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A1625 2002-Feb-01 15:13:28
Technical Page
Proposal Type: Long-term
General Category: Astronomy
Sub-Category: Spectroscopy
Observation Category: Extragalactic
Total Time Requested: 45 Hours
Proposal Title: Properties of the ISM of a sample of the most isolated galaxies: Atomic gas
content.
ABSTRACT:
We are studying a large sample of completely isolated galaxies in order to analyze star formation and galaxy
evolution independent of exterior in uences. Our source is the Catalog of Isolated Galaxies and our sample
contains 760 galaxies for which we are building a multiwavelength database. We already collected old and new
unpublished optical and FIR data which enabled us to study luminosities and global properties of the sample, and
we are currently obtaining/compiling HI, CO and H data. We searched the NED and the HI catalog Huchtmeier
and Richter (1989) nding available HI spectra for half of the sample. Among the rest, we are currently observing
 60 galaxies at the Green Bank Telescope. We have splitted the rest of the sample between Arecibo and other
radiotelescopes according to sensitivity and declination, in order to complete the HI database of the full sample.
Here we ask for observing time to observe 62 galaxies with the Arecibo radio telescope.
Name Institution E-mail Phone Student
Lourdes Verdes-Montenegro Instituto de As-
trosica de Andalu-
cia
lourdes@iaa.es (34) 958121311 no
Service Observing Request Remot e Observing Request
X None X No
All of the observing run. Maybe
Part of the observing run. Yes
Queue Observing
Instrument Setup
L-wide
Atmospheric Observation Instruments:
Special Equipment or setup: none
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RFI Considerations
Frequency Ranges Planned
1320-1397 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.
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