Selaus nimekkeen mukaan kokoelmassa Rinnakkaistallenteet

Aineistot 6321-6340 / 19207

    • G2C2 - II. Integrated colour-metallicity relations for Galactic globular clusters in SDSS passbands 

      Takamiya Marianne; Vanderbeke Joachim; Gregg Michael; De Propris Roberto; West Michael J.; Peng Eric W.; Côté Patrick; Jordán Andrés; Ferrarese Laura; Baes Maarten; Blakeslee John P.
      <p> <span style="color: rgb(0, 0, 0); font-family: Times; font-size: medium;">We use our integrated Sloan Digital Sky Survey (SDSS) photometry for 96 globular clusters in g and z, as well as r and i photometry for a ...

    • [Ga-68]Ga-DOTA-Siglec-9 Detects Pharmacodynamic Changes of FAP-Targeted IL2 Variant Immunotherapy in B16-FAP Melanoma Mice 

      Li Xiang-Guo; Nicolini Valeria; Viitanen Riikka; Jalkanen Sirpa; Klein Christian; Roivainen Anne; Liljenbäck Heidi; Moisio Olli; Nayak Tapan; Richard Marine; Virtanen Helena
      Vascular adhesion protein-1 (VAP-1) is an inflammation-inducible adhesion molecule, which supports contact between leukocytes and inflamed endothelium. There is evidence that VAP-1 is involved in the recruitment of leukocytes ...

    • Gadolinium retention in gliomas and adjacent normal brain tissue: association with tumor contrast enhancement and linear/macrocyclic agents 

      Ek P.; Frantzén J.; Bobacka J.; Minn H.; Gardberg M.; Kiviniemi A.
      <p>Purpose: To quantitate gadolinium deposits in gliomas and adjacent normal brain specimens, and to evaluate their association with tumor contrast enhancement and the type of gadolinium-based contrast agent (GBCA) ...

    • Gaia Data Release 2 

      Shore S; Tolstoy E; Forveille T; Kotak R

    • Gaia16apd-a link between fast and slowly declining type I superluminous supernovae 

      Ł. Wyrzykowski; E. Y. Hsiao; T. Kangas; E. Kankare; J. Isern; M. D. Stritzinger; N. Elias-Rosa; S. Mattila; E. Cappellaro; A. Somero; L. Rhodes; M. B. Nielsen; J. Harmanen; J. M. Carrasco Martinez; P. Lundqvist; N. Blagorodnova; T. M. Reynolds; M. Fraser; L. K. Hardy; Z. Kołaczkowski; U. Burgaz
      We present ultraviolet (UV), optical and infrared photometry and optical spectroscopy of the type Ic superluminous supernova (SLSN) Gaia16apd (= SN 2016eay), covering its evolution from 26 d before the g-band peak to 234.1 ...

    • Gaia17biu/SN 2017egm in NGC 3191: The Closest Hydrogen-poor Superluminous Supernova to Date Is in a "Normal," Massive, Metal-rich Spiral Galaxy 

      Shappee BJ; Mauerhan J; Pooley D; Hu SM; Davis S; Stanek KZ; Bose S; Herczeg GJ; de Jaeger T; Hestenes J; Hsiao EY; Falco E; Hosseinzadeh G; Lundqvist P; Brown PJ; Jeffers B; Woo JH; Ochner P; Lau MW; Elias-Rosa N; Benetti S; Koff RA; Kumar S; Prentice S; Ashall C; Gall C; Jaejin S; Zheng WK; Stassun KG; Fraser M; Chen P; Holoien TWS; Rudy RJ; Kochanek CS; Brink TG; Cai Z; Villanueva S; Filippenko AV; Yunus S; Kurtenkov A; Post R; Dong SB; Mutel R; Gaudi BS; Cappellaro E; Somero A; Shahbandeh M; Mattila S; Reynolds T; Beswick RJ; Pastorello A; Valenti S; Romero-Canizales C; Thompson TA; Stritzinger MD; Prieto JL; Tomasella L; Grupe D
      Hydrogen-poor superluminous supernovae (SLSNe-I) have been predominantly found in low-metallicity, star-forming dwarf galaxies. Here we identify Gaia17biu/SN 2017egm as an SLSN-I occurring in a "normal" spiral galaxy (NGC ...

