Institution
University of Hertfordshire
Education•Hatfield, United Kingdom•
About: University of Hertfordshire is a education organization based out in Hatfield, United Kingdom. It is known for research contribution in the topics: Galaxy & Population. The organization has 14455 authors who have published 23821 publications receiving 768488 citations.
Topics: Galaxy, Population, Star formation, Stars, Radio galaxy
Papers published on a yearly basis
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Alternatives1, John Innes Centre2, University of Bonn3, University of North Carolina at Chapel Hill4, University of Wisconsin-Madison5, University of Utah6, University of Southern California7, University of Edinburgh8, University of Warwick9, Harvard University10, University College Cork11, University of Queensland12, University of Hertfordshire13, University of Potsdam14, University of California, San Diego15, Goethe University Frankfurt16, University of California, San Francisco17, University of Delaware18, Uppsala University19, Medical University of Vienna20, J. Craig Venter Institute21, University of Hawaii at Manoa22, Leibniz Association23, University of Iowa24, University of Aberdeen25, Georgia Institute of Technology26, University of California, Berkeley27, University of Groningen28, Princeton University29, University of Marburg30, University of Illinois at Urbana–Champaign31, Saarland University32, Norwegian University of Life Sciences33, Massey University34, Toyama Prefectural University35, ETH Zurich36, University of Saskatchewan37, Rutgers University38, Scripps Research Institute39, University of Helsinki40, Texas A&M University41, National Institutes of Health42, Technical University of Berlin43, University of Otago44, University of Cambridge45, University of Alberta46, Michigan State University47, Hofstra University48
TL;DR: This review presents recommended nomenclature for the biosynthesis of ribosomally synthesized and post-translationally modified peptides (RiPPs), a rapidly growing class of natural products.
1,560 citations
Cooper University Hospital1, Rhode Island Hospital2, University of Birmingham3, Stony Brook University4, McMaster University5, University of Jena6, University of Pittsburgh7, St Thomas' Hospital8, University Hospital of Lausanne9, University of Minnesota10, St. Michael's Hospital11, University of Turin12, University of Hertfordshire13, Johns Hopkins University School of Medicine14, Harvard University15, NorthShore University HealthSystem16, Houston Methodist Hospital17
TL;DR: An update to the original Surviving Sepsis Campaign clinical management guidelines, “SurvivingSepsis Campaign Guidelines for Management of Severe Sepsis and Septic Shock,” published in 2004 is provided.
Abstract: Objective:To provide an update to the original Surviving Sepsis Campaign clinical management guidelines, “Surviving Sepsis Campaign Guidelines for Management of Severe Sepsis and Septic Shock,” published in 2004.Design:Modified Delphi method with a consensus conference of 55 international experts, s
1,507 citations
University of Auckland1, Deakin University2, Virginia Tech3, Commonwealth Scientific and Industrial Research Organisation4, Catholic University of Leuven5, Public Health Foundation of India6, Imperial College London7, Australian National University8, Washington University in St. Louis9, Brookings Institution10, University of Stirling11, University of London12, Harvard University13, University of Hertfordshire14, McGill University15, Drexel University16, Tehran University of Medical Sciences17, George Washington University18, Newcastle University19, Wellington Management Company20, Huazhong University of Science and Technology21, World Bank22, University of Cape Town23, University of Amsterdam24, University of Newcastle25
TL;DR: This work aims to demonstrate the efforts towards in-situ applicability of EMMARM, which aims to provide real-time information about concrete mechanical properties such as E-modulus and compressive strength.
1,480 citations
TL;DR: In this article, the authors reported evidence for a very energetic supernova (a hypernova), temporally and spatially coincident with a gamma-ray burst at redshift z=0.1685.
Abstract: Over the past five years evidence has mounted that long-duration (greater than 2s) gamma-ray bursts (GRBs), the most brilliant of all astronomical explosions, signal the collapse of massive stars in our Universe. This evidence, originally based on the probable association of one unusual GRB with a supernova, now includes the association of GRBs with regions of massive star-formation in distant galaxies, tantalizing evidence of supernova-like light-curve 'bumps' in the optical afterglows of several bursts, and lines of freshly synthesized elements in the spectra of a few X-ray afterglows. These observations support, but do not yet conclusively validate, models based upon the deaths of massive stars, presumably associated with core collapse. Here we report evidence for a very energetic supernova (a hypernova), temporally and spatially coincident with a GRB at redshift z=0.1685. The timing of the supernova indicates that it exploded within a few days of the GRB, strongly suggesting that core-collapse events can give rise to GRBs. Amongst the GRB central engine models proposed to-date, the properties of this supernova thus favour the collapsar model.
1,415 citations
TL;DR: The HI Nearby Galaxy Survey (THINGS) as discussed by the authors is a high spectral (≤52kms −1 ) and spatial (∼ 6 ′′ ) resolution survey of HI emission in 34 nearby galaxies obtained using the NRAO Very Large Array (VLA).
Abstract: We present “The HI Nearby Galaxy Survey (THINGS)”, a high spectral (≤52kms −1 ) and spatial (∼ 6 ′′ ) resolution survey of HI emission in 34 nearby galaxies obtained using the NRAO Very Large Array (VLA) The overarching scientific goal of THINGS is to investigate fundamental characteristics of the interstellar medium (ISM) related to galaxy morphology, star formation and mass distribution across the Hubble sequence Unique characteristics of the THINGS database are the homogeneous sensitivity as well as spatial and velocity resolution of the HI data which is at the limit of what can be achieved with the VLA for a significant number of galaxies A sample of 34 objects at distances 2 < D <15 Mpc (resulting in linear resolutions of ∼100 to 500pc) are targeted in THINGS, covering a wide range of star formation rates (∼ 10 −3 to 6 M⊙ yr −1 ), total HI masses MHI (001 to 14×10 9 M⊙), absolute luminosities MB (–115 to –217mag) and metallicities (75 to 92 in units of 12+log[O/H]) We describe the setup of the VLA observations, the data reduction procedures and the creation of the final THINGS data products We present an atlas of the integrated HI maps, the velocity fields, the second moment (velocity dispersion) maps and individual channel maps of each THINGS galaxy The THINGS data products are made publicly available through a dedicated webpage Accompanying THINGS papers address issues such as the small–scale structure of the ISM, the (dark) matter distribution in THINGS galaxies, and the processes leading to star formation Subject headings: surveys — galaxies: structure — galaxies: ISM — ISM: general — ISM: atoms — radio lines: galaxies
1,354 citations
Authors
Showing all 14539 results
| Name | H-index | Papers | Citations |
|---|---|---|---|
| Rob Ivison | 166 | 1161 | 102314 |
| Pete Smith | 156 | 2464 | 138819 |
| Matt J. Jarvis | 144 | 1064 | 85559 |
| Geoffrey Burnstock | 141 | 1488 | 99525 |
| Stephen R. Bloom | 134 | 747 | 71493 |
| David P. Lane | 129 | 568 | 90787 |
| David M. Alexander | 125 | 652 | 60686 |
| David J. Smith | 125 | 2090 | 108066 |
| Anthony Howell | 120 | 714 | 55075 |
| J. H. Hough | 117 | 904 | 89697 |
| Christine H. Foyer | 116 | 490 | 61381 |
| Steve P. McGrath | 115 | 483 | 46326 |
| Nial R. Tanvir | 112 | 877 | 53784 |
| John M. Davis | 110 | 790 | 51526 |
| P. van der Werf | 107 | 532 | 35342 |