Austria
University of Innsbruck
2015–2017 · Senior Postdoctoral Fellow, Austrian Science Fund (FWF) Lise Meitner Programme; led an independently funded research project.
Full scientific record
Science–education transfer · Founder of MINT-BRUCK
Innsbruck, Austria · mf.nieva@mint-bruck.at
International research experience, competitive project funding and scientific evaluation, connected with primary school practice and teacher education in Tyrol.
Austria
2015–2017 · Senior Postdoctoral Fellow, Austrian Science Fund (FWF) Lise Meitner Programme; led an independently funded research project.
Germany
Garching · 2008–2011 · Postdoctoral research on massive stars, precision spectroscopy and cosmic abundances.
Germany
Dr. Remeis Observatory, Bamberg · 2004–2008: doctoral research and project scientist; 2011–2013: postdoctoral research.
Spain
Tenerife · 2017 · Visiting scientist through the Severo Ochoa programme; quantitative stellar spectroscopy.
Brazil
Rio de Janeiro · 2002–2004 · Research appointment and doctoral research, followed by cotutelle research in Germany.
Argentina
1995–2002 · Teaching assistant in modern and experimental physics and laboratory courses.
Austria
Innsbruck · November 2025–August 2026 · Contract lecturer in mathematics education for primary-school teacher education.
Austria
Innsbruck · September 2024–August 2025 · Enrichment education, learning support and mathematics and science activities in a primary school.
2020 · Appointed by the European Space Agency (ESA) to the stellar-physics panel for Cycle 28. Evaluation of observing-time proposals at the Space Telescope Science Institute, USA.
2017 · Panel member of the Observing Programmes Committee, Period 100, evaluating and ranking proposals for telescope time. Garching, Germany.
Securing competitive resources, developing independent research questions and leading scientific projects.
Research in Austria, Germany and Brazil.
Awarded telescope time for independently proposed research, alongside further programmes as Co-Investigator.
Project leadership · University of Innsbruck, Austria · 2015–2017
Structure and chemistry of the solar neighborhood ↗ · FWF M1868. Independently secured Lise Meitner project with international research collaboration.
PI (Principal Investigator) denotes the lead applicant responsible for the science; Co-I (Co-Investigator) denotes membership of the investigator team. Awarded observing time is a competitively allocated research resource.
| Year | Telescope / instrument | Time awarded | Programme ID |
|---|---|---|---|
| 2017 | ESO VLT / UVESChile | 11.5 hours | 099.C-0637(A) |
| 2013 | ESO 2.2 m / FEROSChile | 4 nights | 091.C-0713(A) |
| 2011 | ESO 2.2 m / FEROS · MPIAChile | 5 nights | 088.B-9003(A) |
| 2009 | ESO VLT / UVESChile | 10 hours | 384.B-0066(A) |
| Year | Telescope / instrument | Time awarded | Programme ID |
|---|---|---|---|
| 2018 | ESO VLT / UVESChile | 10 hours | 101.D-0851(A) |
| 2015 | ESO VLT / X-ShooterChile | 5 hours | 095.C-0446(A) |
| 2015 | ESO VLT / UVESChile | 15 hours | 094.D-0355(A) |
| 2015 | ESO VLT / FORS2Chile | 15 hours | 094.D-0355(B) |
| 2015 | ESO VLT / UVESChile | 7.5 hours | 093.D-0267(B) |
| 2014 | ESO VLT / FORS2Chile | 3 nights | 191.D-0255(C) |
| 2013–2015 | ESO 3.6 m / HARPS · Large ProgrammeChile | 25 nights | 191.D-0255(B)191.D-0255(D)191.D-0255(F)191.D-0255(H)191.D-0255(I)191.D-0255(J) |
| 2013 | Nordic Optical Telescope / FIESSpain | 2 nights | NOT-47-212 |
| 2013 | ESO 2.2 m / FEROSChile | 4 nights | 090.D-0358(A) |
| 2011 | ESO 2.2 m / FEROSChile | 4.5 nights | 088.D-0064(A) |
| 2011 | Hubble Space Telescope / STIS, COSSpace · USA | 12 orbits | 12222 |
| 2011 | ESO VLT / FORS2Chile | 4 nights | 087.D-0049(A) |
| 2009–2011 | ESO VLT / CRIRES · Large ProgrammeChile | 381 hours | 084.D-0912085.D-0161086.D-0066087.D-0195088.D-0109 |
| 2010 | Nordic Optical Telescope / FIESSpain | 4 nights | NOT-41-027 |
| 2010 | ESO VLT / UVESChile | 4.5 hours | 282.D-5065(A) |
| 2009 | ESO VLT / UVESChile | 10 hours | 383.D-0909(A) |
| 2008 | Calar Alto / TWINSpain | 2 nights | H08-3.5-068 |
| 2007 | ESO VLT / CRIRESChile | 1 night | 079.D-0810(A) |
| 2007 | ESO 2.2 m / FEROSChile | 12 hours | 079.B-0856(A) |
Time allocations for large programmes refer to the team’s full programme. Multiple programme identifiers may belong to a single listed entry. Hubble is a space telescope; USA refers to its operating institute.
