Dr Theresa Falkendal

PostDoc
Falkendal

Contact

Potsdam Institute for Climate Impact Research (PIK)
T +49 (0)331 288 2482
theresa.falkendal[at]pik-potsdam.de
P.O. Box 60 12 03
14412 Potsdam

ORCID

Peer reviewed journals

T. Falkendal, C. Otto, J. Schewe, J. Jägermeyr, M. Konar, M. Kummu, B. Watkins and M. J. Puma. Safeguard global supply chains to protect food security during the COVID-19 pandemic. Nature Food, 2020, under review

T. Falkendal, M. D. Lehnert, J. Vernet, C. De Breuck and , W. Wang.  ALMA and MUSE observations reveal a quiescent multi-phase circumgalactic medium around the z=3.6 radio galaxy 4C 19.71. Astronomy & Astrophysics, 2020, accepted

T. Falkendal, C. De Breuck, M. D. Lehnert, G. Drouart, J. Vernet, B. Emonts, M. Lee, N. P. H. Nesvadba, N. Seymore, M. Béthermin, S. Kolwa, B. Gullberg and D.  Wylezalek. Massive galaxies on the road to quenching: ALMA observations of powerful high redshift radio galaxies. Astronomy & Astrophysics, 2019 DOI: 10.1051/0004-6361/201732485

S. Kolwa, J. Vernet, C. De Breuck, M. Villar-Martín, A. Humphrey, F. Arrigoni-Battaia, B. Gullberg, T. Falkendal, G. Drouart, M. D. Lehnert, D. Wylezalek and A. Man. MUSE unravels the ionisation and origin of metal-enriched absorbers in the gas halo of a z = 2.92 radio galaxy. Astronomy & Astrophysics, 2019 DOI: 10.1051/0004-6361/201935437

 A. W. S Man, M. D. Lehnert, J. Vernet, C. De Breuck, and T. Falkendal. Quenching by gas compression and consumption: A case study of a massive radio galaxy at z = 2.57. Astronomy & Astrophysics, 2019 DOI: 10.1051/0004-6361/201834542

 D. Drouart and T. Falkendal. MR-MOOSE: an advanced SED-fitting tool for heterogeneous multi-wavelength data sets. Monthly Notices of the Royal Astronomical Society, 2018 DOI: 10.1093/mnras/sty831

F. Lelli, C. De Breuck, T. Falkendal, F. Fraternali, A. W. S. Man, N. P. H. Nesvadba and  M. D Lehnert. Neutral versus ionized gas kinematics at z~2.6: the AGN-host starburst galaxy PKS 0529-549. Monthly Notices of the Royal Astronomical Society, 2018  DOI: 10.1093/mnras/sty1795

J. Vernet, M. D. Lehnert, C. De Breuck, M. Villar-Martín, D. Wylezalek, T. Falkendal, G. Drouart, S. Kolwa, A. Humphrey, B. P. Venemans and F. Boulanger. Are we seeing accretion flows in a 250 kpc-sized Lyα halo at z=3? Astronomy & Astrophysic, 2017 DOI: 10.1051/0004-6361/201730865