Mr. Jorge Andres A. Uribe Uribe Profile

Jorge Andres A. Uribe Uribe

Opt-mechanics Manager at Ctr de Ingenieria y Desarrollo Industrial

Publications (11)

Proceedings Article | 6 July 2018 Paper

Mechanical preliminary design of the 6.5-meter Telescopio San Pedro Mártir (TSPM)

Jorge Uribe, Carlos Tovar, Rogelio Manuel, Saúl Rubio, Carlos Ortega, German González, Berenice Rodríguez, William Lee, Michael Richer, J. Jesús González, Cesar Martínez, Vicente Bringas, Antonio Estrada

Proceedings Volume 10700, 107005U (2018) https://doi.org/10.1117/12.2313102

KEYWORDS: Telescopes, Optical instrument design, Mechanical engineering, Mirrors, Finite element methods, 3D modeling, Structural design, Observatories

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Proceedings Article | 6 July 2018 Presentation + Paper

The Telescopio San Pedro Mártir project

Michael Richer, William Lee, Leopoldo Altamirano, J. Jesús González, Charles Alcock, Buell Jannuzi, Fabián Rosales-Ortega, Marisa García-Vargas, Joel Herrera Vázquez, Derek Hill, María Herlinda Pedrayes, Ana Pérez Calpena, Mauricio Reyes Ruiz, Lino Hector Rodríguez Merino, Beatriz Sánchez, Hazael Serrano Guerrero, Gerardo Sierra Díaz, Andrew Szentgyorgyi, Jose Teran, David Urdaibay, Jorge Andrés Uribe Uribe, Alan Watson, Dennis Zaritsky, Mario Rascon, Urania Ceseña Borbón, Francisco Murillo Bracamontes, Fernando Quirós Parra, Erika Sohn

Proceedings Volume 10700, 107000Z (2018) https://doi.org/10.1117/12.2313069

KEYWORDS: Telescopes, Mirrors, Imaging spectroscopy, Observatories, Optical instrument design, Astronomy, Control systems, Interfaces

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Proceedings Article | 9 August 2016 Paper

FRIDA: diffraction-limited imaging and integral-field spectroscopy for the GTC

Alan Watson, José Acosta-Pulido, Luis Álvarez-Núñez, Vicente Bringas-Rico, Nicolás Cardiel, Salvador Cardona, Oscar Chapa, José Javier Díaz García, Stephen Eikenberry, Carlos Espejo, Rubén Flores-Meza, Jorge Fuentes-Fernández, Jesús Gallego , José Leonardo Garcés Medina, Francisco Garzón López, Peter Hammersley, Carolina Keiman, Gerardo Lara, José Alberto López, Pablo López, Diana Lucero, Heidy Moreno Arce, Sergio Pascual Ramirez, Jesús Patrón Recio, Almudena Prieto, Alberto José Rodríguez, José Marco de la Rosa, Beatriz Sánchez, Jorge Uribe, Francisco Váldez Berriozabal

Proceedings Volume 9908, 99080P (2016) https://doi.org/10.1117/12.2233069

KEYWORDS: Imaging spectroscopy, Spectroscopy, System integration, Adaptive optics, Sensors, Cameras, Spectrographs, Mirrors, Optical filters, Control systems

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Proceedings Article | 8 August 2016 Paper

San Pedro Martir Telescope: Mexican design endeavor

Gengis Toledo-Ramirez, Vicente Bringas-Rico, Noe Reyes, Jorge Uribe, Aldo Lopez, Carlos Tovar, Xochitl Caballero, Luis Del-Llano, Cesar Martinez, Eduardo Macias, William Lee, Alberto Carramiñana, Michael Richer, Jesús González, Beatriz Sanchez, Diana Lucero, Rogelio Manuel, Jose Segura, Saul Rubio, German Gonzalez, Obed Hernandez, Mary García, Jose Lazaro, Fabian Rosales-Ortega, Joel Herrera, Gerardo Sierra, Hazael Serrano

Proceedings Volume 9906, 99060S (2016) https://doi.org/10.1117/12.2231732

KEYWORDS: Optical instrument design, Telescope design, Mirrors, Telescopes, Telescopes, Optical instrument design, Mirrors, Astronomy, Control systems, Systems engineering, Manufacturing, Systems modeling, Control systems design

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The Telescopio San Pedro Martir (TSPM) is a new ground-based optical telescope project, with a 6.5 meters honeycomb primary mirror, to be built in the Observatorio Astronomico Nacional on the Sierra San Pedro Martir (OAN-SPM) located in Baja California, Mexico. The OAN-SPM has an altitude of 2830 meters above sea level; it is among the best location for astronomical observation in the world. It is located 1830 m higher than the atmospheric inversion layer with 70% of photometric nights, 80% of spectroscopic nights and a sky brightness up to 22 mag/arcsec2.

