M100 Band3: Difference between revisions

From CASA Guides
Jump to navigationJump to search
Cvlahaki (talk | contribs)
No edit summary
Cvlahaki (talk | contribs)
No edit summary
Line 8: Line 8:


== ALMA Data Overview ==
== ALMA Data Overview ==
=== 12-m Data ===
=== Morita array (ACA) 7-m Data ===
ALMA Science Verification data at Band 3 was taken for M100 with the ACA on DATES. The observations consisted of an X pointing mosaic centered at RA=, Dec=’’ as shown in Figure 1.
A scheduling block about X hours long was run six times for a total of about 3.5 hours of observing time. The integration time of each visibility is X seconds, and the total on-source time of of each pointing is X minutes.
The names of the six datasets are as follows:
*uid___A002_X5e971a_X124
*uid___A002_X5e971a_X2e7
*uid___A002_X5e9ff1_X3f3
*uid___A002_X5e9ff1_X5b3
*uid___A002_X60b415_X44
*uid___A002_X62f759_X4eb
DETAILS OF OBSERVATIONS TO GO HERE.
=== Single-Dish Data ===
=== Acknowledgements and Data Usage ===
'''Using the data for publication:''' The following statement should be included in the acknowledgment of papers using the datasets listed above: “This paper makes use of the following ALMA data:
ADS/JAO.ALMA#2011.0.00004.SV . ALMA is a partnership of ESO (representing
its member states), NSF (USA) and NINS (Japan), together with NRC
(Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of
Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ."
We thank the following people for suggesting M100 for ALMA Science Verification:


== Obtaining the Data ==
== Obtaining the Data ==

Revision as of 18:01, 29 August 2013

M100 Introduction Page.

Science Target Overview

M100 (NGC 4321; RA 12h 22m 54.8s, Dec +15 49' 19") is a nearby (~16 Mpc) 'grand-design' barred spiral galaxy in the Virgo cluster. It has long spiral arms dominating its optical disk and an abundance of molecular gas in its center. It has a relatively face-on inclination of ~30 degrees.

In the 1990s, M100 was mapped at an angular resolution of 6" using the Berkeley-Illinois-Maryland Association (BIMA) millimeter interferometer as part of the BIMA SONG survey (Regan et al. 2001; Helfer et al. 2003; Sheth et al. 2002). Using the Nobeyama mm-wave Array (NMA), the central 1' was mapped by Sakamoto et al. (1995, 1999) at 2.5" resolution. Its nucleus has also been mapped in CO using the IRAM interferometer (Garcia-Burillo et al. 1998).

ALMA Data Overview

12-m Data

Morita array (ACA) 7-m Data

ALMA Science Verification data at Band 3 was taken for M100 with the ACA on DATES. The observations consisted of an X pointing mosaic centered at RA=, Dec=’’ as shown in Figure 1.

A scheduling block about X hours long was run six times for a total of about 3.5 hours of observing time. The integration time of each visibility is X seconds, and the total on-source time of of each pointing is X minutes.

The names of the six datasets are as follows:

  • uid___A002_X5e971a_X124
  • uid___A002_X5e971a_X2e7
  • uid___A002_X5e9ff1_X3f3
  • uid___A002_X5e9ff1_X5b3
  • uid___A002_X60b415_X44
  • uid___A002_X62f759_X4eb

DETAILS OF OBSERVATIONS TO GO HERE.

Single-Dish Data

Acknowledgements and Data Usage

Using the data for publication: The following statement should be included in the acknowledgment of papers using the datasets listed above: “This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00004.SV . ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ."

We thank the following people for suggesting M100 for ALMA Science Verification:

Obtaining the Data

To download all the data, follow one of the next links:

North America

Europe

East Asia

M100 Data Combination Tutorial

How to Use A CASA Guide

For tips on using CASA and ways CASA can be run, see EVLA_Spectral_Line_Calibration_IRC+10216#How_to_Use_This_casaguide page.

To learn how to extract executable Python scripts from the tutorial, see Extracting_scripts_from_these_tutorials.

Within the guides:

# In CASA
Regions of this color are CASA commands (or definitions) that need to be cut and 
pasted in sequence. Wait until one command is finished before pasting another. 
Tabs matter in python, make sure that commands that span more than one line and 
"for" loops keep their spacing. Sometimes (especially "for" loops) you may need to 
explicitly hit enter twice to get the command going.
Information in this color shows excerpts from the CASA Logger output
This color shows you background information about the data or other types of reference material