Explore the words cloud of the PhysSF project. It provides you a very rough idea of what is the project "PhysSF" about.
The following table provides information about the project.
Coordinator |
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
Organization address contact info |
Coordinator Country | Germany [DE] |
Project website | https://www.phangs.org |
Total cost | 2˙495˙000 € |
EC max contribution | 2˙495˙000 € (100%) |
Programme |
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC)) |
Code Call | ERC-2015-AdG |
Funding Scheme | ERC-ADG |
Starting year | 2016 |
Duration (year-month-day) | from 2016-10-01 to 2021-09-30 |
Take a look of project's partnership.
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1 | MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV | DE (Munich) | coordinator | 2˙495˙000.00 |
In the past decade we learned when and where stellar mass was built up in galaxies through cosmic time, now we must understand the physical causes in order to answer `How do galaxies form and evolve?’. This ERC project is designed to greatly advance our understanding of the physics of the star formation (SF) process and its regulation in typical star forming galaxies. The ERC project consists of 2 complementary parts: (A) an unparalleled characterization of the SF process in nearby galaxies through full exploitation of the revolutionary capabilities of the latest millimeter interferometers (ALMA) and optical integral field units (MUSE). This study will constrain the key physical parameters for the SF process on only 50pc scales - the scale of large HII regions and their predecessors, giant molecular clouds. At this crucial scale, the MUSE-ALMA-HST Survey will provide a characterization of the SF history, stellar/gaseous surface densities, metallicities of stars and gas, the stellar radiation field, extinction, and stellar/gas kinematics, and thus uncover the physical conditions that control and regulate the SF process. Part (B) will place the results of part (A) in a cosmological context, by characterizing key galaxy quantities (e.g., gas mass fraction, specific SF rates, gas depletion times) in fully representative galaxy samples after (z<3) and before (z>3) the peak epoch of cosmic star formation density. In addition to providing the critically needed constraints on the conditions that govern the SF process, this ERC project will provide the observational benchmark for state-of-the art galaxy simulations and models. The PI is internationally recognized as a leader in SF studies in nearby and distant galaxies, and has successfully led large international collaborations that strongly shaped our current understanding of the SF process. Through her track record and access to the required data, the PI is uniquely positioned to successful lead this ambitious program.
year | authors and title | journal | last update |
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2017 |
O. Miettinen, I. Delvecchio, V. SmolÄić, M. Aravena, D. Brisbin, A. Karim, B. Magnelli, M. Novak, E. Schinnerer, M. Albrecht, H. Aussel, F. Bertoldi, P. L. Capak, C. M. Casey, C. C. Hayward, O. Ilbert, H. T. Intema, C. Jiang, O. Le Fèvre, H. J. McCracken, A. M. Muñoz Arancibia, F. Navarrete, N. D. Padilla, D. A. Riechers, M. Salvato, K. S. Scott, K. Sheth, L. A. M. Tasca An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling published pages: A17, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201730762 |
Astronomy & Astrophysics 606 | 2019-06-13 |
2017 |
O. Miettinen, M. Novak, V. SmolÄić, I. Delvecchio, M. Aravena, D. Brisbin, A. Karim, E. J. Murphy, E. Schinnerer, M. Albrecht, H. Aussel, F. Bertoldi, P. L. Capak, C. M. Casey, F. Civano, C. C. Hayward, N. Herrera Ruiz, O. Ilbert, C. Jiang, C. Laigle, O. Le Fèvre, B. Magnelli, S. Marchesi, H. J. McCracken, E. Middelberg, A. M. Muñoz Arancibia, F. Navarrete, N. D. Padilla, D. A. Riechers, M. Salvato, K. S. Scott, K. Sheth, L. A. M. Tasca, M. Bondi, G. Zamorani An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array published pages: A54, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201730443 |
Astronomy & Astrophysics 602 | 2019-06-13 |
2018 |
