TY - GEN
T1 - New developments in integral field spectroscopy
AU - Horton, Anthony
AU - Bland-Hawthorn, Joss
AU - Ellis, Simon
PY - 2009/1/1
Y1 - 2009/1/1
N2 - The development of wide field adaptive optics (AO) capabilities greatly increases the potential information content (spatial resolution elements × spectral resolution elements) per telescope pointing. This is illustrated in Table 1, which lists the wide field AO systems for the VLT. The multi-conjugate adaptive optics (MCAO) demonstrator MAD has already proven that a 1′ corrected field of view (FoV) with point spread function (PSF) full width half-maximum (FWHM) of 0.1″ is possible [E. Marchetti, R. Brast et al. in ESO Messenger 129, 8 (2007)]. This corresponds to a number of spatial resolution elements, N sp=4×104. The two ground-layer adaptive optics (GLAO) systems currently under development promise comparable numbers. Comparing these figures with the seeing limited case for the maximum VLT FoV and good seeing we see that in terms of the number of spatial resolution elements the wide field AO foci of the VLT will be just as ‘wide field’ as any seeing limited instrument.
AB - The development of wide field adaptive optics (AO) capabilities greatly increases the potential information content (spatial resolution elements × spectral resolution elements) per telescope pointing. This is illustrated in Table 1, which lists the wide field AO systems for the VLT. The multi-conjugate adaptive optics (MCAO) demonstrator MAD has already proven that a 1′ corrected field of view (FoV) with point spread function (PSF) full width half-maximum (FWHM) of 0.1″ is possible [E. Marchetti, R. Brast et al. in ESO Messenger 129, 8 (2007)]. This corresponds to a number of spatial resolution elements, N sp=4×104. The two ground-layer adaptive optics (GLAO) systems currently under development promise comparable numbers. Comparing these figures with the seeing limited case for the maximum VLT FoV and good seeing we see that in terms of the number of spatial resolution elements the wide field AO foci of the VLT will be just as ‘wide field’ as any seeing limited instrument.
UR - http://www.scopus.com/inward/record.url?scp=85034639956&partnerID=8YFLogxK
U2 - 10.1007/978-1-4020-9190-2_76
DO - 10.1007/978-1-4020-9190-2_76
M3 - Conference proceeding contribution
AN - SCOPUS:85034639956
SN - 9781402091896
T3 - Astrophysics and Space Science Proceedings
SP - 423
EP - 427
BT - Science with the VLT in the ELT Era
A2 - Moorwood, Alan
PB - Springer, Springer Nature
T2 - Workshop on Science with the VLT in the ELT Era, 2007
Y2 - 8 October 2007 through 12 October 2007
ER -