ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

X
feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
  • 1
    facet.materialart.
    Unknown
    GRB 140606B/iPTF14bfu: detection of shock-breakout emission from a cosmological {gamma}-ray burst? (2015)
    Oxford University Press
    Details
    Publication Date: 2015-07-25
    Description: We present optical and near-infrared photometry of GRB 140606B ( z  = 0.384), and optical photometry and spectroscopy of its associated supernova (SN). The results of our modelling indicate that the bolometric properties of the SN ( M Ni  = 0.4 ± 0.2 M , M ej  = 5 ± 2 M , and E K  = 2 ± 1  x  10 52  erg) are fully consistent with the statistical averages determined for other -ray burst (GRB)-SNe. However, in terms of its -ray emission, GRB 140606B is an outlier of the Amati relation, and occupies the same region as low luminosity ( ll ) and short GRBs. The -ray emission in ll GRBs is thought to arise in some or all events from a shock breakout (SBO), rather than from a jet. The measured peak photon energy ( E p   800 keV) is close to that expected for -rays created by an SBO ( 1 MeV). Moreover, based on its position in the M V , p -L iso, plane and the E K –β plane, GRB 140606B has properties similar to both SBO-GRBs and jetted-GRBs. Additionally, we searched for correlations between the isotropic -ray emission and the bolometric properties of a sample of GRB-SNe, finding that no statistically significant correlation is present. The average kinetic energy of the sample is $\bar{E}_{\rm K} = 2.1\times 10^{52}$  erg. All of the GRB-SNe in our sample, with the exception of SN 2006aj, are within this range, which has implications for the total energy budget available to power both the relativistic and non-relativistic components in a GRB-SN event.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
    Published by Oxford University Press
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 2
    facet.materialart.
    Unknown
    Polarimetric constraints on the optical afterglow emission from GRB 990123 (1999)
    American Association for the Advancement of Science (AAAS)
    Details
    Publication Date: 1999-03-26
    Description: Polarization of the optical emission from GRB 990123 was measured on 24.17 January 1999 universal time with the Nordic Optical Telescope. An upper limit of 2.3% on the linear polarization was found. Accurate polarization measurements provide important clues to the blast wave geometry and magnetic field structure of gamma-ray bursts (GRBs). The lack of detectable polarization for GRB 990123 indicates that the optical afterglow was produced by a blast wave of unknown geometry with an insignificant coherent magnetic field or by a beamed outflow at high Lorentz factor seen at a small viewing angle. Such a collimated jet would help solve the problem of energy release in this exceptionally luminous cosmological burst.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hjorth -- Bjornsson -- Andersen -- Caon -- Cairos -- Castro-Tirado -- Osorio -- Pedersen -- Costa -- New York, N.Y. -- Science. 1999 Mar 26;283(5410):2073-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen O, Denmark. Science Institute, University of Iceland, Dunhaga 3, IS-107 Reykjavik, Iceland. Nordic Optical Telescope, Ap. 474 St. Cruz de La Palma, E-387.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10092227" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Published by American Association for the Advancement of Science (AAAS)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 3
    facet.materialart.
    Unknown
    Decay of the GRB 990123 optical afterglow: implications for the fireball model (1999)
    American Association for the Advancement of Science (AAAS)
    Details
    Publication Date: 1999-03-26
    Description: Broad-band (ultraviolet to near-infrared) observations of the intense gamma ray burst GRB 990123 started approximately 8.5 hours after the event and continued until 18 February 1999. When combined with other data, in particular from the Robotic Telescope and Transient Source Experiment (ROTSE) and the Hubble Space Telescope (HST), evidence emerges for a smoothly declining light curve, suggesting some color dependence that could be related to a cooling break passing the ultraviolet-optical band at about 1 day after the high-energy event. The steeper decline rate seen after 1.5 to 2 days may be evidence for a collimated jet pointing toward the observer.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Castro-Tirado -- Zapatero-Osorio -- Caon -- Cairos -- Hjorth -- Pedersen -- Andersen -- Gorosabel -- Bartolini -- Guarnieri -- Piccioni -- Frontera -- Masetti -- Palazzi -- Pian -- Greiner -- Hudec -- Sagar -- Pandey -- Mohan V -- Yadav -- Nilakshi -- Bjornsson -- Jakobsson -- Burud I -- et -- New York, N.Y. -- Science. 1999 Mar 26;283(5410):2069-73.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Instituto de Astrofisica de Andalucia, IAA-CSIC, Granada, Spain. Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain. Astronomical Observatory, University of Copenhagen, Copenhagen, Denmark. Nordic Optical Telescope, La Palma, T.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10092226" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Published by American Association for the Advancement of Science (AAAS)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 4
    facet.materialart.
