Characterisation of the MALT90 Survey and the Mopra Telescope at 90 GHz

Autor: Timea Csengeri, Jill Rathborne, Steven N. Longmore, Sadia Hoq, M. Wienen, Andrew Walsh, Fabrice Herpin, Tui Britton, Maxim Voronkov, Shari Breen, Jonathan B. Foster, Tracey Hill, Christopher H. Jordan, K. J. Brooks, Christopher Claysmith, Patricio Sanhueza, Joshua L. Mascoop, Ana Duarte-Cabral, Peter J. Barnes, Balthasar T. Indermuehle, Maria Cunningham, J. S. Whitaker, James Urquhart, Yanett Contreras, James M. Jackson, João Alves
Přispěvatelé: FORMATION STELLAIRE 2013, Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Observatoire aquitain des sciences de l'univers (OASU), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)
Rok vydání: 2013
Předmět:
Zdroj: Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia, Cambridge University Press (CUP), 2013, 30, pp.id.e038. ⟨10.1017/pasa.2013.18⟩
ISSN: 1448-6083
1323-3580
Popis: We characterize the Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey and the Mopra telescope at 90 GHz. We combine repeated position-switched observations of the source G300.968+01.145 with a map of the same source in order to estimate the pointing reliability of the position-switched observations and, by extension, the MALT90 survey; we estimate our pointing uncertainty to be 8 arcseconds. We model the two strongest sources of systematic gain variability as functions of elevation and time-of-day and quantify the remaining absolute flux uncertainty. Corrections based on these two variables reduce the scatter in repeated observations from 12-25% down to 10-17%. We find no evidence for intrinsic source variability in G300.968+01.145. For certain applications, the corrections described herein will be integral for improving the absolute flux calibration of MALT90 maps and other observations using the Mopra telescope at 90 GHz.
Comment: Corrected Figure 5
Databáze: OpenAIRE