in the I_PRIME band using the PDI technique. The scattered light images
were fitted with a 3D model for single scattering in an optically thin dust
disk. We performed aperture photometry in order to derive the scattering and
polarized phase functions, polarization fraction and spectral scattering albedo
for the dust particles in the disk. This method was also used to obtain the
reflectance spectrum of the disk to retrieve the disk color and study the dust
reflectivity in comparison to the debris disk HD 117214. We also performed the
modeling of the HD 114082 light curve measured by TESS using the models for
planet transit and stellar activity to put constraints on radius of the
detected planet and its orbit. The debris disk appears as an axisymmetric
debris belt with a radius of ~0.37 (35 au), inclination of ~83 and a
wide inner cavity. Dust particles in HD 114082 have a maximum polarization
fraction of ~17% and a high reflectivity which results in a spectral scattering
albedo of 0.65. The analysis of TESS photometric data reveals a transiting
planetary companion to HD 114082 with a radius of 1~ on an
orbit with a semi-major axis of au. Combining different data, we
reach deep sensitivity limits in terms of companion masses down to ~5 at 50 au, and ~10 at 30 au from the central star.Comment: 27 page
TOI-179: a young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit
Transiting planets around young stars are key benchmarks for our
understanding of planetary systems. One of such candidates was identified
around the K dwarf HD 18599 by TESS, labeled as TOI-179. We present the
confirmation of the transiting planet and the characterization of the host star
and of the TOI-179 system over a broad range of angular separations. To this
aim, we exploited the TESS photometric time series, intensive radial velocity
monitoring performed with HARPS, and deep high-contrast imaging observations
obtained with SPHERE and NACO at VLT. The inclusion of Gaussian processes
regression analysis is effective to properly model the magnetic activity of the
star and identify the Keplerian signature of the transiting planet. The star,
with an age of 400+-100 Myr, is orbited by a transiting planet with period
4.137436 days, mass 24+-7 Mearth, radius 2.62 (+0.15-0.12) Rearth, and
significant eccentricity (0.34 (+0.07-0.09)). Adaptive optics observations
identified a low-mass companion at the boundary between brown dwarfs and very
low mass stars (mass derived from luminosity 83 (+4-6) Mjup) at a very small
projected separation (84.5 mas, 3.3 au at the distance of the star). Coupling
the imaging detection with the long-term radial velocity trend and the
astrometric signature, we constrained the orbit of the low mass companion,
identifying two families of possible orbital solutions. The TOI-179 system
represents a high-merit laboratory for our understanding of the physical
evolution of planets and other low-mass objects and of how the planet
properties are influenced by dynamical effects and interactions with the parent
star.Comment: 25 pages, 24 figures, A&A, in pres
A scaled-up planetary system around a supernova progenitor
Context. Virtually all known exoplanets reside around stars with M Mâ either due to the rapid evaporation of the protostellar disks or to selection effects impeding detections around more massive stellar hosts.
Aims. To clarify if this dearth of planets is real or a selection effect, we launched the planet-hunting B-star Exoplanet Abundance STudy (BEAST) survey targeting B stars (M > 2.4 Mâ) in the young (5â20 Myr) Scorpius-Centaurus association by means of the high-contrast spectro-imager SPHERE at the Very Large Telescope.
Methods. In this paper we present the analysis of high-contrast images of the massive (M ~ 9 Mâ) star ÎŒ2 Sco obtained within BEAST. We carefully examined the properties of this star, combining data from Gaia and from the literature, and used state-of-the-art algorithms for the reduction and analysis of our observations.
Results. Based on kinematic information, we found that Ό2 Sco is a member of a small group which we label Eastern Lower Scorpius within the Scorpius-Centaurus association. We were thus able to constrain its distance, refining in turn the precision on stellar parameters. Around this star we identify a robustly detected substellar companion (14.4 ± 0.8 MJ)at a projected separation of 290 ± 10 au, and a probable second similar object (18.5 ± 1.5 MJ) at 21 ± 1 au. The planet-to-star mass ratios of these objects are similar to that of Jupiter to the Sun, and the flux they receive from the star is similar to those of Jupiter and Mercury, respectively.
Conclusions. The robust and the probable companions of Ό2 Sco are naturally added to the giant 10.9 MJ planet recently discovered by BEAST around the binary b Cen system. While these objects are slightly more massive than the deuterium burning limit, their properties are similar to those of giant planets around less massive stars and they are better reproduced by assuming that they formed under a planet-like, rather than a star-like scenario. Irrespective of the (needed) confirmation of the inner companion, Ό2 Sco is the first star that would end its life as a supernova that hosts such a system. The tentative high frequency of BEAST discoveries is unexpected, and it shows that systems with giant planets or small-mass brown dwarfs can form around B stars. When putting this finding in the context of core accretion and gravitational instability formation scenarios, we conclude that the current modeling of both mechanisms is not able to produce this kind of companion. The completion of BEAST will pave the way for the first time to an extension of these models to intermediate and massive stars
A scaled-up planetary system around a supernova progenitor
Stars and planetary system
Food Price Shocks and the Political Economy of Global Agricultural and Development Policy
The recent spikes of global food prices induced a rapid increase in mass media coverage, public policy attention, and donor funding for food security and for agriculture and rural poverty. This has occurred while the shift from low to high food prices has induced a shift in (demographic or social) location of the hunger and poverty effects, but the total number of undernourished and poor people has declined over the same period. We suggest that the observed pattern can be explained by the presence of a global urban bias on agriculture and food policy in developing countries, and we discuss whether this global urban bias may actually benefit poor farmers. We argue that the food price spikes have succeeded where others have failed in the past: to move the problems of poor and hungry farmers to the top of the policy agenda and to induce development and donor strategies to help them
Economic-demographic interactions in long-run growth
Cliometrics confirms that Malthusâ model of the pre-industrial economy, in which increases in productivity raise population but higher population drives down wages, is a good description for much of demographic/economic history. A contributor to the Malthusian equilibrium was the Western European Marriage Pattern, the late age of female first marriage, which promised to retard the fall of living standards by restricting fertility. The demographic transition and the transition from Malthusian economies to modern economic growth attracted many Cliometric models surveyed here. A popular model component is that lower levels of mortality over many centuries increased the returns to, or preference for, human capital investment so that technical progress eventually accelerated. This initially boosted birth rates and population growth accelerated. Fertility decline was earliest and most striking in late eighteenth century France. By the 1830s the fall in French marital fertility is consistent with a response to the rising opportunity cost of children. The rest of Europe did not begin to follow until end of the nineteenth century. Interactions between the economy and migration have been modelled with Cliometric structures closely related to those of natural increase and the economy. Wages were driven up by emigration from Europe and reduced in the economies receiving immigrants
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