Abstract
SETHi is a survey of the distribution of galactic neutral hydrogen being performed comensally at the NAIC Arecibo Observatory. At the same time that observers use receivers in the Gregorian dome, SETHi is recording a 2.5MHz band centered at 1420 MHz from a flat feed on Carriage House 1. During normal astronomical observations, the SETHi feed scans across the sky at twice the sidereal rate. During 4 years of observations, we have accumulated over 15,000 hours of data covering most of the sky accessible to Arecibo. This survey has higher angular resolution than existing single dish surveys and higher sensitivity than existing or planned interferometric surveys.
These data are being converted into spectra and is housed in a database at UCB. It is our intention to make this data publicly accessible. We briefly discuss the status of this effort and show some results obtained with this data.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Korpela et al. 2001, Computing in Science and Engineering 3, 79
Werthimer et al. 1997, in Astronomical and Biochemical Origins and the Search for Life in the Universe, eds: Cosmovici, Bowyer, & Werthimer, (Bologna: Editrice Compositori), p. 711
Haffner et al. 2003, ApJS 149, 405
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2004 Kluwer Academic Publishers
About this paper
Cite this paper
Korpela, E.J., Demorest, P., Heien, E., Heiles, C., Werthimer, D. (2004). Latest Results of the Sethi Survey at Arecibo. In: Alfaro, E.J., Pérez, E., Franco, J. (eds) How does the Galaxy Work?. Astrophysics and Space Science Library, vol 315. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2620-X_18
Download citation
DOI: https://doi.org/10.1007/1-4020-2620-X_18
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-2619-5
Online ISBN: 978-1-4020-2620-1
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)