    Unknown
    Spectroscopic limits on the distance and energy release of GRB 990123 (1999)
    American Association for the Advancement of Science (AAAS)
    Details
    Publication Date: 1999-03-26
    Description: An optical spectrum of the afterglow from the unusually bright gamma-ray burst GRB 990123 obtained on 24.25 January 1999 universal time showed an absorption system at a redshift of z = 1.600. The absence of a hydrogen Lyman alpha forest sets an upper limit of z 〈 2.17, whereas ultraviolet photometry indicates an upper limit of z 〈 2.05. The probability of intersecting an absorption system as strong as the one observed along a random line of sight out to this z is at most a few percent, implying that GRB 990123 was probably at z = 1. 600. Currently favored cosmological parameters imply that an isotropic energy release equivalent to the rest mass of 1.8 neutron stars (4.5 x 10(54) erg) was emitted in gamma rays. Nonisotropic emission, such as intrinsic beaming, may resolve this energy problem.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Andersen -- Castro-Tirado -- Hjorth -- Moller -- Pedersen -- Caon -- Cairos -- Korhonen -- Osorio -- Perez -- Frontera -- New York, N.Y. -- Science. 1999 Mar 26;283(5410):2075-7.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Nordic Optical Telescope, Apartado 474 St. Cruz de La Palma, E-38700 Canarias, Spain. Laboratorio de Astrofisica Espacial y Fisica Fundamental, Instituto Nacional de Tecnica Aeroespacial, Post Office Box 50727, E-28080 Madrid, Spain. Insti.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10092228" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Published by American Association for the Advancement of Science (AAAS)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 5
    facet.materialart.
    Unknown
    A gamma-ray burst at a redshift of z approximately 8.2 (2009)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2009-10-30
    Description: Long-duration gamma-ray bursts (GRBs) are thought to result from the explosions of certain massive stars, and some are bright enough that they should be observable out to redshifts of z 〉 20 using current technology. Hitherto, the highest redshift measured for any object was z = 6.96, for a Lyman-alpha emitting galaxy. Here we report that GRB 090423 lies at a redshift of z approximately 8.2, implying that massive stars were being produced and dying as GRBs approximately 630 Myr after the Big Bang. The burst also pinpoints the location of its host galaxy.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Tanvir, N R -- Fox, D B -- Levan, A J -- Berger, E -- Wiersema, K -- Fynbo, J P U -- Cucchiara, A -- Kruhler, T -- Gehrels, N -- Bloom, J S -- Greiner, J -- Evans, P A -- Rol, E -- Olivares, F -- Hjorth, J -- Jakobsson, P -- Farihi, J -- Willingale, R -- Starling, R L C -- Cenko, S B -- Perley, D -- Maund, J R -- Duke, J -- Wijers, R A M J -- Adamson, A J -- Allan, A -- Bremer, M N -- Burrows, D N -- Castro-Tirado, A J -- Cavanagh, B -- de Ugarte Postigo, A -- Dopita, M A -- Fatkhullin, T A -- Fruchter, A S -- Foley, R J -- Gorosabel, J -- Kennea, J -- Kerr, T -- Klose, S -- Krimm, H A -- Komarova, V N -- Kulkarni, S R -- Moskvitin, A S -- Mundell, C G -- Naylor, T -- Page, K -- Penprase, B E -- Perri, M -- Podsiadlowski, P -- Roth, K -- Rutledge, R E -- Sakamoto, T -- Schady, P -- Schmidt, B P -- Soderberg, A M -- Sollerman, J -- Stephens, A W -- Stratta, G -- Ukwatta, T N -- Watson, D -- Westra, E -- Wold, T -- Wolf, C -- England -- Nature. 2009 Oct 29;461(7268):1254-7. doi: 10.1038/nature08459.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK. nrt3@star.le.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19865165" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 6
    facet.materialart.
