A measurement of the contamination in [O III] λ5007 surveys of intracluster stars and the surface density of z = 3.13 Lyα galaxies

Robin Ciardullo, John J. Feldmeier, Kara Krelove, George H. Jacoby, Caryl Gronwall

Research output: Contribution to journalArticle

31 Citations (Scopus)

Abstract

We present two pieces of evidence supporting the hypothesis that the bright [O III] λ5007 sources found in Virgo's intracluster space are intracluster planetary nebulae rather than [O II] λ3727 galaxies at z ∼ 0.35 or Lyα sources at z ∼ 3.13. First, we confirm the nature of five "overluminous" [O III] sources that are postulated to lie in front of M87: by examining the composite spectrum of these objects, we show that the weaker [O III] line at λ4959 is definitely present at a strength ∼1/3 that of [O III] λ5007. The ratio demonstrates that, at most, only one of the five objects is a background galaxy. We then estimate the surface density of background emission-line objects by conducting a wide-field (0.13 deg2) search at λ5019 for faint emission-line sources in a "blank field" located well away from any galaxy or cluster. We show that the density of blank-field emission-line sources is significantly lower than the density of sources detected between the galaxies of Virgo but in good agreement with the density of Lyα galaxies found by Hu, Cowie, & McMahon. The implication is that background galaxies account for only ∼20% of the planetary nebula candidates in Virgo's intracluster fields.

Original languageEnglish (US)
Pages (from-to)784-793
Number of pages10
JournalAstrophysical Journal
Volume566
Issue number2 I
DOIs
StatePublished - Feb 20 2002

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contamination
galaxies
stars
blanks
planetary nebulae
field emission
conduction
composite materials
estimates
line source

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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title = "A measurement of the contamination in [O III] λ5007 surveys of intracluster stars and the surface density of z = 3.13 Lyα galaxies",
abstract = "We present two pieces of evidence supporting the hypothesis that the bright [O III] λ5007 sources found in Virgo's intracluster space are intracluster planetary nebulae rather than [O II] λ3727 galaxies at z ∼ 0.35 or Lyα sources at z ∼ 3.13. First, we confirm the nature of five {"}overluminous{"} [O III] sources that are postulated to lie in front of M87: by examining the composite spectrum of these objects, we show that the weaker [O III] line at λ4959 is definitely present at a strength ∼1/3 that of [O III] λ5007. The ratio demonstrates that, at most, only one of the five objects is a background galaxy. We then estimate the surface density of background emission-line objects by conducting a wide-field (0.13 deg2) search at λ5019 for faint emission-line sources in a {"}blank field{"} located well away from any galaxy or cluster. We show that the density of blank-field emission-line sources is significantly lower than the density of sources detected between the galaxies of Virgo but in good agreement with the density of Lyα galaxies found by Hu, Cowie, & McMahon. The implication is that background galaxies account for only ∼20{\%} of the planetary nebula candidates in Virgo's intracluster fields.",
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A measurement of the contamination in [O III] λ5007 surveys of intracluster stars and the surface density of z = 3.13 Lyα galaxies. / Ciardullo, Robin; Feldmeier, John J.; Krelove, Kara; Jacoby, George H.; Gronwall, Caryl.

In: Astrophysical Journal, Vol. 566, No. 2 I, 20.02.2002, p. 784-793.

Research output: Contribution to journalArticle

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T1 - A measurement of the contamination in [O III] λ5007 surveys of intracluster stars and the surface density of z = 3.13 Lyα galaxies

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AU - Gronwall, Caryl

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AB - We present two pieces of evidence supporting the hypothesis that the bright [O III] λ5007 sources found in Virgo's intracluster space are intracluster planetary nebulae rather than [O II] λ3727 galaxies at z ∼ 0.35 or Lyα sources at z ∼ 3.13. First, we confirm the nature of five "overluminous" [O III] sources that are postulated to lie in front of M87: by examining the composite spectrum of these objects, we show that the weaker [O III] line at λ4959 is definitely present at a strength ∼1/3 that of [O III] λ5007. The ratio demonstrates that, at most, only one of the five objects is a background galaxy. We then estimate the surface density of background emission-line objects by conducting a wide-field (0.13 deg2) search at λ5019 for faint emission-line sources in a "blank field" located well away from any galaxy or cluster. We show that the density of blank-field emission-line sources is significantly lower than the density of sources detected between the galaxies of Virgo but in good agreement with the density of Lyα galaxies found by Hu, Cowie, & McMahon. The implication is that background galaxies account for only ∼20% of the planetary nebula candidates in Virgo's intracluster fields.

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