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Camille Stock

Name:  Camille Stock

Title:  PhD student

E-mail:  cstock@cp.dias.ie

Phone:  +353-1-4406656

Address:  Astronomy & Astrophysics Section, 31 Fitzwilliam Place Dublin 2, D02 XF86

Maria Moutzouri

Name:  Maria Moutzouri

Title:  PhD student

E-mailmoutzouri@cp.dias.ie

Phone:  +353-1-4406656×331

Address:  Astronomy & Astrophysics Section, 31 Fitzwilliam Place Dublin 2, D02 XF86

Aybike Ozer

Name: Aybike Ozer

Title(s): Scholar

Email:  aybike@stp.dias.ie

Phone: + 353 1 6140145

Address: 10 Burlington Road, Dublin 4, D04 C932.

Eamon O’Gorman

Title: Dr Eamon O’Gorman

E-Mail: ogorman@cp.dias.ie

Phone: +353 1 4406656 extn 352

Address: School of Cosmic Physics, Astronomy & Astrophysics Section, 31 Fitzwilliam Place, Dublin 2

Research Interests: Radio emission from red supergiants, AGB stars, red giants, and exoplanets.

Biographical Sketch :
Eamon studied theoretical physics at University College Dublin and then  moved to Strasbourg, France where he received a masters degree in Space Studies at the International Space University.  He then moved back to Dublin and received his PhD from Trinity College Dublin where he studied the winds of evolved stars at radio wavelengths. After this he obtained a post-doctoral position at Onsala Space Observatory in Sweden where he continued his research and became a member of the ALMA Nordic Node. He is now an IRC postdoctoral research fellow at the Dublin Institute of Advanced Studies and his research is focused on high angular resolution radio observations of evolved stars using ALMA, JVLA, and LOFAR.

Selected Publications :
1) Temporal evolution of the size and temperature of Betelgeuse’s extended atmosphere (http://adsabs.harvard.edu/abs/2015A%26A…580A.101O)
2) Resolving the stellar activity of the Mira AB binary with ALMA (http://adsabs.harvard.edu/abs/2015A%26A…577L…4V)
3) ALMA observations of anisotropic dust mass loss in the inner circumstellar environment of the red supergiant VY Canis Majoris (http://adsabs.harvard.edu/abs/2015A%26A…573L…1O)
4) Multi-wavelength Radio Continuum Emission Studies of Dust-free Red Giants (http://adsabs.harvard.edu/abs/2013AJ….146…98O)
5) CARMA CO(J = 2 – 1) Observations of the Circumstellar Envelope of Betelgeuse (http://adsabs.harvard.edu/abs/2012AJ….144…36O)

Donna Rodgers-Lee

Name: Donna Rodgers-Lee
Title: PhD. student
E-Mail: donna@cp.dias.ie
Phone: +353 1 662 1333 ext 310
Address: Astronomy & Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, Ireland

Research Interests:
Weakly ionised plasmas, protoplanetary disks, low energy cosmic rays.
Biographical Sketch:
Donna Rodgers-Lee graduated from TCD in theoretical physics in 2011.
She is currently undertaking her PhD on protoplanetary disk evolution using multifluid magnetohydrodynamic simulations, as well as observations.

Selected Publications:
The Herschel view of circumstellar discs: a multiwavelength study of Chamaeleon-I
(ADS link:http://adsabs.harvard.edu/abs/2014MNRAS.443.1587R)

Alessio Caratti o Garatti

alessio

Name: Dr Alessio Caratti o Garatti

Title: Researcher

E-Mail: alessio@cp.dias.ie

Phone: +353 1 4406656 ext. 342
Address: DIAS, A&A Section, 31 Fitzwilliam Place, Dublin 2, Ireland

Related Links: http://www.researchgate.net/profile/Alessio_Caratti_o_Garatti

Publication list: http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?library&libname=Alessio+Caratti+o+Garatti&libid=55ec9d6e9b

Research Interests ): Star formation, protostellar jets & disks, low-mass and high-mass YSOs, optical-infrared interferometry.