The TSPM will be suitable for general science projects intended to improve the knowledge of the universe established on the Official Mexican Program for Science, Technology and Innovation 2014-2018. The telescope efforts are headed by two Mexican institutions in name of the Mexican astronomical community: the Universidad Nacional Autonoma de Mexico and the Instituto Nacional de Astrofisica, Optica y Electronica. The telescope has been financially supported mainly by the Consejo Nacional de Ciencia y Tecnologia (CONACYT). It is under development by Mexican scientists and engineers from the Center for Engineering and Industrial Development. This development is supported by a Mexican-American scientific cooperation, through a partnership with the University of Arizona (UA), and the Smithsonian Astrophysical Observatory (SAO). M3 Engineering and Technology Corporation in charge of enclosure and building design.

The TSPM will be designed to allow flexibility and possible upgrades in order to maximize resources. Its optical and mechanical designs are based upon those of the Magellan and MMT telescopes. The TSPM primary mirror and its cell will be provided by the INAOE and UA. The telescope will be optimized from the near ultraviolet to the near infrared wavelength range (0.35-2.5 m), but will allow observations up to 26μm. The TSPM will initially offer a f/5 Cassegrain focal station. Later, four folded Cassegrain and two Nasmyth focal stations are contemplated, nominally with focal ratios of f/5 and f/11. The concept will allow the use of existing instruments like MMIRS and MEGACAM. Available experience from currently working ground-based telescopes will be integrated with up-to-date technology specially for control and information management systems.

Its mount is the well-known azimuth-elevation configuration. The telescope total mass is estimated in about 245 metric tons, with a total azimuth load of 185 metric tons including around 110 metric tons as the total elevation load. A tracking error lower than 0.03 arcsec RMS is expected under steady wind up to 50 Km/h. An open-loop pointing accuracy between 10 and 2 arcsec is planned. The TSPM is in its design phase. It is the first large optical ground-based telescope to be designed and developed primarily by Mexican scientists and engineers. This endeavor will result in the improvement of the scientific and technical capabilities of Mexico including complex scientific instruments development, systems engineering and project management for large engineering projects. In this paper, which aims to gather the attention of the community for further discussions, we present the engineering preliminary design, the basic architecture and challenging technical endeavors of the TSPM project.

Proceedings Article | 27 July 2016 Paper

Mechanical conceptual design of 6.5 meter telescope: Telescopio San Pedro Mártir (TSPM)

Jorge Uribe, Vicente Bringas, Noe Reyes, Carlos Tovar, Aldo López, Xóchitl Caballero, César Martínez, Gengis Toledo, William Lee, Alberto Carramiñana, Jesús González, Michael Richer, Beatriz Sánchez, Diana Lucero, Rogelio Manuel, Saúl Rubio, Germán González, Obed Hernández, José Segura, Eduardo Macias, Mary García, José Lazaro, Fabián Rosales, Luis del Llano

Proceedings Volume 9906, 99062E (2016) https://doi.org/10.1117/12.2232666

KEYWORDS: Telescopes, Optical instrument design, Mechanical engineering, Observatories, Mirrors, Manufacturing, Optical instrument design, Mechanical engineering, Space telescopes, Telescope design, Sodium, Design for manufacturability

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Telescopio San Pedro Mártir (TSPM) project intends to build a 6.5 meters telescope with alt-azimuth design, currently at the conceptual design. The project is an association between Instituto de Astronomía de la Universidad Nacional Autónoma de México (IA-UNAM) and the Instituto Nacional de Astrofísica, Óptica Electrónica (INAOE) in partnership with department of Astronomy and Steward Observatory of University of Arizona and Smithsonian Astrophysical Observatory of Harvard University. Conceptual design of the telescope is lead and developed by the Centro de Ingeniería y Desarrollo Industrial (CIDESI). An overview of the feasibility study and the structural conceptual design are summarized in this paper. The telescope concept is based on telescopes already commissioned such as MMT and the Baade and Clay Magellan telescopes, building up on these proven concepts. The main differences relative to the Magellan pair are; the elevation axis is located 1 meter above the primary mirror vertex, allowing for a similar field of view at the Cassegrain and both Nasmyth focal stations; instead of using a vane ends to position the secondary mirror TSPM considers an Steward platform like MMT; finally TSPM has a larger floor distance to m1 cell than Magellans and MMT. Initially TSPM will operate with an f/5 Cassegrain station, but the design considers further Nasmyth configurations from a Cassegrain f/5 up to a Gregorian f/11. The telescope design includes 7 focal stations: 1 Cassegrain; 2 Nasmyth; and 4 folded-Cassegrain. The telescope will be designed and manufactured in Mexico, will be design in Queretaro by CIDESI and built between Queretaro and Michoacán manufacturing facilities; it will be preassembled in these facilities and disassembled to send it to the San Pedro Mártir Observatory for final integration. The azimuth and altitude structure is planned to be constructed in modules and transported by truck and shipped to Ensenada and finally to the OAN where is going to be finally assembled, verified and tested.

