==========================================================================
VIII/66 IRAM observations in pre-star forming regions (Falgarone+ 1998-2001)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
list.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VIII/66
==========================================================================
drwxr-xr-x 112 cats archive 4096 Nov 7 15:27 [Up]
drwxr-xr-x 3 cats archive 4096 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 463 Dec 19 2022 .message
-r--r--r-- 1 cats archive 7070 Aug 4 2001 ReadMe
-rw-r--r-- 1 cats archive 306 Dec 5 2014 +footg5.gif
-rw-r--r-- 1 cats archive 2301 Dec 5 2014 +footg8.gif
drwxr-xr-x 2 cats archive 4096 Sep 1 2006 fits
-r--r--r-- 1 cats archive 6920 Aug 4 2001 list.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :VIII/66 IRAM observations in pre-star forming regions (Falgarone+ 1998-2001)
================================================================================
IRAM key-project ``Small-scale structure of pre-star forming regions''
I. Observational results
Falgarone E., Panis J.-F., Heithausen A., Perault M., Stutzki J.,
Puget J.-L., Bensch F.
<Astron. Astrophys. 331, 669 (1998)>
=1998A&A...331..669F
III. Influence of and correction for the error beam pick-up
Bensch F., Panis J.-F., Stutzki J., Heithausen A., Falgarone E.
<Astron. Astrophys. 365, 275 (2001)>
=2001A&A...365..275B
================================================================================
ADC_Keywords: Radio lines ; Carbon monoxide
Keywords: turbulence - methods: data analysis - techniques: miscellaneous -
radio lines: ISM - line: profiles - ISM: kinematics and dynamics -
ISM: clouds - ISM: molecules
Description:
The goal of the IRAM key-project ``Small-scale structure of pre-star
forming regions'' is to map three nearby (d 150pc), quiescent
molecular clouds with a high angular and spectral resolution to study
the molecular cloud structure down to the smallest linear scales
currently accessible by single dish radio telescopes.
The key-project maps are available as data cubes (velocity, right
ascension or galactic longitude, declination or galactic latitude)
available as a set of 40 FITS files stored in the fits subdirectory;
a summary of these 40 files is contained in the file "list.dat". The
observations reported concern the molecular clouds L1512, L134A, and
MCLD 123.5+24.9 in the Polaris Flare.
The released data set of the IRAM key-project (Falgarone et al.,
1998A&A...331..669F) are error beam corrected using the beam pattern
parameters published by Garcia-Burillo, Guelin and Cernicharo
(1993A&A...274..123G) and observations made with the KOSMA 3m
telescope. Bensch et al. (2001A&A...365..275B) present the corrected
maps using the 30m beam pattern recently published by Greve et al.
(1998A&AS..133..271G). They estimate the accuracy of the maps of the
key-project as 10-15% for the CO(2-1), except for two ^13^CO(2-1) maps
of the MCLD 123.5+24.9/Polaris Flare and of L1512 where the
uncertainties are estimated to 22% and 18% respectively. For the
CO(1-0) data, the overall accuracy is 11%.