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Science Perspectives for 3D Spectroscopy

Overview of attention for book
Cover of 'Science Perspectives for 3D Spectroscopy'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 3D Instrumentation
  3. Altmetric Badge
    Chapter 2 3D-NTT: A New Instrument for the NTT Based on Versatile Tunable Filter Technology
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    Chapter 3 The Integral Field Unit of the Near Infrared Spectrograph for JWST
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    Chapter 4 Scientific Prospects of the 3D-NTT Instrument
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    Chapter 5 Handling IFU Datasets in the Virtual Observatory
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    Chapter 6 Simulations of High-z Starburst Galaxies for the JWST-MIRI Integral Field Unit
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    Chapter 7 IFUs: Disentangling the Light from Neighbour Fibers
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    Chapter 8 OSIRIS – a New Integral-Field Spectrograph at Keck Observatory
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    Chapter 9 A User–oriented Comparison of the Techniques for 3D Spectroscopy
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    Chapter 10 The Potential of Integral Field Spectroscopy Observing Extrasolar Planet Transits
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    Chapter 11 Solar System Objects with the NACO Fabry-Perot and SINFONI
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    Chapter 12 3D Spectroscopy with an Imaging FTS
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    Chapter 13 Nearby Galaxies: 3D Spectroscopy as a Tool, not as a Goal
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    Chapter 14 Nearby Galaxies Observed with the Kyoto Tridimensional Spectrograph II
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    Chapter 15 Scalable N-body Code for the Modeling of Early-type Galaxies
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    Chapter 16 Internal Kinematics of Galaxies: 3D Spectroscopy on Russian 6m Telescope
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    Chapter 17 SAURON Observations of Sa Bulges: The Formation of a Kinematically Decoupled Core in NGC5953
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    Chapter 18 Characterizing Stellar Populations in Spiral Disks
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    Chapter 19 The Stellar Populations of E and S0 Galaxies as Seen with SAURON
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    Chapter 20 VIMOS-IFU Spectroscopy of Extragalactic Star Forming Complexes
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    Chapter 21 Analyzing Non-circular Motions in Spiral Galaxies Through 3D Spectroscopy
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    Chapter 22 Harmonic Analysis of the Ha Velocity Field of NGC 4254
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    Chapter 23 The NIR Tully-Fisher Relation in Different Environments: the Importance of 3D Observations
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    Chapter 24 3D Kinematics of Local Galaxies and Fabry-Perot Database
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    Chapter 25 Validation of Stellar Population and Kinematical Analysis of Galaxies
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    Chapter 26 Non-Gravitational Motions in Galaxies
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    Chapter 27 Studying the Roots of the Supergalactic Wind in NGC 1569 with Gemini GMOS/IFUV
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    Chapter 28 Gravitational Lensing Studied with Integral Field Spectroscopy
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    Chapter 29 3D Spectroscopy as a Tool for Investigation of the BLR of Lensed QSOs
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    Chapter 30 A VIMOS-IFU Survey of z ∼ 0.2 Massive Lensing Galaxy Clusters: Constraining Cosmography
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    Chapter 31 First Results from the VIMOS-IFU Survey of Gravitationally Lensing Clusters at z ∼ 0.2
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    Chapter 32 Integral Field Spectroscopy of the Core of Abell 2218
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    Chapter 33 Velocity Fields of z∼0.6 Galaxies with GIRAFFE and Perspectives for ELTs
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    Chapter 34 News from the “Dentist’s Chair”: Observations of AM1353-272 with the VIMOS IFU
  36. Altmetric Badge
    Chapter 35 3D Spectroscopy of Low-z (Ultra)Luminous Infrared Galaxies
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    Chapter 36 Optical Spectra in the Non-Nuclear Regions of ULIRGs: Evidence of Ionization by Shocks
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    Chapter 37 Stellar Populations in the Galactic Center with SINFONI
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    Chapter 38 Stellar Populations in the Centers of Nearby Disk Galaxies
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    Chapter 39 AGN Shocks in 3D
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    Chapter 40 Young Kinematically Decoupled Components in Early-Type Galaxies
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    Chapter 41 SINFONI’s take on Star Formation, Molecular Gas, and Black Hole Masses in AGN
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    Chapter 42 The Unified Model in Nearby Seyfert Galaxies Through Integral Field Spectroscopy
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    Chapter 43 A 3D View of the Central Kiloparsec of the Seyfert Galaxy NGC 1358
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    Chapter 44 VLT/SINFONI Integral Field Spectroscopy of the Superantennae
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    Chapter 45 Integral-Field Observations of Centaurus A Nucleus
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    Chapter 46 The Puzzling Case of XBONGs: Will 3D-spectroscopy Explain Their True Nature?
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    Chapter 47 Studying of Some Seyfert Galaxies by Means of Panoramic Spectroscopy
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    Chapter 48 3D Spectroscopy of Emission Nebulae
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    Chapter 49 GMOS-IFU Observations of LV2
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    Chapter 50 The Enigma of Ultraluminous X-ray Sources may be Resolved by 3D-Spectroscopy (MPFS Data)
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    Chapter 51 Spatially Resolved Spectroscopy of Abell 30
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    Chapter 52 Constraining the Galactic Structure with Stellar Clusters in Obscured Hii Regions
  54. Altmetric Badge
    Chapter 53 Integral Field Spectroscopy of a Peculiar Supernova Remnant MF16 in NGC6946
  55. Altmetric Badge
    Chapter 54 SN 1987A: A Complex Physical Laboratory
  56. Altmetric Badge
    Chapter 55 3D-Spectroscopy of Extragalactic Planetary Nebulae as Diagnostic Probes for Galaxy Evolution
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    Chapter 56 3D Spectroscopy of Herbig-Haro Objects
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    Chapter 57 High Mass Star Formation In The Light Of Sinfoni
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    Chapter 58 Internal Kinematics of IIZw40
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    Chapter 59 Integral Field Spectroscopy Survey of Classical LBV Stars in M33
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    Chapter 60 Unravelling the Chemical Inhomogeneity of Planetary Nebulae with VLT FLAMES
  62. Altmetric Badge
    Chapter 61 Integral Field Spectroscopy of Galaxy Emission Line Haloes
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    Chapter 62 Integral Field Spectroscopy of Galaxies in the Distant Universe
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    Chapter 63 Integral-Field Studies of the High-Redshift Universe
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    Chapter 64 3D Kinematics of High-z Galaxies as Seen Through the Gravitational Telescope
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    Chapter 65 AGN Feedback at High Redshift: Shaping the Most Massive Galaxies?
  67. Altmetric Badge
    Chapter 66 Integral Field Observations of a Distant Cluster
Overall attention for this book and its chapters
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (89th percentile)
  • High Attention Score compared to outputs of the same age and source (90th percentile)