Sharon E. Meidt, Adam K. Leroy, Erik Rosolowsky, J. M. Diederik Kruijssen, Eva Schinnerer, Andreas Schruba, Jerome Pety, Guillermo Blanc, Frank Bigiel, Melanie Chevance, Annie Hughes, Miguel Querejeta, Antonio Usero A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces. I. Cloud-scale Gas Motions published pages: 100, ISSN: 0004-637X, DOI: 10.3847/1538-4357/aaa290 |
The Astrophysical Journal 854/2 | 2019-06-13 |
2018 |
D Cormier, F Bigiel, M J Jiménez-Donaire, A K Leroy, M Gallagher, A Usero, K Sandstrom, A Bolatto, A Hughes, C Kramer, M R Krumholz, D S Meier, E J Murphy, J Pety, E Rosolowsky, E Schinnerer, A Schruba, K Sliwa, F Walter Full-disc 13CO(1–0) mapping across nearby galaxies of the EMPIRE survey and the CO-to-H2 conversion factor published pages: 3909-3933, ISSN: 0035-8711, DOI: 10.1093/mnras/sty059 |
Monthly Notices of the Royal Astronomical Society 475/3 | 2019-06-13 |
2017 |
I-Ting Ho, Mark Seibert, Sharon E. Meidt, Rolf-Peter Kudritzki, Chiaki Kobayashi, Brent A. Groves, Lisa J. Kewley, Barry F. Madore, Jeffrey A. Rich, Eva Schinnerer, Joshua D’Agostino, Henry Poetrodjojo The Chemical Evolution Carousel of Spiral Galaxies: Azimuthal Variations of Oxygen Abundance in NGC1365 published pages: 39, ISSN: 0004-637X, DOI: 10.3847/1538-4357/aa8460 |
The Astrophysical Journal 846/1 | 2019-06-13 |
2017 |
Adam K. Leroy, Eva Schinnerer, Annie Hughes, J. M. Diederik Kruijssen, Sharon Meidt, Andreas Schruba, Jiayi Sun, Frank Bigiel, Gonzalo Aniano, Guillermo A. Blanc, Alberto Bolatto, Mélanie Chevance, Dario Colombo, Molly Gallagher, Santiago Garcia-Burillo, Carsten Kramer, Miguel Querejeta, Jerome Pety, Todd A. Thompson, Antonio Usero Cloud-scale ISM Structure and Star Formation in M51 published pages: 71, ISSN: 0004-637X, DOI: 10.3847/1538-4357/aa7fef |
The Astrophysical Journal 846/1 | 2019-06-13 |
2017 |
E. Daddi, S. Jin, V. Strazzullo, M. T. Sargent, T. Wang, C. Ferrari, E. Schinnerer, V. SmolÄić, A. Calabró, R. Coogan, J. Delhaize, I. Delvecchio, D. Elbaz, R. Gobat, Q. Gu, D. Liu, M. Novak, F. Valentino Radio Selection of the Most Distant Galaxy Clusters published pages: L31, ISSN: 0004-6361, DOI: 10.3847/2041-8213/aa8808 |
The Astrophysical Journal 846/2 | 2019-06-13 |
2017 |
Y. Fudamoto, P. A. Oesch, E. Schinnerer, B. Groves, A. Karim, B. Magnelli, M. T. Sargent, P. Cassata, P. Lang, D. Liu, O. Le Fèvre, S. Leslie, V. SmolÄić, L. Tasca The dust attenuation of star-forming galaxies at z ∼ 3 and beyond: New insights from ALMA observations published pages: 483-490, ISSN: 0035-8711, DOI: 10.1093/mnras/stx1948 |
Monthly Notices of the Royal Astronomical Society 472/1 | 2019-06-13 |
2018 |
K. Kreckel, C. Faesi, J. M. D. Kruijssen, A. Schruba, B. Groves, A. K. Leroy, F. Bigiel, G. A. Blanc, M. Chevance, C. Herrera, A. Hughes, R. McElroy, J. Pety, M. Querejeta, E. Rosolowsky, E. Schinnerer, J. Sun, A. Usero, D. Utomo A 50 pc Scale View of Star Formation Efficiency across NGC 628 published pages: L21, ISSN: 0004-637X, DOI: 10.3847/2041-8213/aad77d |
The Astrophysical Journal 863/2 | 2019-06-07 |
2018 |
S. K. Leslie, M. T. Sargent, E. Schinnerer, B. Groves, A. van der Wel, G. Zamorani, Y. Fudamoto, P. Lang, V. SmolÄić Probing star formation and ISM properties using galaxy disk inclination published pages: A7, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201732255 |
Astronomy & Astrophysics 615 | 2019-06-07 |
2018 |
Molly J. Gallagher, Adam K. Leroy, Frank Bigiel, Diane Cormier, MarÃa J. Jiménez-Donaire, Annie Hughes, Jérôme Pety, Eva Schinnerer, Jiayi Sun, Antonio Usero, Dyas Utomo, Alberto Bolatto, Mélanie Chevance, Chris Faesi, Simon C. O. Glover, Amanda A. Kepley, J. M. Diederik Kruijssen, Mark R. Krumholz, Sharon E. Meidt, David S. Meier, Eric Murphy, Miguel Querejeta, Erik Rosolowsky, Toshiki Saito, Andreas Schruba Do Spectroscopic Dense Gas Fractions Track Molecular Cloud Surface Densities? published pages: L38, ISSN: 0004-637X, DOI: 10.3847/2041-8213/aaf16a |
The Astrophysical Journal 868/2 | 2019-06-07 |
2019 |
M. Querejeta, E. Schinnerer, A. Schruba, E. Murphy, S. Meidt, A. Usero, A. K. Leroy, J. Pety, F. Bigiel, M. Chevance, C. M. Faesi, M. Gallagher, S. GarcÃa-Burillo, S. C. O. Glover, A. P. S. Hygate, M. J. Jiménez-Donaire, J. M. D. Kruijssen, E. Momjian, E. Rosolowsky, D. Utomo Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100 pc scales in M 51 published pages: A19, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834915 |
Astronomy & Astrophysics 625 | 2019-06-06 |
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