    Unknown
    An extremely luminous panchromatic outburst from the nucleus of a distant galaxy (2011)
    American Association for the Advancement of Science (AAAS)
    Details
    Publication Date: 2011-06-18
    Description: Variable x-ray and gamma-ray emission is characteristic of the most extreme physical processes in the universe. We present multiwavelength observations of a unique gamma-ray-selected transient detected by the Swift satellite, accompanied by bright emission across the electromagnetic spectrum, and whose properties are unlike any previously observed source. We pinpoint the event to the center of a small, star-forming galaxy at redshift z = 0.3534. Its high-energy emission has lasted much longer than any gamma-ray burst, whereas its peak luminosity was approximately 100 times higher than bright active galactic nuclei. The association of the outburst with the center of its host galaxy suggests that this phenomenon has its origin in a rare mechanism involving the massive black hole in the nucleus of that galaxy.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Levan, A J -- Tanvir, N R -- Cenko, S B -- Perley, D A -- Wiersema, K -- Bloom, J S -- Fruchter, A S -- Postigo, A de Ugarte -- O'Brien, P T -- Butler, N -- van der Horst, A J -- Leloudas, G -- Morgan, A N -- Misra, K -- Bower, G C -- Farihi, J -- Tunnicliffe, R L -- Modjaz, M -- Silverman, J M -- Hjorth, J -- Thone, C -- Cucchiara, A -- Ceron, J M Castro -- Castro-Tirado, A J -- Arnold, J A -- Bremer, M -- Brodie, J P -- Carroll, T -- Cooper, M C -- Curran, P A -- Cutri, R M -- Ehle, J -- Forbes, D -- Fynbo, J -- Gorosabel, J -- Graham, J -- Hoffman, D I -- Guziy, S -- Jakobsson, P -- Kamble, A -- Kerr, T -- Kasliwal, M M -- Kouveliotou, C -- Kocevski, D -- Law, N M -- Nugent, P E -- Ofek, E O -- Poznanski, D -- Quimby, R M -- Rol, E -- Romanowsky, A J -- Sanchez-Ramirez, R -- Schulze, S -- Singh, N -- van Spaandonk, L -- Starling, R L C -- Strom, R G -- Tello, J C -- Vaduvescu, O -- Wheatley, P J -- Wijers, R A M J -- Winters, J M -- Xu, D -- New York, N.Y. -- Science. 2011 Jul 8;333(6039):199-202. doi: 10.1126/science.1207143. Epub 2011 Jun 16.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics, University of Warwick, Coventry, UK. a.j.levan@warwick.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21680811" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Published by American Association for the Advancement of Science (AAAS)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 7
    facet.materialart.
    Unknown
    Gravitational redshift of galaxies in clusters as predicted by general relativity (2011)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2011-10-01
    Description: The theoretical framework of cosmology is mainly defined by gravity, of which general relativity is the current model. Recent tests of general relativity within the Lambda Cold Dark Matter (LambdaCDM) model have found a concordance between predictions and the observations of the growth rate and clustering of the cosmic web. General relativity has not hitherto been tested on cosmological scales independently of the assumptions of the LambdaCDM model. Here we report an observation of the gravitational redshift of light coming from galaxies in clusters at the 99 per cent confidence level, based on archival data. Our measurement agrees with the predictions of general relativity and its modification created to explain cosmic acceleration without the need for dark energy (the f(R) theory), but is inconsistent with alternative models designed to avoid the presence of dark matter.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Wojtak, Radoslaw -- Hansen, Steen H -- Hjorth, Jens -- England -- Nature. 2011 Sep 28;477(7366):567-9. doi: 10.1038/nature10445.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen O, Denmark. wojtak@dark-cosmology.dk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21956329" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 8
    facet.materialart.
