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| DOI | 10.1088/1538-3873/129/973/035005 | ||||
| Año | 2017 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Cloud cover and water vapor conditions in the southwestern USA and northern Mexico were surveyed as a preparatory work for the Thirty Meter Telescope (TMT) in situ site testing program. Although the telescope site is already selected, the TMT site testing team decided to make public these results for its usefulness for the community. Using 58 months of meteorological satellite observations between 1993 July and 1999 September, different atmospheric parameters were quantified from data of the 10.7 mu m and of 6.7 mu m windows. In particular, cloud cover and water vapor conditions were identified in preferred areas. As a result of the aerial analysis, 15 sites of existing and potential telescope were selected, compared, and ranked in terms of their observing quality. The clearest sites are located along the spine of the Baja peninsula and into southern California on mountain peaks above the temperature inversion layer. A steep gradient of cloudiness was observed along the coast where coastal cloud and fog are trapped below the inversion layer. Moving from west to east over the continent, a significant increase in cloudiness was observed. The analysis shows that San Pedro Martir, San Gorgonio Mountain and San Jacinto Peak have the largest fraction of clear sky conditions (similar to 74%). The site with the optimal combination of clear skies and low precipitable water vapor is Boundary Peak, Nevada. An approach based in satellite data provided a reliable method for sites comparison.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | CARRASCO-LICEA, ESPERANZA | Mujer |
Inst Nacl Astrofis Opt & Electr - México
Instituto Nacional de Astrofisica Optica y Electronica - México |
| 2 | AVILA-RUBIO, RICARDO FELIX | Hombre |
Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México UNAM campus Juriquilla - México |
| 3 | Erasmus, A. | - |
South African Astron Observ - República de Sudáfrica
South African Astronomical Observatory - República de Sudáfrica |
| 4 | Djorgovski, S. G. | - |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos |
| 5 | WALKER, ALISTAIR | Hombre |
Natl Opt Astron Observ - Chile
Cerro Tololo Inter American Observatory - Chile National Optical Astronomy Observatory - Chile |
| 6 | Blum, Robert | Hombre |
Natl Opt Astron Observ - Estados Unidos
National Optical Astronomy Observatory - Estados Unidos |
| Fuente |
|---|
| Universidad Nacional Autónoma de México |
| University of Tokyo |
| European Southern Observatory |
| South African Astronomical Observatory |
| Instituto de Astronomia (Universidad Nacional Autonoma de Mexico) |
| CELT project (University of California) |
| Mt. Graham International Observatory (University of Arizona) |
| CELT project (California Institute of Technology) |
| Observatorio Astronomico Nacional de San Pedro Martir |
| Instituto de Astronom?a |
| Universidad Nacional Aut?noma de M?xico |
| University of California and California Institute of Technology |
| Instituto de Astronomía |
| Direct For Mathematical & Physical Scien; Division Of Astronomical Sciences |
| Agradecimiento |
|---|
| The results presented in this paper were based in a study funded by the CELT project (University of California and California Institute of Technology). The data were purchased by Cerro Tololo Inter-American Observatory, the University of Tokyo, and the European Southern Observatory. Mt. Graham International Observatory (University of Arizona); the Observatorio Astronomico Nacional de San Pedro Martir and the Instituto de Astronomia (Universidad Nacional Autonoma de Mexico); and the South African Astronomical Observatory are also acknowledged for their support. |
| The results presented in this paper were based in a study funded by the CELT project (University of California and California Institute of Technology). The data were purchased by Cerro Tololo Inter-American Observatory, the University of Tokyo, and the European Southern Observatory. Mt. Graham International Observatory (University of Arizona); the Observatorio Astrónomico Nacional de San Pedro Mártir and the Instituto de Astronomía (Universidad Nacional Autónoma de México); and the South African Astronomical Observatory are also acknowledged for their support. |