| Year | Telescope / instrument | Time awarded | Programme ID |
|---|---|---|---|
| 2013 | Calar Alto / CAFESpain | 5 nights | H13-2.2-001 |
| 2012 | Calar Alto / CAFESpain | 5 nights | H12-2.2-030 |
The archived CV does not specify a PI or Co-I role for these two Calar Alto programmes.
Telescopes: ESO = European Southern Observatory; VLT = Very Large Telescope; NOT = Nordic Optical Telescope; HST = Hubble Space Telescope; MPIA = Max Planck Institute for Astronomy.
Instruments: UVES = Ultraviolet and Visual Echelle Spectrograph; FEROS = Fiber-fed Extended Range Optical Spectrograph; FORS2 = FOcal Reducer and low dispersion Spectrograph 2; HARPS = High Accuracy Radial velocity Planet Searcher; FIES = FIbre-fed Echelle Spectrograph; STIS = Space Telescope Imaging Spectrograph; COS = Cosmic Origins Spectrograph; CRIRES = CRyogenic high-resolution InfraRed Echelle Spectrograph; CAFE = Calar Alto Fiber-fed Echelle spectrograph. X-Shooter is a wide-band spectrograph; TWIN is a two-channel spectrograph.
From stars to Earth. Scientific ways of working inform education; questions and observations from practice open new perspectives for research and development.
What this experience brings to partners
Quantitative modelling, careful handling of uncertainty, reasoned judgement and peer review provide a rigorous basis for learning tasks, educational projects and their development.
Co-developed a reference standard for the chemical composition of the solar neighbourhood and contributed to precision stellar analysis. Selection updated through September 2026.
Przybilla, N., Aschenbrenner, P., Weßmayer, D., Keiler, S., Nieva, M. F., Butler, K. & Schaffenroth, V. Present-day abundances from OB stars ↗
Morel, T., Blazère, A., Semaan, T. et al. (including M. F. Nieva) (2022). The Gaia-ESO survey: A spectroscopic study of the young open cluster NGC 3293 ↗
Blomme, R., Daflon, S., Gebran, M. et al. (including M. F. Nieva) (2022). The Gaia-ESO Survey: The analysis of the hot-star spectra ↗
Nieva, M.-F. & Przybilla, N. (2012). Present-day cosmic abundances ↗
Nieva, M.-F. & Przybilla, N. (2008). Carbon abundances of early B-type stars in the solar vicinity ↗
Nieva, M.-F. & Przybilla, N. (2006). C II abundances in early-type stars: solution to a notorious non-LTE problem ↗
Invited reviews and seminars, conference contributions and scientific invitations across Europe, North and South America, China and New Zealand.
Seminar
11 November · Department of Astronomy, Stockholm University / AlbaNova. OB stars as laboratories for numerous astrophysical fields.
Scientific presentation.