Biographical Sketch:
Alessio Caratti o Garatti got degree in Physics at Univeristy of Rome “La Sapienza” (2001), and completed his PhD in Astronomy at the University of Rome “Tor Vergata” (2006). He worked on protostellar jets in the NIR (2006-2008) as an experienced researcher in the FP6 Marie Curie Research & Training Network ‘JETSET’ (at the Thüringer Landessternwarte Tautenburg, Tautenburg, Germany). As a post-dcotoral researcher, he worked in the ‘Spitzer Gould Belt Survey Legacy’ at the Dublin Institute for Advanced Studies (2009-2011) and in infrared interferometry of YSOs at the Max Planck Institute for Radioastronomy in Bonn, Germany (2012-2014). From 2014 he is working again at DIAS where he is involved in the scientific exploitation of GRAVITY at VLTI and MIRI on the JWST.

Selected Publications:

Caratti o Garatti A. et al. “Tracing jet emission at the base of a high-mass YSO. First AMBER/VLTI observations of the Brγ emission in IRAS 13481-6124” 2016, A&A 589, L4 http://adsabs.harvard.edu/abs/2016A%26A…589L…4C

Caratti o Garatti A. et al. “AMBER/VLTI high spectral resolution observations of the Brγ emitting region in HD 98922. A compact disc wind launched from the inner disc region” 2015, A&A 582, A44 http://adsabs.harvard.edu/abs/2015A%26A…582A..44C

Caratti o Garatti A. et al. “A near-infrared spectroscopic survey of massive jets towards extended green objects” 2015, A&A 572, A82 http://adsabs.harvard.edu/abs/2015A%26A…573A..82C

Caratti o Garatti A., Garcia Lopez R., et al. “The outburst of an embedded low-mass YSO in L1641” 2011 A&A 526, L1 http://adsabs.harvard.edu/abs/2011A%26A…526L…1C

Caratti o Garatti A. et al. “H2 active jets in the near IR as a probe of protostellar evolution” 2006, A&A 449, 1077

Carlo Romoli

picture_carloromoliName: Carlo Romoli
Title: PhD Student
E-Mail: romolic@cp.dias.ie
Phone: +353-1-4406656 x331
Address: 31, Fitzwilliam Place, Dublin 2, D02 XF86, Ireland

Related Links: https://www.linkedin.com/in/carlorml87

Research Interests: high energy astrophysics, gamma ray astronomy, active galactive nuclei

Biographical Sketch :
Carlo graduated in Physics in Padova in 2009 then he obtained in 2012 a master degree in physics at the same university with a focus on astrophysics. Since the end of the 2012 he is a PhD student in the high energy astrophysics group at the Dublin Institute for Advanced Studies working on the study of bright gamma ray emitters at high and very high energies.

Selected Publications:
Romoli, C.; Bordas, P.; Mariaud, C.; Murach, T.; Aharonian, F.; de Naurois, M.; Pühlhofer, G.; Schwanke, U.; van Soelen, B.; Sushch, I.; Zabalza, V.; for the H. E. S. S. Collaboration – “H.E.S.S. observations of PSR B1259-63 during its 2014 periastron passage”, http://adsabs.harvard.edu/abs/2015arXiv150903090R

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Patrick Kavanagh

Paddy-1Name: Dr. Patrick Kavanagh

Title: Researcher/MIRI software developer

E-Mail: pkavanagh@cp.dias.ie

Phone: +353 1 4406656 ext 336

Address: 31 Fitzwilliam Place, D02-XF86

Related Links: https://www.researchgate.net/profile/Patrick_Kavanagh2

Research Interests: X-ray observations of supernova remnants, superbubbles, hot interstellar medium

Biographical Sketch:
Patrick studied Physics and Physics Technology at Dublin Institute of Technology. He moved to Dublin City University where he was awarded his PhD for his research on the study of X-rays from the youngest Galactic massive star clusters in 2011. He then obtained a post-doctoral position at the University of Tuebingen, Germany, where he focused on high-energy studies of supernova remnants, superbubbles and the hot interstellar medium. At the beginning of 2016 he moved to the Dublin Institute for Advanced Studies where he continues his research and works as a software developer for the Mid-Infrared Instrument on the James Webb Space Telescope. He also contributes as an external collaborator to the German/Russian eROSITA mission and is a member of the ‘Supernova Remnants and Interstellar Medium’ science working group for the European Space Agency’s Athena mission.

