An overdensity of galaxies at z = 5.9 ± 0.2 in the hubble ultra deep field confirmed using the ACS grism

S. Malhotra, J. E. Rhoads, N. Pirzkal, Z. Haiman, C. Xu, E. Daddi, H. Yan, L. E. Bergeron, J. Wang, H. C. Ferguson, C. Gronwall, A. Koekemoer, M. Kuemmel, L. A. Moustakas, N. Panagia, A. Pasquali, M. Stiavelli, J. Walsh, Rogier Windhorst, S. Di Serego Alighieri

Research output: Contribution to journalArticle

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Abstract

We present grism spectra taken with the Advanced Camera for Surveys (ACS) to identify 29 red sources with (i775 - z850) ≥ 0.9 in the Hubble Ultra Deep Field (HUDF). Of these, 23 are found to be galaxies at redshifts between z = 5.4 and 6.7, identified by the break at 1216 Å due to intergalactic medium (IGM) absorption; two are late-type dwarf stars with red colors; and four are galaxies with colors and spectral shapes similar to dust-reddened or old galaxies at redshifts z ≈ 1 - 2. This constitutes the largest uniform, flux-limited sample of spectroscopically confirmed galaxies at such faint fluxes (z850 ≤ 27.5). Many are also among the most distant spectroscopically confirmed galaxies (at redshifts up to z = 6.7). We find a significant overdensity of galaxies at redshifts z = 5.9 ± 0.2. Nearly two-thirds of the galaxies in our sample (15/23) belong to this peak. Taking into account the selection function and the redshift sensitivity of the survey, we get a conservative overdensity of at least a factor of 2 along the line of sight. The galaxies found in this redshift peak are also localized in the plane of the sky in a nonrandom manner, occupying about half of the ACS chip. Thus the volume overdensity is a factor of 4. The star formation rate derived from detected sources in this overdense region is sufficient to reionize the local IGM.

Original languageEnglish (US)
Pages (from-to)666-679
Number of pages14
JournalAstrophysical Journal
Volume626
Issue number2 I
DOIs
StatePublished - Jun 20 2005

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cameras
galaxies
intergalactic media
dust
color
dwarf stars
star formation rate
line of sight
sky
chips
sensitivity
rate

Keywords

  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: high-redshift
  • Galaxies: luminosity function, mass function
  • Intergalactic medium

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Malhotra, S., Rhoads, J. E., Pirzkal, N., Haiman, Z., Xu, C., Daddi, E., ... Di Serego Alighieri, S. (2005). An overdensity of galaxies at z = 5.9 ± 0.2 in the hubble ultra deep field confirmed using the ACS grism. Astrophysical Journal, 626(2 I), 666-679. https://doi.org/10.1086/430047

An overdensity of galaxies at z = 5.9 ± 0.2 in the hubble ultra deep field confirmed using the ACS grism. / Malhotra, S.; Rhoads, J. E.; Pirzkal, N.; Haiman, Z.; Xu, C.; Daddi, E.; Yan, H.; Bergeron, L. E.; Wang, J.; Ferguson, H. C.; Gronwall, C.; Koekemoer, A.; Kuemmel, M.; Moustakas, L. A.; Panagia, N.; Pasquali, A.; Stiavelli, M.; Walsh, J.; Windhorst, Rogier; Di Serego Alighieri, S.

In: Astrophysical Journal, Vol. 626, No. 2 I, 20.06.2005, p. 666-679.

