Tamara Rom

ORCID: 0000-0002-9076-2425
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About
Contact & Profiles
Research Areas
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Astrophysics and Star Formation Studies
  • Impact of Light on Environment and Health
  • Human Mobility and Location-Based Analysis
  • Air Quality Monitoring and Forecasting
  • Remote Sensing and LiDAR Applications
  • Cosmology and Gravitation Theories
  • Astrophysical Phenomena and Observations
  • Pulsars and Gravitational Waves Research
  • Astronomical Observations and Instrumentation
  • Experimental and Theoretical Physics Studies
  • Dark Matter and Cosmic Phenomena

University of Split
2023-2024

Institut de Planétologie et d'Astrophysique de Grenoble
2024

Centre National de la Recherche Scientifique
2023

Université Grenoble Alpes
2023

The relationship between satellite based measurements of city radiance at night and the numbers types physical lights installed on ground is not well understood. Here we present “Nachtlichter app”, which was developed to enable citizen scientists classify count light sources along street segments over large spatial scales. project app were co-designed: played key roles in development, testing, recruitment, as analysis data. In addition describing itself data format, provide a general...

10.26607/ijsl.v25i1.133 article EN cc-by-nc-nd International Journal of Sustainable Lighting 2023-12-03

Context. With a mass exceeding several 10^4 solar masses and rich dense population of massive stars, supermassive young star clusters represent the most star-forming environment that is dominated by feedback from stars gravitational interactions among stars. Aims. In this paper we present "Extended Westerlund 1 2 Open Clusters Survey" (EWOCS) project, which aims to investigate influence starburst on formation planets, evolution both low high The primary targets project are 2, closest Sun....

10.1051/0004-6361/202347778 article EN cc-by Astronomy and Astrophysics 2023-12-11

The typically large distances, extinction, and crowding of Galactic supermassive star clusters (stellar more massive than 10$^4\,$M$_ have so far hampered the identification their very low mass members, required to extend our understanding planet formation, early stellar evolution, extremely energetic star-forming environment typical starbursts. This situation has now evolved thanks James Webb Space Telescope (JWST), its unmatched resolution sensitivity in infrared. In this paper, third...

10.1051/0004-6361/202452150 article EN cc-by Astronomy and Astrophysics 2024-11-15

The typically large distances, extinction, and crowding of Galactic supermassive star clusters have so far hampered the identification their very low mass members, required to extend our understanding planet formation, early stellar evolution, starburst. This situation has now evolved thanks James Webb Space Telescope (JWST), its unmatched resolution sensitivity in infrared. In this paper, third series Extended Westerlund 1 2 Open Clusters Survey (EWOCS), we present JWST/NIRCam JWST/MIRI...

10.48550/arxiv.2411.13051 preprint EN arXiv (Cornell University) 2024-11-20

<title>Abstract</title> The image of Earth at Night from space has become iconic, but we are still in the dark when it comes to question what extent different light source types contribute city emissions. Our team citizen scientists used Nachtlichter app count and classify 234,044 sources over a total area 22 km2 during 2021. We find that space-based radiance observation 1 nW/cm2sr 500-900 nm range corresponds 219 lights/km2 on ground midnight. This suggests 78.0±1.6 million individual...

10.21203/rs.3.rs-4743740/v1 preprint EN cc-by Research Square (Research Square) 2024-08-07

Aim: To formulate a model capable of distinguishing astro-physical from primordial gravitational-wave signals. Methods: We used biased tracer formalism valid on large cosmological scales to introduce modeling basics and con-nected black holes as sources gravitational wave signal with dark matter. Results: LTC By deriving the using online tool Code for Anisotropies in Microwave Background (CAMB), we produced matter power spectrum it construct spectra lin-ear tracer. The were generated...

10.48188/so.4.2 article EN cc-by St open 2023-04-21
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