J/MNRAS/429/3330    AMI Galactic Plane Survey at 16GHz. I.   (Perrott+, 2013)

AMI Galactic Plane Survey at 16GHz: I. Observing, mapping and source extraction. Perrott Y.C., Scaife A.M.M., Green D.A., Davies M. L., Franzen T.M.O., Grainge K.J.B., Hobson M.P., Hurley-Walker N., Lasenby A.N., Olamaie M., Pooley G.G., Rodriguez-Gonzalez C., Rumsey C., Saunders R.D.E., Schammel M.P., Scott P.F., Shimwell T.W., Titterington D.J., Waldram E.M. <Mon. Not. R. Astron. Soc. 429, 3330 (2013)> =2013MNRAS.429.3330P 2013MNRAS.429.3330P
ADC_Keywords: Radio sources ; Surveys ; Radio continuum; Galactic plane Keywords: catalogues - surveys - ISM: general - Galaxy: general - radio continuum: general Description: The AMI Galactic Plane survey is being made with the Arcminute Microkelvin Imager (AMI) Small Array at 15.7GHz and with resolution of approximately 3arcmin. This is the first data release, covering ∼868deg2 of the Northern Galactic plane between |b|~±5° and above δ=40° with a noise level of ∼3mJy/beam away from bright sources. The source catalogue contains a total of 3503 sources. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catdr1.dat 180 3503 AMIGPS source list of 3503 sources -------------------------------------------------------------------------------- See also: http://www.mrao.cam.ac.uk/surveys/AMIGPS/ : AMIGPS Home Page Byte-by-byte Description of file: catdr1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- --- [AMIGPS] 8- 21 A14 --- AMIGPS AMIGPS source designation, JHHMMSS+DDMMSS 28- 29 I2 h RAh Right Ascension J2000 (peak) 31- 32 I2 min RAm Right Ascension J2000 (peak) 34- 38 F5.2 s RAs Right Ascension J2000 (peak) 42 A1 --- DE- Declination sign J2000 (peak) 43- 44 I2 deg DEd Declination J2000 (peak) 46- 47 I2 arcmin DEm Declination J2000 (peak) 49- 52 F4.1 arcsec DEs Declination J2000 (peak) 56- 59 F4.1 arcsec e_RAs Error on Right Ascension J2000 (peak) 63- 66 F4.1 arcsec e_DEs Error on declination J2000 (peak) 70- 76 F7.1 mJy Spk Peak flux density at 15.7GHz 79- 84 F6.1 mJy e_Spk Error on peak flux density 86- 87 I2 h RAIh ? Right Ascension J2000 (centroid) 89- 90 I2 min RAIm ? Right Ascension J2000 (centroid) 92- 96 F5.2 s RAIs ? Right Ascension J2000 (centroid) 100 A1 --- DEI- ? Declination sign J2000 (centroid) 101-102 I2 deg DEId ? Declination J2000 (centroid) 104-105 I2 arcmin DEIm ? Declination J2000 (centroid) 107-110 F4.1 arcsec DEIs ? Declination J2000 (centroid) 113-117 F5.1 arcsec e_RAIs ? Error on Right Ascension J2000 (centroid) 120-124 F5.1 arcsec e_DEIs ? Error on declination J2000 (centroid) 128-135 F8.1 mJy Sint ? Integrated flux density at 15.7GHz 137-143 F7.1 mJy e_Sint ? Error on integrated flux density 146-150 F5.1 arcsec ecrit Critical value of major diameter (1) 152-157 F6.1 arcsec bmaj ? Major axis FWHM after deconvolution 160-164 F5.1 arcsec bmin ? Minor axis FWHM after deconvolution 166-170 F5.1 deg PA ? Position angle of major axis 172-177 F6.2 --- chi2 ? Goodness of fit 180 A1 --- Type [PE-] Source type: Point, Extended, or unclassified (fitting failed) -------------------------------------------------------------------------------- Note (1): the critical major diameter is defined by Equation (2): ecrit=3.0bmaj/sqrt(ρ) (ρ is the signal-to-noise ratio) when larger than 100arcsec. -------------------------------------------------------------------------------- Acknowledgements: Yvette Perrott, ycp21(at)mrao.cam.ac.uk History: * 15-Nov-2012: original version, from MNRAS supporting information * 03-Sep-2013: corrected version of the catalog from Yvette Perrott, with 2 decimals in the RA values.
(End) Yvette Perrott [MRAO], Patricia Vannier [CDS] 03-Sep-2013
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