MIT Libraries logoDSpace@MIT

MIT
View Item 
  • DSpace@MIT Home
  • Haystack Observatory
  • ALMA Phasing Project
  • View Item
  • DSpace@MIT Home
  • Haystack Observatory
  • ALMA Phasing Project
  • View Item
JavaScript is disabled for your browser. Some features of this site may not work without it.

ObsMode2022 Cycle 10 Go/No-Go Report for VLBI Capabilities

Author(s)
Matthews, Lynn D.; Crew, Geoff; Fish, Vincent; Messias, Hugo; Titus, Mike; Krichbaum, Thomas; ... Show more Show less
Thumbnail
DownloadOct2022Report-FINAL.pdf (4.725Mb)
Metadata
Show full item record
Abstract
We present here a report on the Very Long Baseline Interferometry (VLBI) development efforts under consideration at ALMA as new offerings in Cycle 10. These activities are being carried out under the ALMA North America Development Project known as the ALMA Phasing Project Phase 3 (APP3). The two VLBI priorities previously identified for Cycle 10 by the ObsMode process are: (1) spectral line VLBI with flexible tuning; (2) panchromatic VLBI for spectral line and continuum (Bands 1, 3, 6 and 7, with provisions for extension to any other band). This document provides an overview of the development, testing, and readiness of these capabilities. Some updates on minor development efforts are also provided.
Description
This report was prepared for the formal acceptance of the software required for Cycle 10. Notionally it is ALMA Technical Note #25, but not published (yet) as such.
Date issued
2022-11-04
URI
https://hdl.handle.net/1721.1/165044
Keywords
Radio Astronomy, ALMA Observatory, Very Long Baseline Interferometry

Collections
  • ALMA Phasing Project

Browse

All of DSpaceCommunities & CollectionsBy Issue DateAuthorsTitlesSubjectsThis CollectionBy Issue DateAuthorsTitlesSubjects

My Account

Login

Statistics

OA StatisticsStatistics by CountryStatistics by Department
MIT Libraries
PrivacyPermissionsAccessibilityContact us
MIT
Content created by the MIT Libraries, CC BY-NC unless otherwise noted. Notify us about copyright concerns.