Scientific potential of enhancing the integral-field spectrometer SPIFFI with a large detector and high spectral resolution
ESO ASTROPHY SYMP (2002) 149-157
Abstract:
SPIFFI is the near-infrared integral-field spectrometer for the VLT. Assisted by the SINFONI adaptive optics module, the instrument will be offered to the astronomical community in 2004. We outline the scientific rationale for infrared integral-field spectroscopy at the VLT, and specifically for the enhancement of SPIFFI with a larger detector and higher spectral resolution gratings. We give examples of a broad variety of astronomical research which will gain specifically from the high angular and spectral resolution provided by SPIFFI, including studies of high red-shift galaxies, merging galaxies, starburst galaxies, superstar clusters, galactic nuclei, extra-solar planets, and circum-stellar discs.The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 329:1 (2002) 87-101
The 2dF Galaxy Redshift Survey:: the bJ-band galaxy luminosity function and survey selection function
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 336:3 (2002) 907-931
The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 333:1 (2002) 133-144
The 2dF Galaxy Redshift Survey: Constraints on cosmic star formation history from the cosmic spectrum
ASTROPHYSICAL JOURNAL 569:2 (2002) 582-594