Martino Romaniello’s home page

 
 
I
am an astronomer at the European Southern Observatory (ESO), stationed at the Headquarters in Garching bei München (Germany). Before joining ESO I was at the Space Telescope Science Institute in Baltimore (MD) and at the Scuola Normale Superiore in Pisa, where I got my PhD in October 1998.



Munich is a very nice city to live in, but it has notoriously terrible weather. This is why we have placed our telescopes in Northern Chile, where the sky is (virtually) always perfect (pictured here is the rather impressive Paranal Observatory in the Atacama desert).


Here in Garching I share my working time between my functional duties as responsible for ESO’s Back-end Operations Department and my own scientific research. Speaking of which, if you are an astronomer you might be interested in this web site of our collaboration on star formation and young stellar populations.




DISCLAIMER: any view or statement made is not part of an official standpoint of ESO.

 
In a nutshell First Name: Martino Last Name: Romaniello Occupation: Astronomer Employer: ESO, the European Southern Observatory e-mail address: mromanie at eso.org martino.romaniello at eso.org phone number: +49-(0)89-32006565 home page: www.eso.org/~mromanie (but I guess you knew this already) scientific interests: Star formation, mainly in external galaxies Resolved stellar populations, young and old Cepheids as distance indicators and tracers of galactic structure publications in refereed journals: Can be found here (link to the ADS). PhD Thesis: “Young Stellar Populations in the Large Magellanic Cloud: Surprises from HST Observations” is here (PDF file, 12 MB).

In a nutshell


First Name:

Martino


Last Name:

Romaniello


Occupation:

Astronomer


Employer:

ESO, the European Southern Observatory


e-mail address:

mromanie at eso.org

martino.romaniello at eso.org


phone number:

+49-(0)89-32006565


home page:

www.eso.org/~mromanie

(but I guess you knew this already)


scientific interests:

  1. Bullet Star formation, mainly in external galaxies

  2. Bullet Resolved stellar populations, young and old

  3. Bullet Cepheids as distance indicators and tracers of galactic structure


publications in refereed journals:

Can be found here (link to the ADS).


PhD Thesis:

“Young Stellar Populations in the Large Magellanic Cloud: Surprises from HST Observations” is here (PDF file, 12 MB).

About me