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AIPS++

Astronomical Image Processing System ++ is a software package whose development was started in the early nineties, written almost entirely in C… Expand
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AIPSC++

Papers overview

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2019
2019
Bayesian Reconstruction through Adaptive Image Notion
A stable and unique solution to the ill-posed inverse problem in radio synthesis image analysis is sought employing Bayesian… Expand
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2017
2017
eXtended CASA Line Analysis Software Suite (XCLASS)
The eXtended CASA Line Analysis Software Suite (XCLASS) is a toolbox for the Common Astronomy Software Applications package (CASA… Expand
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2016
2016
Jet speeds and flares in SS 433
We present new high-resolution, multi-epoch, VLBA radio images of the Galactic microquasar SS 433. We are able to observe plasma… Expand
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2016
2016
Direct detection of precursors of gas giants formed by gravitational instability with the atacama large millimeter/submillimeter array
Phases of gravitational instability are expected in the early phases of disk evolution, when the disk mass is still a substantial… Expand
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2015
2015
What is a GMC? Are observers and simulators discussing the same star-forming clouds?
As both simulations and observations reach the resolution of the star-forming molecular clouds, it becomes important to clarify… Expand
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Highly Cited
2014
Highly Cited
2014
UVMULTIFIT: A versatile tool for fitting astronomical radio interferometric data
Context. The analysis of astronomical interferometric data is often performed on the images obtained after deconvolving the… Expand
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2014
2014
ALMA service data analysis and level 2 quality assurance with CASA
The Atacama Large mm and sub-mm Array (ALMA) radio observatory is one of the world’s largest astronomical projects. After the… Expand
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2013
2013
Evidence of a SiO collimated outflow from a massive YSO in IRAS 17233–3606
Studies of molecular outflows in high-mass young stellar objects reveal important information about the formation process of… Expand
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Highly Cited
2012
Highly Cited
2012
Trapping dust particles in the outer regions of protoplanetary disks
Aims. We attempt to explain grain growth to mm sized particles and their retention in the outer regions of protoplanetary disks… Expand
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2010
2010
CASA: Common Astronomy Software Applications
 
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