Spectrophotometrically identified stars in the pears-n and pears-s fields

N. Pirzkal, A. J. Burgasser, S. Malhotra, B. W. Holwerda, K. C. Sahu, J. E. Rhoads, C. Xu, J. J. Bochanski, J. R. Walsh, Rogier Windhorst, N. P. Hathi, S. H. Cohen

Research output: Contribution to journalArticle

26 Citations (Scopus)

Abstract

Deep ACS slitless grism observations and identification of stellar sources are presented within the Great Observatories Origins Deep Survey North and South fields which were obtained in the Probing Evolution And Reionization Spectroscopically (PEARS) program. It is demonstrated that even low-resolution spectra can be a very powerful means of identifying stars in the field, especially low-mass stars with stellar types M0 and later. The PEARS fields lay within the larger GOODS fields, and we used new, deeper images to further refine the selection of stars in the PEARS field, down to a magnitude of z850 = 25 using a newly developed stellarity parameter. The total number of stars with reliable spectroscopic and morphological identification was 95 and 108 in the north and south fields, respectively. The sample of spectroscopically identified stars allows constraints to be set on the thickness of the Galactic thin disk as well as contributions from a thick disk and a halo component. We derive a thin disk scale height, as traced by the population of M4-M9 dwarfs along two independent lines of sight, of hthin = 370+60 -65 pc. When including the more massive M0-M4 dwarf population, we derive hthin= 300 ± 70 pc. In both cases, we observe that we must include a combination of thick and halo components in our models in order to account for the observed numbers of faint dwarfs. The required thick disk scale height is typically hthick = 1000 pc and the acceptable relative stellar densities of the thin disk to thick disk and the thin disk to halo components are in the range of 0.00025 < fhalo < 0.0005 and 0.05 < fhalo < 0.08 and are somewhat dependent on whether the more massive M0-M4 dwarfs are included in our sample.

Original languageEnglish (US)
Pages (from-to)1591-1603
Number of pages13
JournalAstrophysical Journal
Volume695
Issue number2
DOIs
StatePublished - Apr 20 2009

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stars
halos
scale height
observatory
line of sight
observatories
programme
goods
parameter

Keywords

  • Color figures
  • Disk
  • Galaxy
  • Galaxy
  • Galaxy
  • Galaxy
  • Halo
  • Late-Type online-only material
  • Stars
  • Stellar content
  • Structure

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Pirzkal, N., Burgasser, A. J., Malhotra, S., Holwerda, B. W., Sahu, K. C., Rhoads, J. E., ... Cohen, S. H. (2009). Spectrophotometrically identified stars in the pears-n and pears-s fields. Astrophysical Journal, 695(2), 1591-1603. https://doi.org/10.1088/0004-637X/695/2/1591

Spectrophotometrically identified stars in the pears-n and pears-s fields. / Pirzkal, N.; Burgasser, A. J.; Malhotra, S.; Holwerda, B. W.; Sahu, K. C.; Rhoads, J. E.; Xu, C.; Bochanski, J. J.; Walsh, J. R.; Windhorst, Rogier; Hathi, N. P.; Cohen, S. H.

In: Astrophysical Journal, Vol. 695, No. 2, 20.04.2009, p. 1591-1603.

Research output: Contribution to journalArticle

Pirzkal, N, Burgasser, AJ, Malhotra, S, Holwerda, BW, Sahu, KC, Rhoads, JE, Xu, C, Bochanski, JJ, Walsh, JR, Windhorst, R, Hathi, NP & Cohen, SH 2009, 'Spectrophotometrically identified stars in the pears-n and pears-s fields', Astrophysical Journal, vol. 695, no. 2, pp. 1591-1603. https://doi.org/10.1088/0004-637X/695/2/1591
Pirzkal N, Burgasser AJ, Malhotra S, Holwerda BW, Sahu KC, Rhoads JE et al. Spectrophotometrically identified stars in the pears-n and pears-s fields. Astrophysical Journal. 2009 Apr 20;695(2):1591-1603. https://doi.org/10.1088/0004-637X/695/2/1591
Pirzkal, N. ; Burgasser, A. J. ; Malhotra, S. ; Holwerda, B. W. ; Sahu, K. C. ; Rhoads, J. E. ; Xu, C. ; Bochanski, J. J. ; Walsh, J. R. ; Windhorst, Rogier ; Hathi, N. P. ; Cohen, S. H. / Spectrophotometrically identified stars in the pears-n and pears-s fields. In: Astrophysical Journal. 2009 ; Vol. 695, No. 2. pp. 1591-1603.
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