23 research outputs found

    Palaeoecological Implications of Archaeological Seal Bone Assemblages: Case Studies from Labrador and Baffin Island

    Get PDF
    In recent years, increasing scientific attention has been paid to sea mammals as biological indicators of Arctic environmental change. The usefulness of animals such as ringed seal (Phoca hispida), harp seal (Phoca groenlandica), bearded seal (Erignathus barbatus), and harbour seal (Phoca vitulina) as indicator species is due to the close relationship of their range, reproductive cycles, and life histories to sea ice. The behaviour and distribution of these species correlate with ice conditions in the areas where the animals are encountered. The proportions of seal species represented in archaeological deposits may therefore reflect, at least in part, environmental conditions characterizing past seascapes. This paper examines zooarchaeological data from several Thule and historic Inuit archaeological sites in Baffin Island and Labrador, sites occupied during the last 700 years, to determine whether regional relationships can be demonstrated between subsistence economies, seal populations, and sea ice conditions. Ratios of ringed seal, harbour seal, bearded seal, and walrus (Odobenus rosmarus) bone frequencies from several archaeological sites are analyzed and discussed in light of new high-resolution proxy sea ice and regional palaeoenvironmental data. This exploratory study suggests that characteristics in seal species composition reflected in these assemblages can, in some circumstances, be correlated with recent sea ice reconstructions. However, a regional comparison of a larger number of more precisely dated archaeological sites is required for a full examination of these relationships. Au cours des dernières années, on a porté de plus en plus d'attention scientifique aux mammifères marins en tant qu'indicateurs biologiques du changement global dans l'Arctique. L'utilité d'animaux tels que le phoque annelé (Phoca hispida), le phoque du Groenland (Phoca groenlandica), le phoque barbu (Erignathus barbatus) et le phoque commun (Phoca vitulina) comme espèces indicatrices est due au rapport étroit que leurs aires de distribution, leurs cycles de reproduction et leurs cycles de vie ont avec la glace marine. Le comportement et la distribution de ces espèces sont corrélés avec les conditions de la glace dans les zones où l'on rencontre ces animaux. Les proportions des espèces de phoques qui se trouvent dans les dépôts archéologiques pourraient donc refléter, du moins partiellement, les conditions environnementales qui caractérisaient les paysages marins du passé. Cet article se penche sur les données zooarchéologiques provenant de plusieurs sites archéologiques Thulé et inuits dans l'île Baffin et le Labrador, sites occupés au cours des 700 dernières années, pour déterminer si l'on peut démontrer l'existence de rapports régionaux entre les économies de subsistance, les populations de phoques et les conditions de glace marine. Des taux de fréquence d'os de phoque annelé, de phoque commun, de phoque barbu et de morse provenant de plusieurs sites archéologiques font l'objet d'une analyse et d'une discussion à la lumière de nouvelles données indirectes à haute résolution sur la glace marine et sur le paléoenvironnement régional. Cette étude préliminaire suggère que les caractéristiques présentes dans la composition des espèces de phoques reflétée dans ces assemblages peuvent, dans certaines conditions, être corrélées aux reconstructions récentes de la glace marine. Une comparaison régionale d'un plus grand nombre de sites archéologiques datés de façon plus précise est toutefois nécessaire pour un examen exhaustif de ces rapports.

    Palaeoecological Implications of Archaeological Seal Bone Assemblages: Case Studies from Labrador and Baffin Island