    • Gains From Training in Phonological Awareness in Kindergarten Predict Reading Comprehension in Grade 9 

      Kjeldsen AC; Niemi P; Karna A; Olofsson A; Witting K
      <p> The effects of a kindergarten training program in phonological awareness with 209 Swedish-speaking children were followed up until the end of Grade 9. Initial levels of letter knowledge and phonological awareness ...

    • Galactic cold cores VII. Filament formation and evolution: Methods and observational constraints 

      I. Ristorcelli; J. Malinen; N. Ysard; L. Montier; P. G. Martin; D. Ward-Thompson; A. Men’shchikov; J.-P. Bernard; L. Pagani; V.-M. Pelkonen; A. Marston; J. Montillaud; D. Paradis; R. Paladini; M. Juvela; A. Rivera-Ingraham; D. J. Marshall; L. V. Tóth
      Context. The association of filaments with protostellar objects has made these structures a priority target in star formation studies. However, little is known about the link between filament properties and their local ...

    • Galactic cold cores VIII. Filament formation and evolution: Filament properties in context with evolutionary models 

      Ristorcelli I; Ysard N; Ward-Thompson D; Pelkonen VM; Marston A; Montier L; Montillaud J; Rivera-Ingraham A; Martin PG; Bernard JP; Juvela M; Paladini R; Paradis D; Men'shchikov A; Pagani L; Toth LV; Malinen J; Marshall DJ
      Context. The onset of star formation is intimately linked with the presence of massive unstable filamentary structures. These filaments are therefore key for theoretical models that aim to reproduce the observed characteristics ...

    • Galactoglucomannan-rich hemicellulose extract from Norway spruce (Picea abies) exerts beneficial effects on chronic prostatic inflammation and lower urinary tract symptoms in vivo 

      Vuorikoski H; Holmbom B; Konkol Y; Bernoulli J; Tuomela J
      Galactoglucomannan (GGM) is the main hemicellulose class in wood of coniferous trees and could be potentially utilized as a possible health-promoting substance for food and pharmaceutical industry. Our aim was to evaluate ...

    • Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions 

      Raouf M; Cluver ME; Peacock JA; D'Eugenio F; Davies LJ; Norberg P; Seibert M; Bland-Hawthorn J; Drinkwater MJ; Haussler B; Taylor EN; Bamford SP; Bauer AE; Croom SM; Kelvin LS; Baldry IK; Lopez-Sanchez AR; Conselice CJ; Hashemizadeh A; Heymans C; Driver SP; Said K; Giblin B; de Jong J; Graham AW; Gunawardhana MLP; Grootes MW; Farrow DJ; Koushan S; Wright AH; Tuffs RJ; Holwerda BW; De Propris R; Radovich M; Hopkins AM; Frenk CS; Lara-Lopez MA; Moffett AJ; Jarrett TH; van Kampen E; Pimbblet KA; van der Wel A; Obreschkow D; Sansom AE; Popescu C; Loveday J; Wilkins SM; Brough S; Robotham ASG; Hildebrandt H; Dvornik A; Meyer M; Turner R; Liske J; Dogruel B; Bellstedt S; Mahajan S; Bravo M; Bilicki M; Owers MS; Lange R; Napolitano NR; Alpaslan M; Casura S; Jones DH; Kuijken K; Phillipps S; Sutherland WJ; Colless M; Thorne JE
      In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra, and, in combination with earlier surveys, results in 330 542 redshifts ...

    • Galaxy And Mass Assembly (GAMA): Defining passive galaxy samples and searching for the UV upturn 

      S Brough; S Phillipps; E N Taylor; B W Holwerda; M J I Brown; L Wang; M E Cluver; A E Sansom; M W Grootes; K Pimbblet; A S G Robotham; S P Driver; P A James; M N Bremer; S S Ali; M Alpaslan; L J M Davies; R De Propris; A M Hopkins
      We use data from the GAMA and GALEX surveys to demonstrate that the UV upturn, an unexpected excess of ultraviolet flux from a hot stellar component, seen in the spectra of many early-type galaxies, arises from processes ...

    • Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass 

      Hopkins AM; Lara-Lopez MA; Mahajan S; Moffett A; Prescott M; Robotham ASG; Obreschkow D; Liske J; Taylor EN; Cluver M; Bauer AE; Lopez-Sanchez AR; Holwerda BW; Driver SP; Penny SJ; Drinkwater MJ; Bland-Hawthorn J; Wilkins SM; Loveday J; Norberg P; Kelvin LS; Owers MS; Davies LJM; Pimbblet K; Baldry IK; Brough S; De Propris R; van Kampen E; Brown MJI; Agius NK; McNaught-Roberts T
      <p> We use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift sample to fully describe the stellar mass dependence of close pairs and mergers between 10(8) and 10(12)M(circle dot). Using the ...

    • Galaxy and Mass Assembly (GAMA): merging galaxies and their properties 

      Brough S; Kelvin L; Hopkins AM; Bland-Hawthorn J; Driver SP; Baldry IK; Robotham ASG; Loveday J; De Propris R; Phillipps S
      <p> We derive the close pair fractions and volume merger rates for galaxies in the Galaxy and Mass Assembly (GAMA) survey with -23 &lt; M-r &lt; -17 (Omega(M) = 0.27, Omega(A) = 0.73, H-0 = 100 km s(-1) Mpc(-1)) at 0.01 ...

    • Galaxy and Mass Assembly (GAMA): Morphological transformation of galaxies across the green valley 

      A Hopkins; Amanda J Moffett; J Liske; P A James; M N Bremer; S Phillipps; S P Driver; B Häußler; S Percival; R De Propris; B Holwerda; Rebecca Kennedy; S Bamford; E N Taylor; L S Kelvin; L J M Davies
      We explore constraints on the joint photometric and morphological evolution of typical low redshift galaxies as they move from the blue cloud through the green valley and on to the red sequence. We select Galaxy And Mass ...

    • Galaxy and mass assembly (GAMA): the consistency of GAMA and WISE derived mass-to-light ratios 

      Kelvin LS; Taylor EN; Phillipps S; Bremer MN; Kettlety T; Bland-Hawthorn J; Cluver ME; Driver SP; Brough S; Sutherland W; Holwerda BW; Hesling J; Wright AH; De Propris R
      Recent work has suggested that mid-IR wavelengths are optimal for estimating the mass-to-light ratios of stellar populations and hence the stellar masses of galaxies. We compare stellar masses deduced from spectral energy ...

    • Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1 < z < 0.35 

      De Propris R; Lopez-Sanchez AR; Baldry IK; Kotilainen J; Holwerda BW; Hopkins AM; Wang LY; Graham AW; Wright AH; Wethers CF; Brough S; Acharya N; Driver SP; Loveday J; Taylor E; Phillipps S; Pimbblet KA
      Understanding the connection between nuclear activity and galaxy environment remains critical in constraining models of galaxy evolution. By exploiting the extensive cataloged data from the Galaxy and Mass Assembly survey, ...

    • Galaxy and Mass Assembly (GAMA): time-scales for galaxies crossing the green valley 

      B. W. Holwerda; P. A. James; L. J. M. Davies; M. N. Bremer; M. E. Cluver; S. P. Driver; S. A. Eales; L. S. Kelvin; A. E. Sansom; S. Phillipps; R. De Propris; E. N. Taylor; A. M. Hopkins
      We explore the constraints that can be placed on the evolutionary time-scales for typical low-redshift galaxies evolving from the blue cloud through the green valley and on to the red sequence. We utilize galaxies from the ...

    • GAMA/XXL: X-ray point sources in low-luminosity galaxies in the GAMA G02/XXL-N field 

      Vignali C; McGee S; Maughan B; Pierre M; Brown MJI; Chiappetti L; De Propris R; Hopkins AM; Giles PA; Driver SP; Pacaud F; Bremer MN; Elyiv A; Nwaokoro E; Plionis M; Young AJ; Poggianti BM; Bongiorno A; Baldry I; Fotopoulou S; Phillipps S
      <p>Relatively few X-ray sources are known that have low-mass galaxies as hosts. This is an important restriction on studies of active galactic nuclei (AGNs), hence black holes, and of X-ray binaries (XRBs) in low-mass ...

    • Gamblification: A definition 

      Hamari Juho; Macey Joseph
      In recent years, gambling has become increasingly prominent in everyday life; the term 'gamblification' first emerged in the late 2000s and was used to describe the colonisation of sports and sporting cultures by the ...