scholarly journals MEAD: data reduction pipeline for ALES integral field spectrograph and LBTI thermal infrared calibration unit

Author(s):  
Zackery Briesemeister ◽  
Charles E. Woodward ◽  
Andrew J. Skemer ◽  
Jordan Stone ◽  
Philip M. Hinz ◽  
...  
1995 ◽  
Vol 149 ◽  
pp. 308-310
Author(s):  
V. V. Vlasiouk

Development of 3D spectral methods on the 6-meter telescope prompted the necessity of creating specialized software for data reduction, adapted to personal computers IBM AT/386/486 class. We had to concentrate our efforts on preparing the software for bidimensional spectral data produced by Multi-Pupil Integral Field Spectrograph of the 6-meter telescope (MPFS) and analog of panoramic spectrophotometer with spectral channeling, using scanning Fabry-Perot interferometer (PYTHEAS-6).MPFS - analog of spectrograph TIGER (Courtes et al., 1988), developed for the 6-meter telescope, provides bidimensional spectroscopy of extended sources, allowing the simultaneous detection of 99 individual spectra, produced by a lens raster from 9 by 11 microlenses. The main features of this instrument are described in (Afanasiev et al, 1994).


2012 ◽  
Vol 333 (2) ◽  
pp. 101-117 ◽  
Author(s):  
R.M. Barnsley ◽  
R.J. Smith ◽  
I.A. Steele

2015 ◽  
Author(s):  
Jorge Llop Sayson ◽  
Nargess Memarsadeghi ◽  
Michael W. McElwain ◽  
Qian Gong ◽  
Marshall Perrin ◽  
...  

Author(s):  
Timothy D. Brandt ◽  
Maxime Rizzo ◽  
Tyler Groff ◽  
Jeffrey Chilcote ◽  
Johnny P. Greco ◽  
...  

2019 ◽  
Vol 157 (2) ◽  
pp. 75 ◽  
Author(s):  
Kelly E. Lockhart ◽  
Tuan Do ◽  
James E. Larkin ◽  
Anna Boehle ◽  
Randy D. Campbell ◽  
...  

2010 ◽  
Author(s):  
Katherine B. Follette ◽  
Laird M. Close ◽  
Derek Kopon ◽  
Jared R. Males ◽  
Victor Gasho ◽  
...  

2020 ◽  
Vol 645 ◽  
pp. A12
Author(s):  
B. Balmaverde ◽  
A. Capetti ◽  
A. Marconi ◽  
G. Venturi ◽  
M. Chiaberge ◽  
...  

We present the final observations of a complete sample of 37 radio galaxies from the Third Cambridge Catalogue (3C) with redshift < 0.3 and declination < 20° obtained with the VLT/MUSE optical integral field spectrograph. These data were obtained as part of the MUse RAdio Loud Emission line Snapshot (MURALES) survey with the main goal of exploring the AGN feedback process in the most powerful radio sources. We present the data analysis and, for each source, the resulting emission line images and the 2D gas velocity field. Thanks to the unprecedented depth these observations reveal emission line regions (ELRs) extending several tens of kiloparsec in most objects. The gas velocity shows ordered rotation in 25 galaxies, but in several sources it is highly complex. We find that the 3C sources show a connection between radio morphology and emission line properties. In the ten FR I sources the line emission region is generally compact, only a few kpc in size; only in one case does it exceed the size of the host. Conversely, all but two of the FR II galaxies show large-scale structures of ionized gas. The median extent is 16 kpc with the maximum reaching a size of ∼80 kpc. There are no apparent differences in extent or strength between the ELR properties of the FR II sources of high and low gas excitation. We confirm that the previous optical identification of 3C 258 is incorrect: this radio source is likely associated with a quasi-stellar object at z ∼ 1.54.


Author(s):  
M. Mingozzi ◽  
G. Venturi ◽  
F. Mannucci ◽  
A. Marconi ◽  
G. Cresci

The central regions of Seyfert galaxies, comprising broad and narrow line regions and the inner parts of galaxy disk and bulge, is characterized by a complex interplay among many physical effects. Specifically, it is shaped by the influence of the central black hole, producing ionization by an hard continuum and gas outflows. The integral-field spectrograph MUSE at the ESO VLT allows to carry out a detailed study of these regions to obtain their ionization, dynamical, and metallicity properties. Here we present some highlights of the MAGNUM survey which is designed to study the central regions of a sample of nearby (D > 500 pc) Seyfert galaxies. We describe the rationale of the survey, the data analysis techniques used to extract information on ionization and dynamics, and the results for one galaxy, Centaurus A.


2018 ◽  
Vol 130 (988) ◽  
pp. 065001 ◽  
Author(s):  
Seth R. Meeker ◽  
Benjamin A. Mazin ◽  
Alex B. Walter ◽  
Paschal Strader ◽  
Neelay Fruitwala ◽  
...  

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