    Get PDF
    In recent years, increasing scientific attention has been paid to sea mammals as biological indicators of Arctic environmental change. The usefulness of animals such as ringed seal (Phoca hispida), harp seal (Phoca groenlandica), bearded seal (Erignathus barbatus), and harbour seal (Phoca vitulina) as indicator species is due to the close relationship of their range, reproductive cycles, and life histories to sea ice. The behaviour and distribution of these species correlate with ice conditions in the areas where the animals are encountered. The proportions of seal species represented in archaeological deposits may therefore reflect, at least in part, environmental conditions characterizing past seascapes. This paper examines zooarchaeological data from several Thule and historic Inuit archaeological sites in Baffin Island and Labrador, sites occupied during the last 700 years, to determine whether regional relationships can be demonstrated between subsistence economies, seal populations, and sea ice conditions. Ratios of ringed seal, harbour seal, bearded seal, and walrus (Odobenus rosmarus) bone frequencies from several archaeological sites are analyzed and discussed in light of new high-resolution proxy sea ice and regional palaeoenvironmental data. This exploratory study suggests that characteristics in seal species composition reflected in these assemblages can, in some circumstances, be correlated with recent sea ice reconstructions. However, a regional comparison of a larger number of more precisely dated archaeological sites is required for a full examination of these relationships. Au cours des dernières années, on a porté de plus en plus d'attention scientifique aux mammifères marins en tant qu'indicateurs biologiques du changement global dans l'Arctique. L'utilité d'animaux tels que le phoque annelé (Phoca hispida), le phoque du Groenland (Phoca groenlandica), le phoque barbu (Erignathus barbatus) et le phoque commun (Phoca vitulina) comme espèces indicatrices est due au rapport étroit que leurs aires de distribution, leurs cycles de reproduction et leurs cycles de vie ont avec la glace marine. Le comportement et la distribution de ces espèces sont corrélés avec les conditions de la glace dans les zones où l'on rencontre ces animaux. Les proportions des espèces de phoques qui se trouvent dans les dépôts archéologiques pourraient donc refléter, du moins partiellement, les conditions environnementales qui caractérisaient les paysages marins du passé. Cet article se penche sur les données zooarchéologiques provenant de plusieurs sites archéologiques Thulé et inuits dans l'île Baffin et le Labrador, sites occupés au cours des 700 dernières années, pour déterminer si l'on peut démontrer l'existence de rapports régionaux entre les économies de subsistance, les populations de phoques et les conditions de glace marine. Des taux de fréquence d'os de phoque annelé, de phoque commun, de phoque barbu et de morse provenant de plusieurs sites archéologiques font l'objet d'une analyse et d'une discussion à la lumière de nouvelles données indirectes à haute résolution sur la glace marine et sur le paléoenvironnement régional. Cette étude préliminaire suggère que les caractéristiques présentes dans la composition des espèces de phoques reflétée dans ces assemblages peuvent, dans certaines conditions, être corrélées aux reconstructions récentes de la glace marine. Une comparaison régionale d'un plus grand nombre de sites archéologiques datés de façon plus précise est toutefois nécessaire pour un examen exhaustif de ces rapports.

    The James Webb Space Telescope Mission

    Full text link
    Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized space telescope with an aperture of at least 4m4m. With the support of their governments in the US, Europe, and Canada, 20,000 people realized that vision as the 6.5m6.5m James Webb Space Telescope. A generation of astronomers will celebrate their accomplishments for the life of the mission, potentially as long as 20 years, and beyond. This report and the scientific discoveries that follow are extended thank-you notes to the 20,000 team members. The telescope is working perfectly, with much better image quality than expected. In this and accompanying papers, we give a brief history, describe the observatory, outline its objectives and current observing program, and discuss the inventions and people who made it possible. We cite detailed reports on the design and the measured performance on orbit.Comment: Accepted by PASP for the special issue on The James Webb Space Telescope Overview, 29 pages, 4 figure

    Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network

    Get PDF
    Gravitational lensing by massive objects along the line of sight to the source causes distortions of gravitational wave-signals; such distortions may reveal information about fundamental physics, cosmology and astrophysics. In this work, we have extended the search for lensing signatures to all binary black hole events from the third observing run of the LIGO--Virgo network. We search for repeated signals from strong lensing by 1) performing targeted searches for subthreshold signals, 2) calculating the degree of overlap amongst the intrinsic parameters and sky location of pairs of signals, 3) comparing the similarities of the spectrograms amongst pairs of signals, and 4) performing dual-signal Bayesian analysis that takes into account selection effects and astrophysical knowledge. We also search for distortions to the gravitational waveform caused by 1) frequency-independent phase shifts in strongly lensed images, and 2) frequency-dependent modulation of the amplitude and phase due to point masses. None of these searches yields significant evidence for lensing. Finally, we use the non-detection of gravitational-wave lensing to constrain the lensing rate based on the latest merger-rate estimates and the fraction of dark matter composed of compact objects

    Search for eccentric black hole coalescences during the third observing run of LIGO and Virgo

    Get PDF
    Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass M>70 M⊙) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities 0<e≤0.3 at 0.33 Gpc−3 yr−1 at 90\% confidence level

    Ultralight vector dark matter search using data from the KAGRA O3GK run

    Get PDF
    Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for U(1)B−L gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the U(1)B−L gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM

    Observation of gravitational waves from the coalescence of a 2.5−4.5 M⊙ compact object and a neutron star

    Get PDF
    corecore