H alpha kinematics of the SINGS nearby galaxies survey - I
Abstract
This is the first part of an H alpha kinematics follow-up survey of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample. The data for 28 galaxies are presented. The observations were done on three different telescopes with Fabry-Perot of New Technology for the Observatoire du mont Megantic (FaNTOmM), an integral field photon-counting spectrometer, installed in the respective focal reducer of each telescope. The data reduction was done through a newly built pipeline with the aim of producing the most homogenous data set possible. Adaptive spatial binning was applied to the data cubes in order to get a constant signal-to-noise ratio across the field of view. Radial velocity and monochromatic maps were generated using a new algorithm, and the kinematical parameters were derived using tilted-ring models.
Más información
| Título según WOS: | ID WOS:000236064800004 Not found in local WOS DB |
| Título de la Revista: | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
| Volumen: | 367 |
| Número: | 2 |
| Editorial: | OXFORD UNIV PRESS |
| Fecha de publicación: | 2006 |
| Página de inicio: | 469 |
| Página final: | 512 |
| DOI: |
10.1111/j.1365-2966.2006.10002.x |
| Notas: | ISI |