381 research outputs found

    Employment promotion : the Danish case

    Get PDF
    Der Beitrag wurde auf einer wissenschaftlichen Tagung anlĂ€sslich des dreißigjĂ€hrigen Bestehens des Instituts fĂŒr Arbeitsmarkt- und Berufsforschung der Bundesanstalt fĂŒr Arbeit prĂ€sentiert. Der Autor berichtet darin ĂŒber dĂ€nische Erfahrungen beim Abbau der Arbeitslosigkeit. (IAB)Arbeitsmarktentwicklung, ArbeitslosigkeitsbekĂ€mpfung, BeschĂ€ftigungspolitik, DĂ€nemark

    A Danish Profiling System

    Get PDF
    We describe the statistical model used for profiling new unemployed workers in Denmark. When a worker - during his or her first six months in unemployment - enters the employment office for the first time, this model predicts whether he or she will be unemployed for more than six months from that date or not. The case workers’ assessment of how to treat the person is partially based upon this prediction.unemployment duration; profiling

    A Danish Profiling System

    Full text link
    We describe the statistical model used for profiling new unemployed workers in Denmark. When a worker – during his or her first six months in unemployment – enters the employment office for the first time, this model predicts whether he or she will be unemployed for more than six months from that date or not. The case workers? assessment of how to treat the person is partially based upon this prediction

    Oxygen isotope composition of surface snow collected along the traverse route from Zhongshan Station toward Dome A, Antarctica

    Get PDF
    Oxygen isotope composition of surface snow sampled in the austral summer of 1998/1999 along the traverse route from Zhongshan Station toward Dome A, Antarctica is measured with the conventional mass spectrometer technique. The results of measurement show that oxygen isotope composition of surface snow varies in a wide range from -22.51‰ to -50.67‰, and has a tendency that isotopic values gradually decrease with increase of distance from Zhongshan Station and altitude. Linear regression analysis indicates that there exists good correlation between oxygen isotope composition of surface snow and distance from Zhongshan Station, altitude and/or latitude, which actually reflects the close relation between stable isotope composition and air temperature

    The Highly Energetic Expansion of SN2010bh Associated with GRB 100316D

    Get PDF
    We present the spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed type Ic supernova, SN 2010bh, associated with the soft, long-duration gamma-ray burst (X-ray flash) GRB 100316D. Intensive follow-up observations of SN 2010bh were performed at the ESO Very Large Telescope (VLT) using the X-shooter and FORS2 instruments. Owing to the detailed temporal coverage and the extended wavelength range (3000--24800 A), we obtained an unprecedentedly rich spectral sequence among the hypernovae, making SN 2010bh one of the best studied representatives of this SN class. We find that SN 2010bh has a more rapid rise to maximum brightness (8.0 +/- 1.0 rest-frame days) and a fainter absolute peak luminosity (L_bol~3e42 erg/s) than previously observed SN events associated with GRBs. Our estimate of the ejected (56)Ni mass is 0.12 +/- 0.02 Msun. From the broad spectral features we measure expansion velocities up to 47,000 km/s, higher than those of SNe 1998bw (GRB 980425) and 2006aj (GRB 060218). Helium absorption lines He I lambda5876 and He I 1.083 microm, blueshifted by ~20,000--30,000 km/s and ~28,000--38,000 km/s, respectively, may be present in the optical spectra. However, the lack of coverage of the He I 2.058 microm line prevents us from confirming such identifications. The nebular spectrum, taken at ~186 days after the explosion, shows a broad but faint [O I] emission at 6340 A. The light-curve shape and photospheric expansion velocities of SN 2010bh suggest that we witnessed a highly energetic explosion with a small ejected mass (E_k ~ 1e52 erg and M_ej ~ 3 Msun). The observed properties of SN 2010bh further extend the heterogeneity of the class of GRB supernovae.Comment: 37 pages and 12 figures (one-column pre-print format), accepted for publication in Ap
    • 

    corecore