Mentioned by

blogs
1 blog

Citations

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3 Dimensions

Readers on

mendeley
3 Mendeley
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Title
Science Perspectives for 3D Spectroscopy
Published by
ADS, December 2007
DOI 10.1007/978-3-540-73491-8
ISBNs
978-3-54-073490-1, 978-3-54-073491-8
Editors

Kissler-Patig, Markus, Walsh, Jeremy R., Roth, Martin M.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 3 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 3 100%

Demographic breakdown

Readers by professional status Count As %
Other 1 33%
Student > Ph. D. Student 1 33%
Unknown 1 33%
Readers by discipline Count As %
Earth and Planetary Sciences 1 33%
Physics and Astronomy 1 33%
Unknown 1 33%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 9. 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 25 September 2017.
All research outputs
#3,317,701
of 23,041,514 outputs
Outputs from ADS
#2,271
of 37,451 outputs
Outputs of similar age
#13,648
of 156,790 outputs
Outputs of similar age from ADS
#42
of 462 outputs
Altmetric has tracked 23,041,514 research outputs across all sources so far. Compared to these this one has done well and is in the 84th percentile: it's in the top 25% of all research outputs ever tracked by Altmetric.
So far Altmetric has tracked 37,451 research outputs from this source. They receive a mean Attention Score of 4.6. This one has done particularly well, scoring higher than 92% 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 156,790 tracked outputs that were published within six weeks on either side of this one in any source. This one has done well, scoring higher than 89% of its contemporaries.
We're also able to compare this research output to 462 others from the same source and published within six weeks on either side of this one. This one has done particularly well, scoring higher than 90% of its contemporaries.