scholarly journals Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy – I. Morphology and mass inventory★

2012 ◽  
Vol 428 (3) ◽  
pp. 2389-2406 ◽  
Author(s):  
X. Mazzalay ◽  
R. P. Saglia ◽  
Peter Erwin ◽  
M. H. Fabricius ◽  
S. P. Rusli ◽  
...  
Keyword(s):  
Molecular Gas ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Mass Inventory ◽  
Nearby Galaxies ◽  
Integral Field

scholarly journals Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy – II. Kinematics★

2014 ◽  
Vol 438 (3) ◽  
pp. 2036-2064 ◽  
Author(s):  
X. Mazzalay ◽  
W. Maciejewski ◽  
P. Erwin ◽  
R. P. Saglia ◽  
R. Bender ◽  
...  
Keyword(s):  
Molecular Gas ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Nearby Galaxies ◽  
Integral Field

scholarly journals Integral field spectroscopy of a sample of nearby galaxies

2011 ◽  
Vol 534 ◽  
pp. A8 ◽  
Author(s):  
E. Mármol-Queraltó ◽  
S. F. Sánchez ◽  
R. A. Marino ◽  
D. Mast ◽  
K. Viironen ◽  
...  
Keyword(s):  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Nearby Galaxies ◽  
Integral Field

scholarly journals The Hector Survey: integral field spectroscopy of 100,000 galaxies

2014 ◽  
Vol 10 (S309) ◽  
pp. 21-28 ◽  
Author(s):  
J. Bland-Hawthorn
Keyword(s):  
Galaxy Evolution ◽  
Scientific Impact ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Nearby Galaxies ◽  
Unique Parameter ◽  
Integral Field Spectrograph ◽  
New Facility ◽  
Larger Sample ◽  
Integral Field

AbstractIn March 2013, the Sydney–AAO Multi-object Integral field spectrograph (SAMI) began a major survey of 3400 galaxies at the AAT, the largest of its kind to date. At the time of writing, over a third of the targets have been observed and the scientific impact has been immediate. The Manga galaxy survey has now started at the SDSS telescope and will target an even larger sample of nearby galaxies. In Australia, the community is now gearing up to deliver a major new facility called Hector that will allow integral field spectroscopy of 100 galaxies observed simultaneously. By the close of the decade, it will be possible to obtain integral field spectroscopy of 100,000 galaxies over 3000 square degrees of sky down to r=17 (median). Many of these objects will have HI imaging from the new ASKAP radio surveys. We discuss the motivation for such a survey and the use of new cosmological simulations that are properly matched to the integral field observations. The Hector survey will open up a new and unique parameter space for galaxy evolution studies.

scholarly journals Nature and physical properties of gas-mass selected galaxies using integral field spectroscopy

2019 ◽  
Vol 15 (S352) ◽  
pp. 326-330
Author(s):  
Leindert A. Boogaard
Keyword(s):  
Physical Properties ◽  
High Redshift ◽  
Formation Rate ◽  
Cosmic Time ◽  
Gas Content ◽  
Molecular Gas ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field ◽  
Cold Gas

AbstractMapping the molecular gas content of the universe is key to our understanding of the build-up of galaxies over cosmic time. Spectral line scans in deep fields, such as the Hubble Ultra Deep Field (HUDF), provide a unique view on the cold gas content out to high redshift. By conducting ‘spectroscopy-of-everything’, these flux-limited observations are sensitive to the molecular gas in galaxies without preselection, revealing the cold gas content of galaxies that would not be selected in traditional studies.In order to capitalize on the molecular gas observations, knowledge about the physical conditions of the galaxies detected in molecular gas, such as their interstellar medium conditions, is key. Fortunately, deep surveys with integral-field spectrographs are providing an unprecedented view of the galaxy population, providing redshifts and measurements of restframe UV/optical lines for thousands of galaxies.We present the results from the synergy between the ALMA Spectroscopic Survey of the HUDF (ASPECS), with deep integral field spectroscopy from the MUSE HUDF survey and multi-wavelength data. We discuss the nature of the galaxies detected in molecular gas without preselection and their physical properties, such as star formation rate and metallicity. We show how the combination of ALMA and MUSE integral field spectroscopy can constrain the physical properties in galaxies located around the main sequence during the peak of galaxy formation.

scholarly journals The relation between the radio jet and the near-IR line emission in Seyfert galaxies

2010 ◽  
Vol 6 (S275) ◽  
pp. 172-173
Author(s):  
Rogemar A. Riffel ◽  
Thaisa Storchi-Bergmann
Keyword(s):  
Line Emission ◽  
Seyfert Galaxies ◽  
Molecular Gas ◽  
Gas Emission ◽  
Ionized Gas ◽  
Integral Field Spectroscopy ◽  
Near Ir ◽  
Field Spectroscopy ◽  
Molecular Flux ◽  
Integral Field

AbstractWe used near-IR integral field spectroscopy, obtained with Gemini NIFS and GNIRS integral field units (IFUs), to map the ionized and molecular flux distributions and kinematics in the central few hundreds of parsecs of Seyfert galaxies. We conclude that the molecular gas emission can be considered a tracer of the feeding of the AGN, while the emission of the ionized gas a tracer of its feedback.

scholarly journals Integral field spectroscopy of a sample of nearby galaxies

2012 ◽  
Vol 546 ◽  
pp. A2 ◽  
Author(s):  
S. F. Sánchez ◽  
F. F. Rosales-Ortega ◽  
R. A. Marino ◽  
J. Iglesias-Páramo ◽  
J. M. Vílchez ◽  
...  
Keyword(s):  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Nearby Galaxies ◽  
Integral Field
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