- March 3, 10:30 to 12:00 (CET)   Programme 10:30 Welcome, Introduction 10:40 Current shortcomings in stellar modelling in the PLATO context (Santi Cassisi) 11:10 Reference stars for 4MOST S4 survey and PLATO SAPP pipeline (Maria Bergemann) 11:40 Discussion   Talk Slides Slides for talk: 'Current shortcomings in stellar modelling in the PLATO context' by Santi Cassisi (pdf) Slides for talk: 'Refer

https://www.astro.lu.se/lundreferencestars/programme/session-1 - 2025-07-11

- March 17, 14:00 to 15:30 (CET)   Programme 14:00 Gaia FGK Benchmark stars v3 and beyond (Paula Jofre) 14:20 Transiting exoplanets and eclipsing binaries as stellar density benchmarks (Pierre Maxted) 14:40 Fine-tuning the stellar parameters of evolved stars with Gaia (Shreeya Shetye) 14:48 Discussion   Talk Slides Slides for talk: 'Gaia FGK Benchmark stars v3 and beyond' by Paula Jofre (pdf) Slid

https://www.astro.lu.se/lundreferencestars/programme/session-2 - 2025-07-11

The workshop will be held virtually from Lund Observatory. Zoom link: https://lu-se.zoom.us/s/63428486301 Slack workspace: https://join.slack.com/t/referencestar-iuh1027/shared_invite/zt-lysz0ygk-Te8SdAh2MSSmw0OR7usGMQ If you are registered, you have received the password for this Zoom meeting by email. In case of any troubles, please contact Diane Feuillet or Gregor Traven. You can also join the

https://www.astro.lu.se/lundreferencestars/venue - 2025-07-11

The following people have registered to attend the workshop: Vardan Adibekyan Louis Amard Anish Amarsi Martina Baratella Chiara Battistini Thomas Bensby Spencer Bialek Thibault Boulet Angela Bragaglia Tobias Buck Sven Buder Ricardo Carrera Eugenio Carretta Laia Casamiquela Santi Cassisi William Chantereau Corinne Charbonnel Ross Church Ioana Ciuca Jake Clark Danielle de Brito Silva Klemen Čotar Or

https://www.astro.lu.se/lundreferencestars/participants - 2025-07-11

We are committed to creating a virtual work environment that is safe, professional and of mutualtrust where diversity and inclusion are valued, and where everyone is entitled to be treated withcourtesy and respect. We commit to making the workshop and all associated activities productiveand enjoyable for everyone. We will not tolerate harassment of participants in any form. Please follow these gui

https://www.astro.lu.se/lundreferencestars/code-conduct - 2025-07-11

- MARCH 31, 09:00 TO 10:30 (CEST)   Programme 9:00 Reference stars and values for and from GALAH (Sven Buder) 9:20 Words of Caution on the fitting of metal-poor benchmark stars and globular clusters with stellar tracks and isochrones (Meridith Joyce) 9:40 The chemical composition of very young open clusters (Martina Baratella) 9:48 Discussion   Talk Slides Slides for talk: 'Reference stars and val

https://www.astro.lu.se/lundreferencestars/programme/session-3 - 2025-07-11

The "For All" meeting series was aimed at professional astronomers who wanted to broaden their expertise. The meetings were organized and held at Lund Observatory in early February each year from 2007 to 2020, but were discontinued when Covid hit. Year Meeting theme 2021 - - canceled - - 2020 Compact Objects for All 2019 ELTs for All 2018 Dynamic Universe for All 2017 Gaseous Universe for All 2016

https://www.astro.lu.se/LundObservatory/all-meeting-series - 2025-07-11

- APRIL 14, 15:00 TO 16:30 (CEST)   Programme 15:00 Bridging the Gap between Theory and Data by Leveraging Large Data sets (Yuan-Sen Ting) 15:20 Reference stars and analysis challenges for the metal-poor Galaxy (Kim Venn) 15:40 Building a reference sample from differential spectroscopy (Laia Casamiquela) 16:00 Discussion   Talk Slides Slides for talk: 'Bridging the Gap between Theory and Data by L

https://www.astro.lu.se/lundreferencestars/programme/session-4 - 2025-07-11

High-precision observational astrophysics: solar and stellar spectroscopy, stellar surface structure, radial velocities and wavelength shifts, methods in searches for exoplanets, intensity interferometry, quantum optics, and other. Highest-precision stellar spectroscopy Spectroscopy reveals the structure of stellar surfaces and enables to determine their physical properties.  ‘Ab-initio’ hydrodyna