Proceedings Article | 27 July 2016 Paper

The Telescopio San Pedro Mártir project

Michael Richer, William Lee, Jesús González, Buell Jannuzi, Beatriz Sánchez, Fabián Rosales Ortega, Charles Alcock, Alberto Carramiñana Alonso, Ma. Teresa García Díaz, Leonel Gutiérrez, Joel Herrera, Derek Hill, Timothy Norton, Maria Pedrayes, Ana Pérez-Calpena, Mauricio Reyes-Ruíz, Hazael Serrano Guerrero, Gerardo Sierra, Jose Teran, David Urdaibay, Jorge Uribe, Alan Watson, Dennis Zaritsky, Marisa García Vargas

Proceedings Volume 9906, 99065S (2016) https://doi.org/10.1117/12.2232000

KEYWORDS: Telescopes, Atmospheric Cherenkov telescopes, Observatories, Mirrors, Astronomy, Optical instrument design, Telescopes, Control systems, Optics manufacturing, Optical alignment, Interfaces

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Proceedings Article | 4 August 2014 Paper

FRIDA diffraction limited NIR instrument: the challenges of its verification processes

Be. Sánchez, C. Keiman, C. Espejo, S. Cuevas, L. Álvarez, O. Chapa, R. Flores-Meza, J. Fuentes, L. Garcés, G. Lara, J. A. López, R. Rodríguez, A. Watson, V. Bringas, A. Corrales, D. Lucero, A. Rodríguez, B. Rodríguez, D. Torres, J. Uribe

Proceedings Volume 9150, 91501R (2014) https://doi.org/10.1117/12.2057439

KEYWORDS: Cameras, Collimators, Mirrors, Current controlled current source, Diffraction, Near infrared, Iterated function systems, Cryogenics, Spectrographs, Prototyping

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Proceedings Article | 8 July 2014 Paper

FRIDA, the diffraction limited NIR imager and IFS for the Gran Telescopio Canarias: status report

J. López, J. Acosta, L. Alvarez, V. Bringas, N. Cardiel, D. Clark, A. Corrales, S. Cuevas, O. Chapa, J. J. Díaz Garcia, S. Eikenberry, C. Eliche, C. Espejo, R. Flores, J. Fuentes, J. Gallego, J. Garcés, F. Garzón, P. Hammersley, C. Keiman, G. Lara, P. López, D. Lucero, H. Moreno, S. Pascual, J. Patrón, A. Prieto, A. Rodríguez, B. Rodríguez, B. Sánchez, D. Torres, J. Uribe, A. Watson

Proceedings Volume 9147, 91471P (2014) https://doi.org/10.1117/12.2057236

KEYWORDS: Cameras, Spectrographs, Iterated function systems, Sensors, Optics manufacturing, Imaging systems, Mirrors, Optical components, System integration, Adaptive optics

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Proceedings Article | 24 September 2012 Paper

Electronics and mechanisms control system for FRIDA (inFRared Imager and Dissector for Adaptive optics)

R. Flores-Meza, S. Cuevas, J. Díaz, C. Espejo, C. Keiman, G. Lara, B. Sánchez, J. Uribe

Proceedings Volume 8451, 84513H (2012) https://doi.org/10.1117/12.926729

KEYWORDS: Control systems, Electronics, Control systems design, Sensors, Prototyping, Temperature sensors, Photonic integrated circuits, Human-machine interfaces, Optical benches, Infrared radiation

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Proceedings Article | 24 September 2012 Paper

Current status of FRIDA: diffraction limited NIR instrument for the GTC

Beatriz Sánchez, José Acosta, Luis Álvarez, Vicente Bringas, Nicolás Cardiel, Adi Corrales, Salvador Cuevas, Oscar Chapa, José Javier Díaz, Stephen Eikenberry, Carmen Eliche, Carlos Espejo, Rubén Flores, Francisco Garzón, Peter Hammersley, Carolina Keiman, Gerardo Lara, José López, Pablo López, Diana Lucero, Jose Manuel Montoya, Heidy Moreno, Sergio Pascual, Jesús Patrón, Almudena Prieto, N. Raines, Alberto Rodríguez, Jorge Uribe, Alan Watson

Proceedings Volume 8446, 844624 (2012) https://doi.org/10.1117/12.926499

KEYWORDS: Cameras, Diffraction, Sensors, Spectrographs, Optical benches, Near infrared, Adaptive optics, Iterated function systems, Prototyping, Imaging systems

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Proceedings Article | 13 September 2012 Paper

Frida integral field unit opto-mechanical design

Salvador Cuevas, Stephen Eikenberry, Vicente Bringas, Adi Corrales, Carlos Espejo, Diana Lucero, Alberto Rodriguez, Beatriz Sánchez, Jorge Uribe

Proceedings Volume 8450, 84504I (2012) https://doi.org/10.1117/12.925504

KEYWORDS: Mirrors, Iterated function systems, Spectrographs, Ray tracing, Diffraction, Off axis mirrors, Diffraction gratings, Adaptive optics, Imaging systems, Sensors

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Showing 5 of 11 publications

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