Invited talk
High accuracy quantitative spectroscopy in the Galaxy
International Astronomical Union (IAU), Symposium 329
Seminar
Chemical composition of cosmic dust in the solar vicinity
Instituto de Astrofísica de Canarias
Contributed conference talk
Chemical composition of cosmic dust in the solar neighbourhood, as derived from massive stars
Multiple Faces of the Interstellar Dust
Invited review
Fundamental parameters and chemical composition of massive stars
Second BRITE-Constellation Science Conference
Research workshop invitation
The chemical evolution of Galaxies
Munich Institute for Astro- and Particle Physics
Invited talk
The chemical composition of our Milky Way derived from massive stars
Universidad Nacional de Salta
Invited talk
OB stars as laboratories for numerous astrophysical fields
Friends of Friends Meeting · Instituto de Astronomía Teórica y Experimental
Invited talk
A new density and chemical abundance map in the solar neighbourhood
University of Innsbruck · Joint Institute Seminar
Invited talk
Spectrum analysis of early B-type stars: stellar parameters and abundances
Massive stars and the Gaia-ESO survey
Invited talk
Present-day helium abundances in the solar vicinity
European Week of Astronomy and Space Sciences
Poster contribution
Fundamental parameters of B-type stars
New windows on massive stars
Invited talk
Effective temperature scale and bolometric corrections for OB stars
Setting a new standard in the analysis of binary stars
Contributed conference talk
Present-day cosmic abundances in the solar neighbourhood and implications
The Milky Way: Stars, Gas, Dust and Magnetic Fields in 3D
Contributed conference talk
Present-day cosmic oxygen abundance in the solar neighbourhood
Mapping oxygen in the Universe
Invited talk
A cosmic abundance standard from massive stars in the solar neighbourhood
Science Day of the Excellence Cluster · Research Area G
Contributed conference talk
Present-day cosmic abundances from B-type stars
Quantitative Stellar Spectroscopy as a Key Tool of Astrophysical Research
Contributed conference talk
Fundamental parameters of normal B-stars in the solar neighbourhood
IAU Symposium · Active OB Stars
Invited seminar
Max Planck Institute for Astronomy
Invited talk
Stellar parameters and chemical abundances at high precision in massive stars
The Chemical Enrichment of the Milky Way
Invited talk
A present-day cosmic abundance standard
Heraeus workshop · Nucleosynthesis: making the Elements in the Universe
Invited seminar
Geneva Observatory
Contributed conference talk
High-precision determinations of stellar parameters and chemical abundances in early B-type stars
California Institute of Technology · Hot and Cool: Bridging Gaps in Massive Star Evolution
Invited seminar
Max Planck Institute for Astrophysics
Poster contribution
High-resolution near-IR spectroscopy of massive stars
Lowell Observatory · Hot massive stars: a lifetime of influence
Contributed conference talk
Near-IR spectroscopy of OB stars with CRIRES: pilot study for E-ELT science
Joint European and National Astronomy Meeting · Science with the E-ELT
Contributed conference talk
Accurate quantitative spectroscopy of OB stars: C and N abundances near the Main Sequence
Massive Stars: Fundamental Parameters and Circumstellar Interactions
Contributed conference talk
Accurate quantitative spectroscopy of OB stars: the H, He and C spectrum
European Southern Observatory (ESO) conference · Precision Spectroscopy in Astrophysics
Invited seminar
European Southern Observatory (ESO) · Lunch talk
Invited seminar
Dr. Remeis Observatory · University of Erlangen–Nuremberg
Poster contribution
Chemical abundances of LMC fast-rotating B-stars
Optical and Infrared Astronomical Instrumentation for Modern Telescopes
Poster contribution
Determinación de parámetros físicos y estado de evolución de estrellas B, A y F
Reunión Latinoamericana de Astronomía
National Meeting of the Argentine Astronomical Association · September 2016.
Conference “Putting A stars into context” · June 2013.
National Meeting of the Argentine Astronomical Association · September 2013.
International Astronomical Union (IAU) General Assembly. Invited review: Atmospheric modelling of massive stars in the IR domain.
Additional contributed talk in Special Session 12: Modern views of the interstellar medium.
Both contributions were presented by Norbert Przybilla on behalf of María Fernanda Nieva, who was unable to attend in person.