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Thanks to our sponsors ♦ The OAN-SPM has been supported by the Consejo Nacional de Ciencia y Tecnología (CONACyT) through projects Laboratorios Nacionales LN-232649 in 2014, LN-260369 in 2015, and LN-271117 in 2016.
♦ El OAN-SPM has been supported fron the Consejo Nacional de Ciencia y Tecnología (CONACyT) through the project 122736 Laboratorio de Astrofísica en San Pedro Mártir, B.C 2010-2013. |
Form for service-mode observations with:
Contact:
Originally written by: Michael Richer
Updated by: Ilse Plauchu Frayn (September 28th, 2020)
To all personnel and users of the OAN-SPM
ln spite of its natural beauty, there exist important workplace hazards at the Observatorio Astronómico Nacional in the Sierra de San Pedro Mártir (OAN-SPM). Given that the OAN-SPM is more than three hours travel from the nearest medical centre, it is essential to adopt safe work practices to minimize the risk of accidents. Safety begins with one’s actions and habits, so please use common sense to help keep yourself and others safe. Please also remember that everyone's safety is a shared responsibility.
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1.- Always carry a flashlight and use it when you are in dark places, indoors or out (dormitory, telescopes, parking lots, etc.). If you do not have a flashlight, ask the site Head of Operations (a.k.a. supervisor) for one.
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2.- The Head of Operations may supply you with a vehicle for use within the observatory (valid driver’s license required). If you must drive at night (please minimize this), use the car’s normal headlights. Ask someone else to drive when the road is snow-covered if you lack experience driving under these conditions.
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3.- At the end of the night, wait for the telescope operator to finish all operations (close the dome, fill the dewar, etc.) so that everyone can go to the dormitory together. Many of the highest-risk activities undertaken by the telescope operator occur at the beginning and end of the night, so it is best that she or he is accompanied.
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4.- Inform others of your activities, especially at night or if you will be far from commonly frequented areas (buildings). If you are accompanied at the telescope, notify others of your whereabouts. If someone is away longer than expected, check and make sure that all is well.
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5.- If you leave the main observatory areas (dormitory, workshops, telescopes), to go hiking or walking, it is best to do so accompanied. Always notify the Head of Operations; request a radio and instructions of how to use it so that you may call for help if needed.
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6.- Obey all signs as well as instructions from the site Head of Operations. If any sign’s meaning is unfamiliar, ask for an explanation, but never ignore it.
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7.- In case of any emergency or dangerous situation, immediately notify the site Head of Operations, medical personnel or other observatory personnel.
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8.- If you feel ill or if someone tells you they are ill, notify someone immediately (at all hours), preferably the site Head of Operations. If you have a medical condition, even if it allows you to travel, notify the Head of the observatory before going up to the observatory and bring all your prescription medicine with you.
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CanHiS (Cananea High-Resolution Spectrograph) is an echelle f / 13.5 spectrograph, "R3.2", which can reach a very high resolution (R ≈ 40000 with a 100 micron slit, up to R ≈ 180000 with a 25 micron slit ). Its "quasi-Littrow" type design makes use of bandpass filters (instead of a cross dispersor), to isolate individual dispersion orders. Its average coverage range is from approximately 50 Å (about 4500 Å), to 140 Å (about 7800 Å). CanHis can be used in direct mode coupled to the 2.1m telescope stage or with fibers and the FICUS polarization analysis module.
Documents:
Contact:
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This FICUS polarization module (FIber Copled Unit System) is used exclusively with the 2.1m telescope of the OAN-SPM. It is a module that was designed to be able to be coupled to the Boller & Chivens spectrograph (low and intermediate resolution) without being coupled to the telescope. This module was designed to work in the F / 7 configuration. FICUS was designed to observe specific objects (the input is limited to a 250 micrometer pinhole).
Documents:
