Dust-depletion sequences in damped Lyman-α absorbers-A unified picture from low-metallicity systems to the Galaxy A De Cia, C Ledoux, L Mattsson, P Petitjean, R Srianand, I Gavignaud, ... Astronomy & Astrophysics 596, A97, 2016 | 190 | 2016 |
‘Counterpart’ method for abundance determinations in H ii regions LS Pilyugin, EK Grebel, L Mattsson Monthly Notices of the Royal Astronomical Society 424 (3), 2316-2329, 2012 | 147 | 2012 |
Dust driven mass loss from carbon stars as a function of stellar parameters-I. A grid of solar-metallicity wind models L Mattsson, R Wahlin, S Höfner Astronomy & Astrophysics 509, A14, 2010 | 131 | 2010 |
Intense mass loss from C-rich AGB stars at low metallicity? L Mattsson, R Wahlin, S Höfner, K Eriksson Astronomy & Astrophysics 484 (1), L5-L8, 2008 | 104 | 2008 |
Abundance determination in H ii regions from spectra without the [O ii]λ3727+λ3729 line LS Pilyugin, L Mattsson Monthly Notices of the Royal Astronomical Society 412 (2), 1145-1150, 2011 | 77 | 2011 |
Polynomial probability distribution estimation using the method of moments J Munkhammar, L Mattsson, J Rydén PloS one 12 (4), e0174573, 2017 | 66 | 2017 |
Abundance determination from global emission-line SDSS spectra: exploring objects with high N/O ratios LS Pilyugin, JM Vílchez, L Mattsson, TX Thuan Monthly Notices of the Royal Astronomical Society 421 (2), 1624-1634, 2012 | 66 | 2012 |
Mass loss evolution and the formation of detached shells around TP-AGB stars L Mattsson, S Höfner, F Herwig Astronomy & Astrophysics 470 (1), 339-352, 2007 | 66 | 2007 |
On the dust abundance gradients in late-type galaxies–II. Analytical models as evidence for massive interstellar dust growth in SINGS galaxies L Mattsson, AC Andersen Monthly Notices of the Royal Astronomical Society 423 (1), 38-48, 2012 | 64 | 2012 |
The origin of carbon: Low-mass stars and an evolving, initially top-heavy IMF? L Mattsson Astronomy & Astrophysics 515, A68, 2010 | 62 | 2010 |
On the (in) variance of the dust-to-metals ratio in galaxies L Mattsson, A De Cia, AC Andersen, T Zafar Monthly Notices of the Royal Astronomical Society 440 (2), 1562-1570, 2014 | 60 | 2014 |
Dust-driven mass loss from carbon stars as a function of stellar parameters-ii. effects of grain size on wind properties L Mattsson, S Höfner Astronomy & Astrophysics 533, A42, 2011 | 57 | 2011 |
Dust in the early Universe: evidence for non-stellar dust production or observational errors? L Mattsson Monthly Notices of the Royal Astronomical Society 414 (1), 781-791, 2011 | 56 | 2011 |
On the electron temperatures in high-metallicity H ii regions LS Pilyugin, L Mattsson, JM Vílchez, B Cedrés Monthly Notices of the Royal Astronomical Society 398 (1), 485-496, 2009 | 49 | 2009 |
On the dust abundance gradients in late-type galaxies–I. Effects of destruction and growth of dust in the interstellar medium L Mattsson, AC Andersen, JD Munkhammar Monthly Notices of the Royal Astronomical Society 423 (1), 26-37, 2012 | 46 | 2012 |
The metallicity–redshift relations for emission-line SDSS galaxies: examination of the dependence on the star formation rate LS Pilyugin, MA Lara-López, EK Grebel, C Kehrig, IA Zinchenko, ... Monthly Notices of the Royal Astronomical Society 432 (2), 1217-1230, 2013 | 39 | 2013 |
The vanishing and appearing sources during a century of observations project. I. USNO objects missing in modern sky surveys and follow-up observations of a “Missing Star” B Villarroel, J Soodla, S Comerón, L Mattsson, K Pelckmans, ... The Astronomical Journal 159 (1), 8, 2019 | 37 | 2019 |
The Herschel exploitation of local galaxy Andromeda (HELGA) – V. Strengthening the case for substantial interstellar grain growth L Mattsson, HL Gomez, AC Andersen, MWL Smith, I De Looze, M Baes, ... Monthly Notices of the Royal Astronomical Society 444 (1), 797-807, 2014 | 36 | 2014 |
On the influence of the environment on galactic chemical abundances LS Pilyugin, EK Grebel, IA Zinchenko, YA Nefedyev, L Mattsson Monthly Notices of the Royal Astronomical Society, stw2831, 2016 | 30 | 2016 |
Modelling dust processing and the evolution of grain sizes in the ISM using the method of moments L Mattsson Planetary and Space Science 133, 107-123, 2016 | 29 | 2016 |