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Дата изменения: Tue Sep 11 04:14:21 2012
Дата индексирования: Tue Feb 5 00:31:02 2013
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Proposal Identification No.:

A2749 Arecibo Observatory

Date Received: 2012-Sep-04 09:18:57 William E. Gordon Telescope Observing Time Request COVER SHEET

Section I - General Information
Submitted for Sep 1 2012. This proposal has been submitted before. The previous proposal number is A2666, A2703. Proposal Type: General Category: Sub-Category: Observation Category: Time Requested this semester: Hours Next Semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time: Expected Data Storage: Prop osal Title: ABSTRACT: The GALEX Arecibo SDSS Survey (GASS) was a large Arecibo program that measured the HI content of about 1000 massive (M*>1e10 Msun) galaxies in the local Universe. Here we propose to extend GASS to a lower stellar mass regime (1e9
Insights into the Physical Processes that Regulate Star-forming Systems: The Low Stellar Mass GASS Extension

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Name Barbara Catinella David Schiminovich

Institution Max Planck Institute for Astrophysics Columbia University

E-mail bcatinel@mpa-garching.mpg.de ds@astro.columbia.edu

Phone +49 89 30000 2233 +1 212 8547819

Student no no

Additional Authors
GASS and COLD GASS Teams (see proposal)

This work is not part of a thesis.

Remote Observing Request

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

Section I I - Time Request
The following times are in LST. For these observations night-time is required.

Begin ­ End Interval­Interval 08 ­ ­ ­ ­ 15

Days Needed at This Interval 23

Time Constraints (Must Be Justified in the Prop osal Text)

Next Semester Time Request

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Begin ­ End Interval­Interval 23 ­ ­ ­ ­ 02

Days Needed at This Interval 6

Time Constraints (Must Be Justified in the Prop osal Text)

Section I I I - Instruments Needed
L-wide Atmospheric Observation Instruments:

Sp ecial Equipment or setup:

none

Section IV - RFI Considerations Frequency Ranges Planned
1392 - 1406 This proposal requires coordination with Punta Salinas radar within the band 1222-1381 MHz.. This proposal requires coordination with GPS L3 at 1381 MHz.

Section V - Observing List Target List
see Justification

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