scholarly journals Integral Field Spectroscopy of the Extended Emission‐Line Region of 4C 37.43

2007 ◽  
Vol 666 (2) ◽  
pp. 794-805 ◽  
Author(s):  
Hai Fu ◽  
Alan Stockton
Keyword(s):  
Emission Line ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Line Region ◽  
Integral Field ◽  
Extended Emission

scholarly journals Photoionization, line emission diagnostics

2013 ◽  
Vol 9 (S304) ◽  
pp. 18-18
Author(s):  
Lisa Kewley
Keyword(s):  
Emission Line ◽  
Radiation Field ◽  
Line Emission ◽  
Narrow Line ◽  
Ionization State ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Line Region ◽  
Narrow Line Region ◽  
Integral Field

AbstractPhotoionization models for AGN, including Seyfert and LINERs are discussed. These photoionization models can be used to derive emission-line diagnostics for AGN that can determine the properties of the AGN and surrounding ISM, including the relative AGN contribution to the EUV radiation field, the hardness of the AGN radiation field, the ionization state of the gas, and the metallicity of the narrow-line region. It is shown how the AGN emission-line diagnostics are expected to change with redshift. Finally, latest application of these models by the author to wide integral field spectroscopy to separate starburst and AGN contributions in composite galaxies are presented.

First results of the DIVING3D survey of bright galaxies in the local universe: The mini-DIVING3D sample

2019 ◽  
Vol 15 (S359) ◽  
pp. 450-451
Author(s):  
R. B. Menezes ◽  
J. E. Steiner ◽  
T. V. Ricci ◽  
Patrícia da Silva ◽  
D. M. Nicolazzi
Keyword(s):  
Emission Line ◽  
High Spatial Resolution ◽  
H Ii Regions ◽  
Local Universe ◽  
Composite Systems ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Line Region ◽  
First Results ◽  
Integral Field

AbstractWe present the first results of the Deep Integral Field Spectroscopy View of Nuclei of Galaxies (DIVING3D) survey, obtained from the analysis of the nuclear emission-line spectra of a sub-sample we call mini-DIVING3D, including all southern galaxies with B < 11.2 and |b| >15°. In comparison with previous studies, very few galaxies were classified as Transition objects. A possible explanation is that at least part of the Transition objects are composite systems, with a central low-ionization nuclear emission-line region (LINER) contaminated by the emission from circumnuclear H II regions. The high spatial resolution of the DIVING3D survey allowed us to isolate the nuclear emission from circumnuclear contaminations, reducing the number of Transition objects.

scholarly journals Mapping the Dynamics of the Quasar 3C 48

2001 ◽  
Vol 205 ◽  
pp. 162-165
Author(s):  
Eleni T. Chatzichristou
Keyword(s):  
Emission Line ◽  
Radio Source ◽  
Star Forming ◽  
Physical Conditions ◽  
Star Forming Regions ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Ir Emission ◽  
Integral Field ◽  
Extended Emission

The archetypical, nearby (z=0.37) quasar 3C 48 is an unusual CSS radio source with excess far-IR emission, whose one-sided radio jet is aligned with the extended ionized emission and a putative second nucleus. Because of its high AGN luminosity and proximity, 3C 48 is a good candidate to search for kinematic signatures of the radio jet-gas coupling and/or of a recent interaction. The radio morphology and our ground-based integral field spectroscopy suggest that the jet is interacting with its immediate environment. Using STIS aboard HST in several slit positions within the central 1”, we map the kinematics and physical conditions of the extended emission line gas and their relations to near-nuclear star forming regions found in existing HST images.

scholarly journals Imaging FTS: A Different Approach to Integral Field Spectroscopy

2014 ◽  
Vol 2014 ◽  
pp. 1-15 ◽  
Author(s):  
Laurent Drissen ◽  
Laurie Rousseau-Nepton ◽  
Sébastien Lavoie ◽  
Carmelle Robert ◽  
Thomas Martin ◽  
...  
Keyword(s):  
Fourier Transform ◽  
Emission Line ◽  
Absorption Line ◽  
Spiral Galaxy ◽  
Hyperspectral Imagery ◽  
Fourier Transform Spectroscopy ◽  
Wide Field ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

Imaging Fourier transform spectroscopy (iFTS) is a promising, although technically very challenging, option for wide-field hyperspectral imagery. We present in this paper an introduction to the iFTS concept and its advantages and drawbacks, as well as examples of data obtained with a prototype iFTS, SpIOMM, attached to the 1.6 m telescope of the Observatoire du Mont-Mégantic: emission line ratios in the spiral galaxy NGC 628 and absorption line indices in the giant elliptical M87. We conclude by introducing SpIOMM's successor, SITELLE, which will be installed at the Canada-France-Hawaii Telescope in 2014.

scholarly journals Orientation of galactic bulge planetary nebulae toward the Galactic center

2014 ◽  
Vol 10 (S312) ◽  
pp. 128-130
Author(s):  
Ashkbiz Danehkar ◽  
Quentin A. Parker
Keyword(s):  
Emission Line ◽  
Galactic Center ◽  
Planetary Nebulae ◽  
Wide Field ◽  
Spatially Resolved ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
National University ◽  
Hα Emission ◽  
Integral Field

AbstractWe have used the Wide Field Spectrograph on the Australian National University 2.3-m telescope to perform the integral field spectroscopy for a sample of the Galactic planetary nebulae. The spatially resolved velocity distributions of the Hα emission line were used to determine the kinematic features and nebular orientations. Our findings show that some bulge planetary nebulae toward the Galactic center have a particular orientation.

scholarly journals Resolving the coronal line region of NGC 1068 with near-infrared integral field spectroscopy★

2013 ◽  
Vol 430 (3) ◽  
pp. 2411-2426 ◽  
Author(s):  
X. Mazzalay ◽  
A. Rodríguez-Ardila ◽  
S. Komossa ◽  
Peter J. McGregor
Keyword(s):  
Near Infrared ◽  
Coronal Line ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Line Region ◽  
Ngc 1068 ◽  
Integral Field
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