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Invited Talks at IRAM/Granada
2010
Date	Speaker	Topic
May, 18th 16:30	Lourdes Verdes-Montenegro IAA	AMIGA - the interstellar medium of isolated galaxies
Feb 11 16:00	Helmut Wiesemeyer IRAM	VLBI and SgrA*
January, 26th 17:00	Pierre Gratier Observatoire Bordeaux	Wide-field high-resolution CO observations of Giant Molecular Clouds in M33
2009
Dec 3rd 17:00	Rainer Schodel IAA	At the Bottom of the Potential Well - The Galactic Center
November, 19 17:00	Jesus Martin-Pintado Madrid	Galactic Center Chemistry
August, 20 17:00	Marco Padovani Arcetri	Properties of prestellar cores: cosmic ray ionization and non-LTE effects
July, 16 17:00	Simon Verley UGR	Star formation in M33
July, 14 13:00	Carolyn McCoey University of Waterloo, Canada, HIFI Instrument Control Centre Support Scientist	The Herschel data reduction software HIPE and the current status of HIFI/Herschel
June, 23 17:00	Wolfgang Wild	The status of the Atacama Large Millimeter Array ALMA
Jun 18 15:00	Christof Buchbender	An In-Depth Study of the Interstellar Medium in the Barred Spiral Galaxy NGC3627
June 3rd 17:00	Rebeca Aladro	Chemical differences between two types of starburst galaxies
May 15th 13:00	Javier Adrian Rodon MPIA Heidelberg	The Core Mass Function of IRAS 19410+2336
May 5th 13:00	Manuel Gonzalez Garcia OBSPM	Infrared pumping of molecular lines in PDRs
2008
November 13th 13:00	Jeffrey Wagg	Submm-to-radio observations of molecular and atomic gas in massive high-redshift galaxies
October 29th 9.30am	Dr. Igor Zinchenko, Mr. Vadim Gimmelman and Mr. Yuri Artemenko	A 70m millimetric antenna in Plateau Suffa in Uzbekistan - The Suffa Project

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-Chemical differences between two types of starburst galaxies

by Rebeca Aladro

at 5 pm on June, 3rd

in the IRAM library

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The Core Mass Function of IRAS 19410+2336 

by Javier Adrian Rodon (MPIA Heidelberg)

on 15.5.2009 at 1pm

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Infrared pumping of molecular lines in PDRs

by Manuel Gonzalez Garcia (OBSPM)

14.5.2009 at 1pm

Abstract: 

The arrival of new instruments such as Herschel or ALMA opens new resarch
possibilities. Astrophysical models such as the Meudon PDR code will be
very important to prepare and analyse furure observations. We will explain
how we have improved the grain model of PDR Meudon code, by making an
interface with DUSTEM code. We will also explain that an exact computation
of the infrared pumping term has to be done if we want to accurately
describe excitation of some molecules, such as water. Finally we will show
how these improvements permits us to describe the objects S140 and M82. 

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Submm-to-radio observations of molecular and atomic gas in massive high-redshift galaxies

by Jeffrey Wagg

at 1 p.m. on November, 13, 2008

in the IRAM library

The current generation of large single-dish submm/radio-wavelength telescopes and interferometers have opened up the study of gas and dust in galaxies and AGN out to the epoch of reionization at z>6. The IRAM facilities have been at the forefront of this revolution, and I will present our most recent results of an ongoing survey of dust continuum emission and molecular CO line emission in z~6 quasars using the CSO, the IRAM 30m, the PdBI and the GBT. I will also present our first attempts at using observations of redshifted CO line emission as a means of measuring redshifts for dust-obscured submm galaxies. Finally, I will discuss some of the applications of redshifted atomic lines such as neutral and ionized Carbon for studying star-formation in the first galaxies. 

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A 70m millimetric antenna in Plateau Suffa in Uzbekistan - The Suffa Project

by Dr. Igor Zinchenko, Mr. Vadim Gimmelman and Mr. Yuri Artemenko

at 9:30 a.m. on October, 29th, 2008

in the IRAM library in Granada

-----
+ ||||||<tablewidth="80%">'''Invited Talks at IRAM/Granada''' ||
 ||||||<tablewidth="80%">'''2010'''||
 ||'''Date'''||'''Speaker'''||'''Topic''' ||
 ||<rowbgcolor="#FFFFE0"> May, 18th <<BR>> 16:30 ||Lourdes Verdes-Montenegro <<BR>> IAA|| AMIGA - the interstellar medium of isolated galaxies ||
 || Feb 11 <<BR>> 16:00 ||Helmut Wiesemeyer <<BR>> IRAM|| VLBI and SgrA* ||
 ||<rowbgcolor="#FFFFE0">January, 26th <<BR>> 17:00  || Pierre Gratier <<BR>> Observatoire Bordeaux || Wide-field high-resolution CO observations of Giant Molecular Clouds in M33 ||
 ||||||<tablewidth="80%">'''2009'''||
 || Dec 3rd <<BR>> 17:00 ||Rainer Schodel <<BR>> IAA|| At the Bottom of the Potential Well - The Galactic Center||
 ||<rowbgcolor="#FFFFE0">November, 19 <<BR>> 17:00 || Jesus Martin-Pintado <<BR>> Madrid || Galactic Center Chemistry ||
 || August, 20 <<BR>> 17:00 || Marco Padovani <<BR>> Arcetri || Properties of prestellar cores: cosmic ray ionization and non-LTE effects  ||
 ||<rowbgcolor="#FFFFE0"> July, 16 <<BR>> 17:00 || Simon Verley <<BR>> UGR || Star formation in M33  ||
 || July, 14 <<BR>> 13:00 || Carolyn !McCoey <<BR>> University of Waterloo, Canada, HIFI Instrument Control Centre Support Scientist || The Herschel data reduction software HIPE and the current status of HIFI/Herschel  ||
 ||<rowbgcolor="#FFFFE0"> June, 23 <<BR>> 17:00 || Wolfgang Wild || The status of the Atacama Large Millimeter Array ALMA  ||
 || Jun 18 <<BR>> 15:00 || Christof Buchbender || An In-Depth Study of the Interstellar Medium in the Barred Spiral Galaxy NGC3627 ||
 ||<rowbgcolor="#FFFFE0"> June 3rd <<BR>> 17:00 || Rebeca Aladro <<BR>> || Chemical differences between two types of starburst galaxies  ||
 || May 15th <<BR>> 13:00 || Javier Adrian Rodon <<BR>> MPIA Heidelberg || The Core Mass Function of IRAS 19410+2336  ||
 ||<rowbgcolor="#FFFFE0"> May 5th <<BR>> 13:00 || Manuel Gonzalez Garcia <<BR>> OBSPM ||Infrared pumping of molecular lines in PDRs   ||
 ||||||<tablewidth="80%">'''2008'''||
 || November 13th <<BR>> 13:00 || Jeffrey Wagg || Submm-to-radio observations of molecular and atomic gas in massive high-redshift galaxies ||
 ||<rowbgcolor="#FFFFE0"> October 29th <<BR>> 9.30am || Dr. Igor Zinchenko, Mr. Vadim Gimmelman and Mr. Yuri Artemenko || A 70m millimetric antenna in Plateau Suffa in Uzbekistan - The Suffa Project ||