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008			150903s2008 gw | o |||| 0|eng d
020			_a9783540754855 _99783540754855
024	7		_a10.1007/9783540754855 _2doi
035			_avtls000351093
039		9	_a201509030504 _bVLOAD _c201405060245 _dVLOAD _y201402171113 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB1-991
100	1		_aSantos, Nuno C. _eeditor. _9334133
245	1	0	_aPrecision Spectroscopy in Astrophysics : _bProceedings of the ESO/Lisbon/Aveiro Conference held in Aveiro, Portugal, 11–15 September 2006 / _cedited by Nuno C. Santos, Luca Pasquini, Alexandre C. M. Correia, Martino Romaniello.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2008.
300			_brecurso en línea.
336			_atexto _btxt _2rdacontent
337			_acomputadora _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_aarchivo de texto _bPDF _2rda
490	0		_aESO Astrophysics Symposia, European Southern Observatory, _x1431-2433
500			_aSpringer eBooks
505	0		_aPart I Abundances and Isotopes -- Part II QSO Absorption Lines -- Part III Fundamental Constants -- Part IV Beyond Photon Noise -- Part V Asteroseismology/Oscillations -- Part VI Planets -- Part VII Future Developments -- Part VIII Posters.
520			_aHigh-accuracy Doppler shift measurements and high-precision spectroscopy are primary techniques in the search for exo-planets. Further extremely interesting applications include the analysis of QSO absorption lines to determine the variability of physical constants and the analysis of the isotopic ratios of absorption lines both in stars and in QSOs, and the determination of stellar oscillations through radial velocity measurements. Since the use of high-precision/resolution spectroscopy is closely connected to the ability to collect a large number of photons, the scientific domains using this technique benefit tremendously from the use of 8-meter class telescopes and will fully exploit the tremendous gain provided by future Extremely Large Telescopes (ELTs). IR high-resolution spectroscopy should soon approach the same accuracy regime achieved in the optical range. This volume comprehensively covers the astrophysical and technical aspects of high-precision spectroscopy with an outlook to future developments, and represents a useful reference work for researchers in those fields.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700	1		_aPasquini, Luca. _eeditor. _9330447
700	1		_aCorreia, Alexandre C. M. _eeditor. _9334134
700	1		_aRomaniello, Martino. _eeditor. _9334135
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9783540754848
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-540-75485-5 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c298045 _d298045