Selected Publications:

Two evolved supernova remnants with newly identified Fe-rich cores in the Large Magellanic Cloud
Kavanagh, P. J.
; Sasaki, M.; Bozzetto, L. M.; et al.
http://adsabs.harvard.edu/abs/2016A%26A…586A…4K

Evidence for a binary origin of a central compact object
Doroshenko, V; Puehlhofer, G; Kavanagh, P. J.; et al.
http://adsabs.harvard.edu/abs/2016MNRAS.458.2565D

The population of X-ray supernova remnants in the Large Magellanic Cloud
Maggi, P.; Haberl, F.; Kavanagh, P. J.; et al.
http://adsabs.harvard.edu/abs/2016A%26A…585A.162M

Multi-frequency study of the newly confirmed supernova remnant MCSNR J0512-6707 in the Large Magellanic Cloud
Kavanagh, P. J.; Sasaki, M.; Bozzetto, L. M.; et al.
http://adsabs.harvard.edu/abs/2015A%26A…583A.121K

XMM-Newton study of 30 Doradus C and a newly identified MCSNR J0536-6913 in the Large Magellanic Cloud
Kavanagh, P. J.; Sasaki, M.; Bozzetto, L. M.; et al.

Ruben Fedriani Lopez

lopez

Title: PhD student
E-Mail: fedriani@cp.dias.ie
Phone: +353-1-4406656 x313
Address: Astronomy & Astrophysics Section, 31 Fitzwilliam Place Dublin 2,
Related Links (optional – e.g. personal pages, full CV, full ist of publications):
Research Interests: Star Formation, Protostellar Jets, Massive Young Stellar Objects (MYSOs)

Biographical Sketch:
Ruben Fedriani Lopez studied Mathematics at University of Cadiz (Spain), Saarland University (Germany) and Complutense University of Madrid (Spain). He completed his master degree in Astrophysics at Complutense University of Madrid. During his master, he did a Traineeship at the European Space Astronomy Centre (ESAC) working on M dwarfs using Virtual Observatory tools. On October 2015 he started his PhD on massive star formation studying the connection between the inner structure of MYSOs and their parsec scale jets.

Andrew Castillo Taylor

ID_photo2-1Name: Dr. Andrew Castillo Taylor

Title: Schrödinger Fellow

E-Mail: taylora@cp.dias.ie

Phone:  +353 1 4406656 extn 337

Address: 31 Fitzwilliam Place, Dublin 2, D02-XF86

Related Links: https://homepages.dias.ie/~taylora/

Research Interests: High Energy Astrophysics, Gamma-Rays, AGN, Neutrinos, Cosmic-Rays

Biographical Sketch : The high energy physics group at DIAS focuses
on astrophysical accelerators and the secondary particles they produce. Utilising data from space-based gamma-ray
detectors, as well as ground-based Cherenkov arrays such as the H.E.S.S. in Namibia, an abundance of efficient
astrophysical accelerators is currently being revealed. One of the connected aims of this research is to determine the
sources of the accelerated cosmic rays observed to arrive at Earth, both from Galactic and extragalactic origins.

Selected Publications:

http://arxiv.org/abs/astro-ph/0407618
http://arxiv.org/abs/astro-ph/0608085
https://arxiv.org/abs/1101.0932
https://arxiv.org/abs/1107.2055
https://arxiv.org/abs/1603.07730