Conference program > Detailed program

Sunday, March 29, 2020

Time Event  
17:30 - 19:30 Welcome cocktail and registration  

Monday, March 30, 2020

Time Event  
08:30 - 09:00 Conference - registration  
09:00 - 09:10 Welcome - Karl SCHUSTER  
09:10 - 09:30 Status of IRAM observatories - Roberto NERI  
09:30 - 09:55 Understanding PDRs through multiline diagnostics - Javier GOICOECHEA (IS)  
09:55 - 10:10 HCN/HNC intensity ratio: a new chemical thermometer for the molecular ISM - Alvaro HACAR  
10:10 - 10:30 Gas phase Elemental abundances in Molecular cloudS (gems) - Asuncion FUENTE (LP)  
10:30 - 11:00 Coffee break (Salle Matisse)  
11:00 - 11:25 Isotopic ratios and fractionation in the local Universe - Serena VITI (IS)  
11:25 - 11:45 The IRAM 30m Nearby Galaxy Dense Gas Survey EMPIRE - Frank BIGIEL (LP)  
11:45 - 12:00 Probing the link between molecular clouds, star formation, and environment in nearby galaxies with multi-transition observations of dense gas tracers - Antonio USERO  
12:00 - 13:30 Lunch break  
13:30 - 13:55 The Atomic to Molecular (HI-to-H2) Transition in Galaxy Star-Forming Regions - Amiel STERNBERG (IS)  
13:55 - 14:15 A Cloud-Scale View of the Molecular Gas Disk in the Whirlpool Galaxy - Eva SCHINNERER (LP)  
14:15 - 14:30 Characterising the ISM of low metallicity galaxies: Quantifying the CO-dark gas reservoir with C+ - Suzanne MADDEN  
14:30 - 14:45 A Wide-area, Cloud-Scale ISM Survey of IC 342 - Andreas SCHRUBA  
14:45 - 15:00 A new tool to estimate the atomic and molecular ISM content using probability distributions - Thomas BISBAS  
15:00 - 15:15 ALCHEMI: Results from the ALMA Comprehensive High-resolution Extragalactic Molecular Inventory of NGC253 - Jeff MANGUM  
15:15 - 15:30 Cold and massive filaments in cool core clusters and groups - Valeria OLIVARES  
15:30 - 16:40 Poster session & Coffee break - Authors of poster contributions will be available for discussion. Room MATISSE (2nd floor).  
16:40 - 17:05 Molecular gas dynamics around nuclei of galaxies - Françoise COMBES (IS)  
17:05 - 17:20 Multi-scale dynamics in star-forming regions: the interplay between gravity and turbulence - Alessio TRAFICANTE  
17:20 - 17:35 High-velocity warm molecular gas close to Sgr A* - Miriam G. SANTA-MARIA  
17:35 - 17:50 Dynamically-regulated star formation in the strongly interacting Taffy galaxies - Axel GARCIA-RODRIGUEZ  

Tuesday, March 31, 2020

Time Event  
08:30 - 08:55 Astrochemistry at the dawn of star and planet formation - Paola CASELLI (IS)  
08:55 - 09:15 LEGO: A Cloud–Scale Line Survey to constrain Cosmic Star Formation - Jens KAUFFMANN (LP)  
09:15 - 09:30 Molecular-cloud-scale multi-line imaging toward W3(OH) in the 3 mm and 0.8 mm bands - Yuri NISHIMURA  
09:30 - 09:45 A complete 3mm line survey of the B1-b and TMC-1 cores - Nuria MARCELINO  
09:45 - 10:00 Multi-line characterization of whole molecular clouds using stratified random sampling - Mario TAFALLA  
10:00 - 10:15 Observable tracers of the ionization fraction - Emeric BRON  
10:15 - 10:45 Coffee break (Salle Matisse)  
10:45 - 11:10 Significance and evolution of molecular gas during the star formation noon - Reinhard GENZEL (IS)  
11:10 - 11:25 The rich molecular inventory of two dusty galaxies twelve billion years ago - Chentao YANG  
11:25 - 11:40 Gas properties in the Early Universe deciphered from spectral line surveys of high-z objects: the Cloverleaf quasar - Michel GUELIN  
11:40 - 11:55 Probing ISM properties and AGN feedback in the z=0-4 Universe with IRAM (and ALMA) - Manuela BISCHETTI  
11:55 - 12:15 z-GAL: A Comprehensive Redshift Survey of the Brightest Herschel Galaxies - Pierre COX (LP)  
12:15 - 13:45 Lunch break  
13:45 - 14:10 Molecular richness in protostars: lessons learnt from spectral observations - Ana LOPEZ SEPULCRE (IS)  
14:10 - 14:25 What can chemistry tell us about the initial conditions of star formation? - Siyi FENG  
14:25 - 14:40 From hot-corinos to comets: astrochemistry and the protostellar heritage - Eleonora BIANCHI  
14:40 - 15:05 Molecules from evolved stars and their role in the cycle of the ISM - Marcelino AGUNDEZ (IS)  
15:05 - 15:20 Streams, disk and chemistry in the S-type AGB star RS Cnc - Jan-Martin WINTERS  
15:20 - 15:35 CTB 109: How a supernova remnant affects a giant molecular cloud - Seamus CLARKE  
15:35 - 16:45 Coffee break & Poster session - Authors of poster contributions will be available for discussion. Room MATISSE (2nd floor).  
16:45 - 17:05 Fragmentation and disk formation in high-mass star formation: The NOEMA large program CORE - Henrik BEUTHER (LP)  
17:05 - 17:20 Photodissociation regions associated with massive dense dust clumps - Wonju KIM  
17:20 - 17:35 The Sulphur depletion problem in molecular clouds: the H2S case - David NAVARRO  
17:35 - 17:50 Investigation of the "dense gas tracers" within a massive star forming region - Ashley BARNES  
17:50 - 18:05 Enhanced nitrogen fractionation at core scales: the high-mass star-forming region IRAS 05358+3543 - Laura COLZI  
20:00 - 23:55 Conference dinner NEGRESCO  

