| Isotopic evidence for primordial molecular cloud material in metal-rich carbonaceous chondrites EMME Van Kooten, D Wielandt, M Schiller, K Nagashima, A Thomen, ... Proceedings of the National Academy of Sciences 113 (8), 2011-2016, 2016 | 162 | 2016 |
| Precise measurement of chromium isotopes by MC-ICPMS M Schiller, E Van Kooten, JC Holst, MB Olsen, M Bizzarro Journal of Analytical Atomic Spectrometry 29 (8), 1406-1416, 2014 | 82 | 2014 |
| Magnesium and 54Cr isotope compositions of carbonaceous chondrite chondrules–Insights into early disk processes MB Olsen, D Wielandt, M Schiller, EMME Van Kooten, M Bizzarro Geochimica et cosmochimica acta 191, 118-138, 2016 | 79 | 2016 |
| 182Hf–182W age dating of a 26Al-poor inclusion and implications for the origin of short-lived radioisotopes in the early Solar System JC Holst, MB Olsen, C Paton, K Nagashima, M Schiller, D Wielandt, ... Proceedings of the National Academy of Sciences 110 (22), 8819-8823, 2013 | 62 | 2013 |
| Combined U-corrected Pb-Pb dating and 26Al-26Mg systematics of individual chondrules–Evidence for a reduced initial abundance of 26Al amongst inner Solar System chondrules J Bollard, N Kawasaki, N Sakamoto, M Olsen, S Itoh, K Larsen, ... Geochimica et Cosmochimica Acta 260, 62-83, 2019 | 49 | 2019 |
| MAGNESIUM ISOTOPE EVIDENCE FOR SINGLE STAGE FORMATION OF CB CHONDRULES BY COLLIDING PLANETESIMALS MB Olsen, M Schiller, M Krot, Alexander N. & Bizzarro Astrophysical Journal Letters, L1, 2013 | 31 | 2013 |
| Evidence for a reduced initial abundance of 26Al in chondrule forming regions and implications for the accretion timescales of protoplanets M Bizzarro, M Olsen, S Itoh, N Kawasaki, M Schiller, L Bonal, H Yurimoto 77th Annual Meeting of the Meteoritical Society 77 (1800), 5125, 2014 | 5 | 2014 |
| Whole‐rock 26Al‐26Mg systematics of amoeboid olivine aggregates from the oxidized CV3 carbonaceous chondrite Allende MB Olsen, AN Krot, K Larsen, C Paton, D Wielandt, M Schiller, M Bizzarro Meteoritics & Planetary Science 46 (11), 1688-1702, 2011 | 4 | 2011 |
| TOWARDS A (HF)-H-182-W-182 CHRONOLOGY OF FUN CAIS JC Holst, MBS Olsen, D Wielandt, C Paton, M Bizzarro Annual Meeting of the Meteoritical-Society: Meteoritics & Planetary Science, 2012 | 1 | 2012 |
| Midtvejsevaluering: Science i Fritiden MBS Olsen Rambøll, 2022 | | 2022 |
| EVIDENCE FOR A REDUCED INITIAL ABUNDANCE OF Al-26 IN CHONDRULE FORMING REGIONS AND IMPLICATIONS FOR THE ACCRETION TIMESCALES OF PROTOPLANETS M Bizzarro, MBS Olsen, S Itoh, N Kawasaki, M Schiller, L Bonal, ... | | 2014 |
| Brorfelde Observatorium åbner som oplevelsescenter JKL Bouchet, MB Olsen Kvant 4, 14-17, 2014 | | 2014 |
| Study of Meteoritic Inclusion MBS Olsen | | 2014 |
| Towards a 182Hf-182W Chronology of FUN CAIs JC Holst, MB Olsen, D Wielandt, C Paton, M Bizzarro Meteoritics and Planetary Science Supplement 75, 5223, 2012 | | 2012 |
| Preserved Nucleosynthetic Heterogeneity in Cv and CR Chondrules: Implications for Chondrule-Forming Mechanisms MB Olsen, D Wielandt, M Schiller, C Paton, M Bizzarro Meteoritics and Planetary Science Supplement 75, 5195, 2012 | | 2012 |
| Mineralogy, Petrography and Pb-Pb Isotope Systematics of a Type II Allende Chondrule MB Olsen, AN Krot, JN Connelly, K Larsen, CB Paton, D Wielandt, ... Workshop on Formation of the First Solids in the Solar System 1639, 9060, 2011 | | 2011 |
| 26Al-26Mg Systematics of Allende AOAs MB Olsen, K Larsen, C Paton, D Wielandt, AN Krot, M Bizzarro Meteoritics and Planetary Science Supplement 73, 5220, 2010 | | 2010 |
| Al-26-(26) Mg SYSTEMATICS OF ALLENDE AOAs MB Olsen, K Larsen, C Paton, D Wielandt, AN Krot, M Bizzarro METEORITICS & PLANETARY SCIENCE 45, A156-A156, 2010 | | 2010 |
| 73rd Annual Meteoritical Society Meeting (2010) 5220. pdf MB Olsen, K Larsen, C Paton, D Wielandt, AN Krot | | |
| Heterogeneous distribution of 26Al in the solar protoplanetary disk–insights from chondritic components and angrite meteorites. M Bizzarro, M Olsen, M Schiller, JN Connelly, S Itoh, N Kawasaki, ... | | |
Martin SchillerUniversity of CopenhagenAdresse e-mail validée de snm.ku.dk