Research output: Contribution to journalArticle

Malhotra, S, Rhoads, JE, Pirzkal, N, Haiman, Z, Xu, C, Daddi, E, Yan, H, Bergeron, LE, Wang, J, Ferguson, HC, Gronwall, C, Koekemoer, A, Kuemmel, M, Moustakas, LA, Panagia, N, Pasquali, A, Stiavelli, M, Walsh, J, Windhorst, R & Di Serego Alighieri, S 2005, 'An overdensity of galaxies at z = 5.9 ± 0.2 in the hubble ultra deep field confirmed using the ACS grism', Astrophysical Journal, vol. 626, no. 2 I, pp. 666-679. https://doi.org/10.1086/430047
Malhotra, S. ; Rhoads, J. E. ; Pirzkal, N. ; Haiman, Z. ; Xu, C. ; Daddi, E. ; Yan, H. ; Bergeron, L. E. ; Wang, J. ; Ferguson, H. C. ; Gronwall, C. ; Koekemoer, A. ; Kuemmel, M. ; Moustakas, L. A. ; Panagia, N. ; Pasquali, A. ; Stiavelli, M. ; Walsh, J. ; Windhorst, Rogier ; Di Serego Alighieri, S. / An overdensity of galaxies at z = 5.9 ± 0.2 in the hubble ultra deep field confirmed using the ACS grism. In: Astrophysical Journal. 2005 ; Vol. 626, No. 2 I. pp. 666-679.
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AU - Xu, C.

AU - Daddi, E.

AU - Yan, H.

AU - Bergeron, L. E.

AU - Wang, J.

AU - Ferguson, H. C.

AU - Gronwall, C.

AU - Koekemoer, A.

AU - Kuemmel, M.

AU - Moustakas, L. A.

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AU - Pasquali, A.

AU - Stiavelli, M.

AU - Walsh, J.

AU - Windhorst, Rogier

AU - Di Serego Alighieri, S.

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N2 - We present grism spectra taken with the Advanced Camera for Surveys (ACS) to identify 29 red sources with (i775 - z850) ≥ 0.9 in the Hubble Ultra Deep Field (HUDF). Of these, 23 are found to be galaxies at redshifts between z = 5.4 and 6.7, identified by the break at 1216 Å due to intergalactic medium (IGM) absorption; two are late-type dwarf stars with red colors; and four are galaxies with colors and spectral shapes similar to dust-reddened or old galaxies at redshifts z ≈ 1 - 2. This constitutes the largest uniform, flux-limited sample of spectroscopically confirmed galaxies at such faint fluxes (z850 ≤ 27.5). Many are also among the most distant spectroscopically confirmed galaxies (at redshifts up to z = 6.7). We find a significant overdensity of galaxies at redshifts z = 5.9 ± 0.2. Nearly two-thirds of the galaxies in our sample (15/23) belong to this peak. Taking into account the selection function and the redshift sensitivity of the survey, we get a conservative overdensity of at least a factor of 2 along the line of sight. The galaxies found in this redshift peak are also localized in the plane of the sky in a nonrandom manner, occupying about half of the ACS chip. Thus the volume overdensity is a factor of 4. The star formation rate derived from detected sources in this overdense region is sufficient to reionize the local IGM.

AB - We present grism spectra taken with the Advanced Camera for Surveys (ACS) to identify 29 red sources with (i775 - z850) ≥ 0.9 in the Hubble Ultra Deep Field (HUDF). Of these, 23 are found to be galaxies at redshifts between z = 5.4 and 6.7, identified by the break at 1216 Å due to intergalactic medium (IGM) absorption; two are late-type dwarf stars with red colors; and four are galaxies with colors and spectral shapes similar to dust-reddened or old galaxies at redshifts z ≈ 1 - 2. This constitutes the largest uniform, flux-limited sample of spectroscopically confirmed galaxies at such faint fluxes (z850 ≤ 27.5). Many are also among the most distant spectroscopically confirmed galaxies (at redshifts up to z = 6.7). We find a significant overdensity of galaxies at redshifts z = 5.9 ± 0.2. Nearly two-thirds of the galaxies in our sample (15/23) belong to this peak. Taking into account the selection function and the redshift sensitivity of the survey, we get a conservative overdensity of at least a factor of 2 along the line of sight. The galaxies found in this redshift peak are also localized in the plane of the sky in a nonrandom manner, occupying about half of the ACS chip. Thus the volume overdensity is a factor of 4. The star formation rate derived from detected sources in this overdense region is sufficient to reionize the local IGM.

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KW - Galaxies: high-redshift

KW - Galaxies: luminosity function, mass function

KW - Intergalactic medium

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