    Unknown
    A 'kilonova' associated with the short-duration gamma-ray burst GRB 130603B (2013)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2013-08-06
    Description: Short-duration gamma-ray bursts are intense flashes of cosmic gamma-rays, lasting less than about two seconds, whose origin is unclear. The favoured hypothesis is that they are produced by a relativistic jet created by the merger of two compact stellar objects (specifically two neutron stars or a neutron star and a black hole). This is supported by indirect evidence such as the properties of their host galaxies, but unambiguous confirmation of the model is still lacking. Mergers of this kind are also expected to create significant quantities of neutron-rich radioactive species, whose decay should result in a faint transient, known as a 'kilonova', in the days following the burst. Indeed, it is speculated that this mechanism may be the predominant source of stable r-process elements in the Universe. Recent calculations suggest that much of the kilonova energy should appear in the near-infrared spectral range, because of the high optical opacity created by these heavy r-process elements. Here we report optical and near-infrared observations that provide strong evidence for such an event accompanying the short-duration gamma-ray burst GRB 130603B. If this, the simplest interpretation of the data, is correct, then it confirms that compact-object mergers are the progenitors of short-duration gamma-ray bursts and the sites of significant production of r-process elements. It also suggests that kilonovae offer an alternative, unbeamed electromagnetic signature of the most promising sources for direct detection of gravitational waves.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Tanvir, N R -- Levan, A J -- Fruchter, A S -- Hjorth, J -- Hounsell, R A -- Wiersema, K -- Tunnicliffe, R L -- England -- Nature. 2013 Aug 29;500(7464):547-9. doi: 10.1038/nature12505. Epub 2013 Aug 28.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK. nrt3@le.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23912055" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 9
    facet.materialart.
    Unknown
    A dust-parallax distance of 19 megaparsecs to the supermassive black hole in NGC 4151 (2014)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2014-11-28
    Description: The active galaxy NGC 4151 has a crucial role as one of only two active galactic nuclei for which black hole mass measurements based on emission line reverberation mapping can be calibrated against other dynamical techniques. Unfortunately, effective calibration requires accurate knowledge of the distance to NGC 4151, which is not at present available. Recently reported distances range from 4 to 29 megaparsecs. Strong peculiar motions make a redshift-based distance very uncertain, and the geometry of the galaxy and its nucleus prohibit accurate measurements using other techniques. Here we report a dust-parallax distance to NGC 4151 of 19.0(+2.4)(-2.6) megaparsecs. The measurement is based on an adaptation of a geometric method that uses the emission line regions of active galaxies. Because these regions are too small to be imaged with present technology, we use instead the ratio of the physical and angular sizes of the more extended hot-dust emission as determined from time delays and infrared interferometry. This distance leads to an approximately 1.4-fold increase in the dynamical black hole mass, implying a corresponding correction to emission line reverberation masses of black holes if they are calibrated against the two objects with additional dynamical masses.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Honig, Sebastian F -- Watson, Darach -- Kishimoto, Makoto -- Hjorth, Jens -- England -- Nature. 2014 Nov 27;515(7528):528-30. doi: 10.1038/nature13914.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉1] Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen O, Denmark [2] School of Physics &Astronomy, University of Southampton, Southampton SO17 1BJ, UK. ; Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen O, Denmark. ; Department of Physics, Faculty of Science, Kyoto Sangyo University, Kamigamo-motoyama, Kita-ku, Kyoto 603-8555, Japan.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25428499" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
  • 10
    facet.materialart.
    Unknown
    Denmark: Women's grants lost in inequality ocean (2015)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2015-03-13
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Watson, Darach -- Hjorth, Jens -- England -- Nature. 2015 Mar 12;519(7542):158. doi: 10.1038/519158d.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Niels Bohr Institute, University of Copenhagen, Denmark.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25762273" target="_blank"〉PubMed〈/a〉
    Keywords: Competitive Behavior ; Denmark ; Female ; Financing, Organized/*economics/*statistics & numerical data ; Humans ; Male ; Research/*economics/manpower ; Sex Distribution ; Sexism/economics/*statistics & numerical data ; *Women
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
    PAPER CURRENT
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...