Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/vscience/schedule/tpfiles/SchneidertagA2416tp.pdf
Дата изменения: Wed Jun 11 19:00:26 2008
Дата индексирования: Wed Jan 14 17:34:40 2009
Кодировка:

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Proposal Identification No.:

A2416

Date Received:

2008-Jun-02 17:00:41

Technical Page
Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Extragalactic 62 Hours 1 hour

The HI masses of galaxies as a function of stellar luminosity

We propose to follow up on Nancay non-detections of a sample of SDSS galaxies. The sample is designed to provide an unbiased cross-section of galaxy stellar and HI mass content for galaxies of various luminosities. The observations already carried out at Nancay have detected over 60 percent of the galaxies, showing surprises both in the galaxies that were detected and that were undetected. Arecibo observations will provide much more sensitive limits or detections and more clearly characterize the HI characteristics of these galaxies.

Name Stephen E Schneider

Institution Univ. of sachusetts

Mas-

E-mail schneider@astro.umass.edu

Phone 413-545-2076

Student no

Remote Observing Request

Observer will travel to AO X Remote Observing In Absentia (instructions to operator)

Instrument Setup
L-wide Atmospheric Observation Instruments:

Sp ecial Equipment or setup:

none

RFI Considerations Frequency Ranges Planned
1


1360-1420 MHz This proposal requires coordination with Punta Salinas radar within the band 1222-1381 MHz.. This proposal requires coordination with GPS L3 at 1381 MHz.

2