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VIII/82    2nd Epoch Molonglo Galactic Plane Survey (MGPS-2)   (Murphy+, 2007)

The 2nd Epoch Molonglo Galactic Plane Survey (MGPS-2), Version 15 August 2007. Murphy T., Mauch T., Green A., Hunstead R.W., Piestrzynska B., Kels A.P., Sztajer P. <Mon. Not. R. Astron. Soc. 382, 382 (2007)> =2007MNRAS.382..382M
ADC_Keywords: Galactic plane ; Radio sources ; Surveys ; Radio continuum Keywords: catalogues - surveys - methods: data analysis - radio continuum: ISM - Galaxy: general Description: The MGPS-2 (second epoch Molonglo Galactic Plane Survey) was carried out with the Molonglo Observatory Synthesis Telescope at a frequency of 843MHz and with a restoring beam of 45"x45"csd|δ|, making it he highest resolution large scale radio survey of the southern Galactic plane. It covers the range |b|<10° and 245<l<365°; it is the Galactic counterpart to the SUMSS (Cat. VIII/81) which covers the southern sky (δ←30°, |b|>10°). This catalogue (15-Aug-2007) consists of 48850 compact sources, made by fitting elliptical gaussians in the MGPS-2 mosaics to a limiting peak brightness of 10mJy/beam. We used a custom method (described in the associated publication) to remove extended sources from the catalogue. Positions in the catalogue are accurate to 1-2". See http://www.astrop.physics.usyd.edu.au/mosaics for access to the mosaic images. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file mgpscat.dat 179 48850 The MGPS-2 Catalog, Version 1.0 (2007-08-15)
See also: VIII/78 : Sydney University Molonglo Sky Survey (SUMSS) (Mauch+ 2006) http://www.physics.usyd.edu.au/ioa/Main/MGPS2 : the MGPS-2 Home Page Byte-by-byte Description of file: mgpscat.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [MGPS] 6- 19 A14 --- MGPS MGPS designation (JHHMMSS-DDMMSS) 21- 31 F11.7 deg GLON Galactic longitude (degrees) 33- 43 F11.7 deg GLAT Galactic latitude (degrees) 45- 46 I2 h RAh Right Ascension J2000 (hours) 48- 49 I2 min RAm Right Ascension J2000 (minutes) 51- 55 F5.2 s RAs Right Ascension J2000 (seconds) 58 A1 --- DE- Declination J2000 (sign) 59- 60 I2 deg DEd Declination J2000 (degrees) 62- 63 I2 arcmin DEm Declination J2000 (minutes) 65- 69 F5.2 arcsec DEs Declination J2000 (seconds) 71- 74 F4.1 arcsec e_RAs rms uncertainty in Right Ascension (1) 76- 79 F4.1 arcsec e_DEs rms uncertainty in Declination (1) 83- 89 F7.1 mJy Sp Peak brightness at 843MHz (in mJy/beam) 91- 96 F6.1 mJy e_Sp Uncertainty on Sp 99-106 F8.1 mJy St Total flux density at 843MHz 108-113 F6.1 mJy e_St Uncertainty on St 116-121 F6.1 arcsec MajAxis Fitted major axis 123-127 F5.1 arcsec MinAxis Fitted minor axis 129-133 F5.1 deg PA Fitted major axis position angle (N to E) 136-141 F6.1 arcsec dMajAxis Fitted major axis after deconvolution (2) 143-147 F5.1 arcsec dMinAxis Fitted minor axis after deconvolution (2) 149-153 F5.1 deg dPA ? Fitted major axis position angle after deconvolution 156-163 A8 --- Mosaic Mosaic in which the source appears (3) 165 I1 --- Nm Number of mosaics with the source (4) 167-172 F6.1 pix Xpos Position of the source on quoted mosaic (4) 174-179 F6.1 pix Ypos Position of the source on quoted mosaic (4)
Note (1): Positional uncertainties are calculated from the quadratic sum of the MOST calibration using Equations (1) and (2) of the paper. Note (2): If the fitted major axis size exceeds the beam size by more than 2.33σ(θM), the major axis size after deconvolution from the MOST beam is given in arcseconds. Note (3): The naming scheme for MGPS-2 mosaics is JHHMMMDD indicating the J2000 RA and Dec of the mosaic centre. The original mosaics are available online at http://www.astrop.physics.usyd.edu.au/mosaics In the case of duplicate matches the mosaic name quoted is that used for the fit which is chosen to be included in the catalogue. Note (4): When the source appears in more than one image, the source parameters are those of the most reliable fit.
Nomenclature Notes: MGPS-2 sources should be referred by their truncated position MGPS JHHMMSS-DDMMSS Acknowledgements: Tara Murphy, tara(at)physics.usyd.edu.au
(End) Patricia Vannier [CDS] 17-Aug-2007
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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