Wednesday, April 1, 2020

Time Event  
08:30 - 08:55 Feedback from young stars, the molecular signature of shocks and outflows - Sylvie CABRIT (IS)  
08:55 - 09:10 Interstellar Complex Organic Molecules in the NGC 1333 IRAS 4A Outflows - Marta DE SIMONE  
09:10 - 09:25 Are jets ubiquitous in young forming stars? CALYPSO IRAM-PdBI survey of jets in Class 0/I protostars - Linda PODIO  
09:25 - 09:45 ASAI - Charlotte VASTEL (LP)  
09:45 - 10:10 Molecular Diagnostics of Disk Forming Regions - Satoshi YAMAMOTO (IS)  
10:10 - 10:40 Coffee break  
10:40 - 11:05 Chemical richness of protoplanetary disks and related physical properties - Anne DUTREY (IS)  
11:05 - 11:20 Chemical, morphological and dynamical study of circumstellar material in AB Aur. - Pablo RIVIERE  
11:20 - 11:35 Feeding a Protostar with 10,000 au Scale Streamers - Jaime PINEDA  
11:35 - 11:50 Tracing episodic accretion with NOEMA: FU Orionis-type stars and their millimeter environment - Orsolya FEHER  
11:50 - 12:15 Evolution of Volatile CO from Protostellar Disks to Protoplanetary Disks - Edwin BERGIN (IS)  
12:15 - 13:45 Lunch break  
13:45 - 14:10 Physical Conditions for Galaxy Evolution as Revealed by Detailed (Sub-) Millimeter Spectroscopy of High-Redshift Galaxies - Dominik RIECHERS (IS)  
14:10 - 14:25 Probing the physical conditions of the interstellar medium (ISM) in the quasar host galaxies at z ~ 6 - Jianan LI  
14:25 - 14:40 CH+(1-0) in z~2-4 starburst galaxies: probes of multi-phasic turbulent gas reservoirs - Alba VIDAL GARCIA  
14:40 - 14:55 The Interstellar and Circumgalactic Media at low and high redshift as traced by Atomic Carbon and Carbon Monoxide - Paola ANDREANI  
14:55 - 15:15 The Evolution of Molecular Gas and Star Formation from z=0 to z=2.5: Results from the PHIBSS Large Programs and Forward Look to NOEMA 3D - Linda TACCONI (LP)  
15:15 - 15:40 Tracing cosmic large scale structures with molecular lines - Guilaine LAGACHE (IS)  
15:40 - 16:10 Coffee break  
16:10 - 16:35 Modelling of turbulent ISM and corresponding molecular tracers - Patrick HENNEBELLE (IS)  
16:35 - 16:50 The Expanding Orion Nebula - A combined C+ and CO square-degree map of the Orion A molecular cloud - Cornelia PABST  
16:50 - 17:05 A multi-tracer view of turbulence and triggered star-formation in the Orion B molecular cloud - Jan ORKISZ  
17:05 - 17:25 Astrophysics meets data science in the Orion B Giant Molecular Cloud - Jérôme PETY (LP)  
17:25 - 17:45 Wrap-up - SOC  
  
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