https://www.astro.lu.se/~dainis/research - 2025-07-11

sdgaeaerae

https://www.astro.lu.se/~dainis/popul%C3%A4rvetenskap - 2025-07-11

​ ​ Var i rymden finns drägliga förhållanden för liv? Nordenmarkföreläsningen vid svenska Astronomdagarna i Göteborg 2022                                                                    https://youtu.be/jdtuCTSjLg0 Att se ytan på andra stjärnor Artikel från tidskriften "Populär Astronomi" Artikeln "Skåda stjärnor med kilometerstora teleskop" Mycket av astronomins framsteg möjliggörs tack vare a

https://www.astro.lu.se/~dainis/popular - 2025-07-11

  Telescopes in the Atacama desert, Chile The Atacama desert of Chile is home to several of the world's greatest telescopes. In this aerial view, the low evening Sun accentuates the mountainous topography. The nearby Cerro Paranal hosts VLT, the Very Large Telescope of ESO, the European Southern Observatory.  In the distance to the left, ELT, the Extremely Large Telescope is being erected on Cerro

https://www.astro.lu.se/~dainis/images - 2025-07-11

from the Lund University Planetarium Show description: Show length: ca 20-45 minutes Available languages: English, Swedish The Lund University Planetarium produced a flat screen version of Distant Universe for Culture Night 2020. This is a live show that requires narration from an experienced astronomer. Only the background videos are provided here and then it is up to you to set it up and provide

https://www.astro.lu.se/Outreach/Planetarium/Distant-Universe - 2025-07-11

The LU and the ROG production teams are willing to share clips and resources with the community.  We are always interested in knowing how people are using our resources, so if you find any of this useful then feel free to reach out and let us know. Flying through the International Space Station Produced by:  Lund Universtiy Planetarium Fulldome video for download In this five minute clip we start

https://www.astro.lu.se/Outreach/Planetarium/Resources - 2025-07-11

- APRIL 28, 9:00 TO 10:30 (CEST)   Programme 9:00 Reference stars for large spectroscopic surveys - the case of LAMOST (Maosheng Xiang) 9:20 Selection of oscillating red giants in multiple-stars systems (Patrick Gaulme) 9:40 Utilising Galactic Archaeology for Exoplanetary Science (Jake Clark) 9:48 Discussion   Talk Slides Slides for talk: 'Reference stars for large spectroscopic surveys - the case

https://www.astro.lu.se/lundreferencestars/programme/session-5 - 2025-07-11

Projects:   The origin of the Nuclear Star Cluster The purpose of the research is to systematically determine and characterize the processes involved in the build up of the Nuclear Star Cluster of the Milky Way and the surrounding central structures, and to investigate the consequences and implications for our understanding of the formation engines of galaxies in general. By studying the present d

https://www.astro.lu.se/~ryde/GCE - 2025-07-11

  Projects:   Water vapor in the atmospheres of Red Giants I have made major contributions to the interpretation of high-resolution, mid-infrared spectra of stars, especially those of red supergiants. For instance, I discovered unexpected water vapour in the atmospheres of warm giant stars. These observations are very useful to test models of the outer atmospheric structures. We still do not know

https://www.astro.lu.se/~ryde/RG - 2025-07-11

Projects:   Near-IR Atomic and Molecular Spectroscopy in the Laboratory With the new Fourier Transform Spectrometer installed at Lund Observatory, we are involved in measuring wavelengths and line strengths of transitions in astrophysically interesting elements, such as Sr, Y, and Ba.   IR spectroscopy at high spectral resolution for the E-ELT I am enaged by ESO to investigate the scientific case

https://www.astro.lu.se/~ryde/IR - 2025-07-11

- Information coming soon Back Red Giants Galactic Chemical Evolution Infrared Spectroscopy

https://www.astro.lu.se/~ryde/Teaching - 2025-07-11

The main aim of my research is to unravel the origin and evolution of large spiral galaxies like our own Milky Way. This is best done by by probing and mapping in detail the age, chemical abundance, and kinematical properties of its main structural components. To do this I have utilised different tracers: dwarf stars in the solar neighbourhood, red giant stars in the inner and outer regions of the

https://www.astro.lu.se/~tbensby/research - 2025-07-11