Benjamin Martinez

First Light with RATIR: An Automated 6-band Optical/NIR Imaging Camera

The Reionization and Transients InfraRed camera (RATIR) is a simultaneous optical/NIR multi-band imaging camera which is 100% time-dedicated to the followup of Gamma-ray Bursts. The camera is mounted on the 1.5-meter Johnson telescope of the Mexican Observatorio Astronomico Nacional on Sierra San Pedro Martir in Baja California. With rapid slew capability and autonomous interrupt capabilities, the system will image GRBs in 6 bands (i, r, Z, Y, J, and H) within minutes of receiving a satellite position, detecting optically faint afterglows in the NIR and quickly alerting the community to potential GRBs at high redshift (z>6-10). We report here on this Springs first light observing campaign with RATIR. We summarize the instrumental characteristics, capabilities, and observing modes.

Automation of the OAN/SPM 1.5-meter Johnson telescope for operations with RATIR

The Reionization And Transients Infra-Red (RATIR) camera is intended for robotic operation on the 1.5-meter Harold Johnson telescope of the Observatorio Astronómico Nacional on the Sierra de San Pedro Mártir, Baja California, Mexico. This paper describes the work we have carried out to successfully automate the telescope and prepare it for RATIR. One novelty is our use of real-time absolute astrometry from the finder telescopes to point and guide the main telescope.

Surface roughness results using a hydrodynamic polishing tool (HyDra)

HyDRa is a hydrodynamic radial polishing tool ideal for the corrective lapping and fine polishing of diverse materials by means of an accelerated abrasive flux. The roughness of an optical surface is analysed for a continuous manufacturing process, beginning with the basic generation steps up to a finished optical surface. These results were obtained using a Linnik interferometer.

Polishing TIM mirror segments with HyDra

We report experimental results and analysis about a new hydrodynamic radial tool (HyDra, patent pending), which expels a suspension of water and polishing particles radially on glass. With this method it is possible to locally shape optical surfaces. The depth of material removed by HyDra grows linearly with the time. The removal rate is independent of the velocity between the tool and the glass element. The HyDra has been used to fabricate successfully an optical flat and Schmidt surface.

HyDra: A novel hydrodynamic polishing tool for high quality optical surfaces

A novel hydrodynamic radial polishing tool (HyDRa) is presented. It performs corrective lapping and fine polishing of diverse materials by means of a low-cost abrasive flux and a hydrostatic suspension system that avoids contact of the tool with the working surface. With this tool it is currently possible to polish aspheres and free-form optics of up to 2.5 meters in diameter. It has the advantage of avoiding fallen edges during the polishing process as well as reducing tool wear out and deformation. The functioning principle is based on the generation of a high-velocity, high-pressure abrasive emulsion flux with radial geometry. The polishing process is repeatable and achieves high degrees of precision and accuracy on optical and semiconductor surfaces. An additional advantage of this new tool is the possibility to perform in-process interferometric measurements. Recent results of polished aspheres are discussed.

New perspectives in hydrodynamic radial polishing techniques for optical surfaces

In order to overcome classic polishing techniques, a novel hydrodynamic radial polishing tool (HyDRa) is presented; it is useful for the corrective lapping and fine polishing of diverse materials by means of a low-cost abrasive flux and a hydrostatic suspension system that avoids contact of the tool with the working surface. This tool enables the work on flat or curved surfaces of currently up to two and a half meters in diameter. It has the advantage of avoiding fallen edges during the polishing process as well as reducing tool wear out and deformation. The functioning principle is based on the generation of a high-velocity, high-pressure, abrasive emulsion flux with radial geometry. The polishing process is repeatable by means of the control of the tool operational parameters, achieving high degrees of precision and accuracy on optical and semiconductor surfaces, with removal rates of up to 9 mm3/hour and promising excellent surface polishing qualities. An additional advantage of this new tool is the possibility to perform interferometric measurements during the polishing process without the need of dismounting the working surface. A series of advantages of this method, numerical simulations and experimental results are described.

Optics and the mechanical system of the 62-cm telescope at the Severo Díaz Galindo Observatory in Guadalajara, Jalisco, México

We present the results of a modification performed in the optical system of the 62 cm telescope (f/14.32) at observatory “Severo Díaz Galindo” Universidad de Guadalajara, Mexico. This modification consists of a change of distance between the primary and secondary mirrors from 1020 to 1135 mm. With this, a change in the image plane from 5200 mm to 600 mm, measured from the vertex of the primary mirror, is obtained. The latter allow to get the first astronomical images of The Telescope. This modification was necessary because alignment errors, such as distance between primary and secondary mirrors in the original system were presented. Besides, the telescope has a new accurate and adequate mechanical system installed on November 2011. Details and the first images obtained, are here presented.

New results in hydrodynamic radial polishing using HyDRa

New results using hydrodynamic radial polishing techniques on assorted materials, using HyDRa are presented. This tool performs corrective lapping and fine polishing by means of a low-cost, foamy abrasive flux. The functioning principle is based on the generation of a grazing, high-velocity, low-pressure, rotational, variable density, abrasive flux with radial geometry. It is currently possible to polish aspheres and free-form optics on diverse materials and sizes. This tool is particularly useful for polishing thin substrates such as membranes and semiconductors since it can be biased for a non-interactive action on the work piece. This process also has the advantage of achieving high removal rates. In order to achieve high degrees of accuracy and repeatability in the HyDRa finishing process, fully automated bias and slurry supply units must be incorporated to the polishing system. The air and slurry supply systems are described, as well as operational tool parameters for optimal polishing performance.