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J/A+A/531/L2      Images of Vega at 1.3mm                     (Pietu+, 2011)

High-sensitivity search for clumps in the Vega Kuiper-belt. New PdBI 1.3 mm observations. Pietu V., Di Folco E., Guilloteau S., Gueth F., Cox P. <Astron. Astrophys. 531, L2 (2011)> =2011A&A...531L...2P
ADC_Keywords: Stars, variable ; Photometry, millimetric/submm Keywords: radio continuum: stars - stars: individual: Vega - circumstellar matter - method: observational - instrumentation: interferometers Abstract: Previous studies have found that Vega is surrounded by an extended debris disc that is very smooth in the far infrared, but displays possible clumpiness at 850um and dust emission peaks at 1.3mm. We reobserved Vega at 1.3mm with PdBI to constrain its circumstellar dust distribution. Description: Our observations of a three-field mosaic have a factor of two higher sensitivity than previous observations. Objects: -------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------- 18 36 56.2 +38 46 59 Vega = * alf Lyr -------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file list.dat 90 2 FITS images list fig1.fits 2880 94 Natural weighting 1.3mm continuum image fig2.fits 2880 94 1.3mm continuum image obtained with (u,v) taper
Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 9 A9 --- FileName Name of the fits image (256x256pix, 0.25aércsec/pix) 12- 90 A79 --- Title Title of the image
Acknowledgements: Vincent Pietu, pietu(at)iram.fr
(End) Patricia Vannier [CDS] 01-Jun-2011
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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