A5091428206- Astronomy and Astrophysical Research
- Adaptive optics and wavefront sensing
- Astronomical Observations and Instrumentation
- Astro and Planetary Science
- Gamma-ray bursts and supernovae
- Astrophysics and Star Formation Studies
- Radiation Detection and Scintillator Technologies
- Business, Innovation, and Economy
- Spacecraft Design and Technology
- Stellar, planetary, and galactic studies
Universidad Nacional Autónoma de México
2020-2024
We report the discovery and characterisation of a super-Earth sub-Neptune transiting bright ( K = 8.8), quiet, nearby (37 pc) M3V dwarf TOI-1266. validate planetary nature TOI-1266 b c using four sectors TESS photometry data from newly-commissioned 1-m SAINT-EX telescope located in San Pedro Mártir (México). also include additional ground-based follow-up as well high-resolution spectroscopy high-angular imaging observations. The inner, larger planet has radius R 2.37 −0.12 +0.16 ⊕ an orbital...
This work presents the design, implementation, and commissioning of infrastructure support services 1.3- meter COLIBRI robotic telescope site, located at Observatorio Astronómico Nacional en San Pedro Martir, Instituto de Astronomía- UNAM, Baja California, Mexico. is a ground-based telescope, associated with SVOM (Space Variable Object Monitor) mission dedicated to study gamma ray bursts. We share progress on building as well installations electrical systems, communications, air conditioning...
Cosmic explosions have emerged as a major field of astrophysics over the last years with our increasing capability to monitor large parts sky in different wavelengths and messengers (photons, neutrinos, gravitational waves). In this context, gamma-ray bursts (GRBs) play very specific role, they are most energetic Universe. The forthcoming Sino-French SVOM mission will make contribution scientific domain by improving understanding GRB phenomenon allowing their use understand infancy order...
This work describes the architectural design for construction of building COLIBRI robotic telescope, which has a 1.3 m primary mirror and forms part ground segment SVOM (Space Variable Object Monitor) mission dedicated to detection study gamma-ray bursts (GRBs). The is currently being installed. that will house telescope have total height 10 including dome. center contain concrete column with an independent foundation 2.5 in diameter 5.3 meter height. In addition it 2 levels (floors) control...
STRATEGIC MODEL OF COLLABORATION BETWEEN UNIVERSITY AND INDUSTRY TO R&D+I ASTRONOMICAL AEROSPACE INSTRUMENTATION PM4R-RIS3 APPROACH: PROPOSAL BAJA CALIFORNIA-SONORA MÉXICO
We present the design of tools and equipment needed for mounting dismounting M1, M2, M3 mirrors DDRAGO/CAGIRE instrument Colibrí telescope at observing room floor from there to ground level outside building. Also, it includes tool balance instruments that will be attach Nasmyth stations ones handle in vacuum chamber. Our designs confront problem handling these components very limited space available dome a fast alt-az telescope.