Wide field, integral field spectroscopy at Dome C with an infrared Imaging FTS

2005 ◽  
Vol 14 ◽  
pp. 187-192 ◽  
Author(s):  
J. P. Maillard ◽  
C. Joblin
2010 ◽  
Vol 410 (1) ◽  
pp. 313-340 ◽  
Author(s):  
S. F. Sánchez ◽  
F. F. Rosales-Ortega ◽  
R. C. Kennicutt ◽  
B. D. Johnson ◽  
A. I. Diaz ◽  
...  

2016 ◽  
Vol 11 (S321) ◽  
pp. 288-288
Author(s):  
N. F. Boardman ◽  
A. Weijmans ◽  
R. C. E. van den Bosch ◽  
L. Zhu ◽  
A. Yildirim ◽  
...  

Much progress has been made in recent years towards understanding how early-type galaxies (ETGs) form and evolve. SAURON (Bacon et al. 2001) integral-field spectroscopy from the ATLAS3D survey (Cappellari et al. 2011) has suggested that less massive ETGs are linked directly to spirals, whereas the most massive objects appear to form from a series of merging and accretion events (Cappellari et al. 2013). However, the ATLAS3D data typically only extends to about one half-light radius (or effective radius, Re), making it unclear if this picture is truly complete.


2014 ◽  
Vol 2014 ◽  
pp. 1-15 ◽  
Author(s):  
Laurent Drissen ◽  
Laurie Rousseau-Nepton ◽  
Sébastien Lavoie ◽  
Carmelle Robert ◽  
Thomas Martin ◽  
...  

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.


2014 ◽  
Vol 10 (S312) ◽  
pp. 128-130
Author(s):  
Ashkbiz Danehkar ◽  
Quentin A. Parker

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.


2008 ◽  
Author(s):  
F. Gracia-Temich ◽  
B. García-Lorenzo ◽  
Y. Padilla-Michel ◽  
J. F. M. Escobar-Romero ◽  
J. J. Fuensalida ◽  
...  

2012 ◽  
Vol 541 ◽  
pp. A119 ◽  
Author(s):  
A. Fernández-Martín ◽  
D. Martín-Gordón ◽  
J. M. Vílchez ◽  
E. Pérez Montero ◽  
A. Riera ◽  
...  

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