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The Impact of HST on European Astronomy

Overview of attention for book
Cover of 'The Impact of HST on European Astronomy'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 The Impact of HST on European Astronomy
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    Chapter 2 HST Spectroscopy of the Hottest White Dwarfs
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    Chapter 3 Key Abundance Tracers in the UV: From the Lightest to the Heaviest
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    Chapter 4 UV Spectroscopy of Metal-Poor Massive Stars in the Small Magellanic Cloud
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    Chapter 5 Star Formation Histories of Resolved Galaxies
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    Chapter 6 HST’s View of the Youngest Massive Stars in the Magellanic Clouds
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    Chapter 7 Planetary Nebulae and Their Central Stars in the Magellanic Clouds
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    Chapter 8 A Look at Neutron Stars with HST: From Positions to Physics
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    Chapter 9 The HST Contribution to Neutron Star Astronomy
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    Chapter 10 Exotic Populations in Galactic Globular Clusters
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    Chapter 11 The Stellar Mass Function in Globular Clusters
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    Chapter 12 Early Phases of Protoplanetary Disk Evolution
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    Chapter 13 The Impact of HST on European Astronomy
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    Chapter 14 A Hubble View of Star Forming Regions in the Magellanic Clouds
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    Chapter 15 A Preliminary Budget for the Ionizing Photons in HII Regions of M51
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    Chapter 16 New HST Views at Old Stellar Systems
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    Chapter 17 Young Massive Star Clusters in the Era of the Hubble Space Telescope
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    Chapter 18 The Central Regions of Early-Type Galaxies
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    Chapter 19 Nuclear Star Clusters Across the Hubble Sequence
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    Chapter 20 Stellar Populations in the Outskirts of M31: The View from HST
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    Chapter 21 Variable Stars in “Nearby” Galaxies with HST
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    Chapter 22 Extremely Metal-Poor Star-Forming Dwarf Galaxies
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    Chapter 23 Resolved Stellar Populations in Nearby Galaxy Halos
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    Chapter 24 The Kinematics of Core and Cusp Galaxies: Comparing HST Imaging and Integral-Field Observations
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    Chapter 25 Resolving Extragalactic Star Clusters with HST/ACS
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    Chapter 26 Tracing Galaxy Evolution in Clusters and Groups at z ≈1
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    Chapter 27 The Dawn of Galaxies
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    Chapter 28 A Simple Physical Model for Young Galaxies in the Early Universe
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    Chapter 29 Diffuse Ionized Gas Halos Seen with HST
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    Chapter 30 The Host Galaxy Properties of Powerful Radio Sources Across Cosmic Time
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    Chapter 31 A New View of the Origin of the Radio-Quiet/Radio-Loud AGN Dichotomy?
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    Chapter 32 The Bright and the Dark Side of Malin 1
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    Chapter 33 Cluster Lensing with Hubble
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    Chapter 34 HST Observations of Gravitationally Lensed QSOs
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    Chapter 35 Study of Quasar Host Galaxies Combining HST/ACS Images and VLT Spectra
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    Chapter 36 Local Lyman α Emitters and Their Relevance to High Redshift Ones
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    Chapter 37 The HST View of Low Luminosity AGN
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    Chapter 38 The Black Hole Masses in Galactic Nuclei
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    Chapter 39 The HST/ACS Coma Cluster Treasury Survey
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    Chapter 40 Discovery of a Population of Evolved and Massive Galaxies at High Redshift
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    Chapter 41 Searching for High Redshift Galaxies Using Population Synthesis Models
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    Chapter 42 The ACS Grism Mode and ACS Grism Observations of Deep Fields and High z Ly- α Galaxies
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    Chapter 43 The Role of HST in the Study of Near- and Mid-infrared-selected Galaxies
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    Chapter 44 Large Scale Structure and Galaxy Evolution in COSMOS
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    Chapter 45 Mass Estimations of Supermassive Black Holes in Brightest Cluster Galaxies
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    Chapter 46 Near-UV Study of Active Galactic Nuclei with Advanced Camera for Surveys
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    Chapter 47 A Quantitative Analysis of the Morphology of Star Formation in a Sample of GOODS-HST/ACS Galaxies
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    Chapter 48 Visiting Hubble in Orbit
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    Chapter 49 HST and JWST: Present and Future
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    Chapter 50 Enabling Science with the Hubble Legacy Archive
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    Chapter 51 Advanced Calibration Using Physical Instrument Models: HST, VLT and Beyond
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    Chapter 52 The Hubble Constant and HST
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    Chapter 53 Recent Progress on the Cepheid Distance Scale with HST
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    Chapter 54 Seeing Dark Energy
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    Chapter 55 Closing Remarks
Overall attention for this book and its chapters
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About this Attention Score

  • Good Attention Score compared to outputs of the same age (70th percentile)
  • Above-average Attention Score compared to outputs of the same age and source (64th percentile)

Mentioned by

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1 X user
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2 Wikipedia pages

Citations

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4 Dimensions

Readers on

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5 Mendeley
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Title
The Impact of HST on European Astronomy
Published by
ADS, January 2010
DOI 10.1007/978-90-481-3400-7
ISBNs
978-9-04-813399-4, 978-9-04-813400-7
Editors

Macchetto, F. Duccio

X Demographics

X Demographics

The data shown below were collected from the profile of 1 X user who shared this research output. Click here to find out more about how the information was compiled.
Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 5 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Sweden 1 20%
Germany 1 20%
Unknown 3 60%

Demographic breakdown

Readers by professional status Count As %
Researcher 3 60%
Student > Ph. D. Student 1 20%
Student > Master 1 20%
Readers by discipline Count As %
Physics and Astronomy 5 100%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 4. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 14 May 2023.
All research outputs
#7,333,689
of 23,122,481 outputs
Outputs from ADS
#9,090
of 37,519 outputs
Outputs of similar age
#48,096
of 166,265 outputs
Outputs of similar age from ADS
#293
of 851 outputs
Altmetric has tracked 23,122,481 research outputs across all sources so far. This one has received more attention than most of these and is in the 67th percentile.
So far Altmetric has tracked 37,519 research outputs from this source. They receive a mean Attention Score of 4.6. This one has done well, scoring higher than 75% of its peers.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 166,265 tracked outputs that were published within six weeks on either side of this one in any source. This one has gotten more attention than average, scoring higher than 70% of its contemporaries.
We're also able to compare this research output to 851 others from the same source and published within six weeks on either side of this one. This one has gotten more attention than average, scoring higher than 64% of its contemporaries.