Calibrated and completeness-corrected optical stellar density maps of the Northern Galactic Plane

H. J. Farnhill, J. E. Drew, G. Barentsen, E. A. González-Solares

Research output: Contribution to journalArticlepeer-review

4 Citations (Scopus)
123 Downloads (Pure)

Abstract

Following on from the second release of calibrated photometry from IPHAS, the INT/WFC Photometric Hα Survey of the Northern Galactic Plane, we present incompleteness-corrected stellar density maps in the r and i photometric bands. These have been computed to a range of limiting magnitudes reaching to 20th magnitude in r and 19th in i (Vega system), and with different angular resolutions – the highest resolution available being 1 arcmin2. The maps obtained cover 94 per cent of the 1800 square degree IPHAS footprint, spanning the Galactic latitude range, −5◦ < b < +5◦, north of the celestial equator. The corrections for incompleteness, due to confusion and sensitivity loss at the faint limit, have been deduced by the method of artificial source injection. The presentation of this method is preceded by a discussion of other more approximate methods of determining completeness. Our method takes full account of position-dependent seeing and source ellipticity in the survey data base. The application of the star counts to testing reddened Galactic disc models is previewed by a comparison with predicted counts along three constant-longitude cuts at 30◦, 90◦ and 175◦: some overprediction of the most heavily reddened 30◦ counts is found, alongside good agreement at 90◦ and 175◦. Key
Original languageEnglish
Pages (from-to)642-665
Number of pages24
JournalMonthly Notices of the Royal Astronomical Society
Volume457
Issue number1
Early online date22 Jan 2016
DOIs
Publication statusPublished - 21 Mar 2016

Keywords

  • astro-ph.GA
  • astro-ph.IM
  • astro-ph.SR
  • Atlases
  • dust, extinction
  • Galaxy: disc
  • Stellar content
  • Galaxy: structure

Fingerprint

Dive into the research topics of 'Calibrated and completeness-corrected optical stellar density maps of the Northern Galactic Plane'. Together they form a unique fingerprint.

Cite this