IFU observations of the core of Abell 2218

N. Cardiel; S. F. Sánchez; M. A. W. Verheijen; S. Pedraz; G. Covone

doi:10.1017/S1743921307009118

IFU observations of the core of Abell 2218

N. Cardiel, S. F. Sánchez, M. A. W. Verheijen, S. Pedraz, G. Covone

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

Abstract

We present a study of the morphologies and stellar content of the galaxies in the central ∼ 74”×64” region of the galaxy cluster Abell 2218 (see Fig. 1). The spectroscopic data were obtained with the integral field unit PMAS (Roth et al. 2005) in the PPAK mode (Verheijen et al. 2004; Kelz et al. 2006), at the 3.5 m telescope of the Calar Alto Observatory. The covered wavelength range was 4650–8000 Å, with a spectral resolution FWHM∼ 10Å. These data were combined with with deep HST/ACS F475W, F555W, F625W and F850LP imaging, and additional data from the literature.

Original language	English
Title of host publication	Stellar Populations as Building Blocks of Galaxies
Publisher	Cambridge University Press
Pages	561-562
Number of pages	2
Volume	241
DOIs	https://doi.org/10.1017/S1743921307009118
Publication status	Published - 1-Aug-2007

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IFU observations of the core of Abell 2218
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@inproceedings{e483c3e1642146049be6aa3c24052506,

title = "IFU observations of the core of Abell 2218",

abstract = "We present a study of the morphologies and stellar content of the galaxies in the central ∼ 74”×64” region of the galaxy cluster Abell 2218 (see Fig. 1). The spectroscopic data were obtained with the integral field unit PMAS (Roth et al. 2005) in the PPAK mode (Verheijen et al. 2004; Kelz et al. 2006), at the 3.5 m telescope of the Calar Alto Observatory. The covered wavelength range was 4650–8000 {\AA}, with a spectral resolution FWHM∼ 10{\AA}. These data were combined with with deep HST/ACS F475W, F555W, F625W and F850LP imaging, and additional data from the literature.",

author = "N. Cardiel and S{\'a}nchez, {S. F.} and Verheijen, {M. A. W.} and S. Pedraz and G. Covone",

note = "Stellar Populations as Building Blocks of Galaxies, Proceedings of IAU Symposium #241. Edited by A. Vazdekis and R. F. Peletier. Cambridge: Cambridge University Press, 2007, pp.561-562",

year = "2007",

month = aug,

day = "1",

doi = "10.1017/S1743921307009118",

language = "English",

volume = "241",

pages = "561--562",

booktitle = "Stellar Populations as Building Blocks of Galaxies",

publisher = "Cambridge University Press",

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TY - GEN

T1 - IFU observations of the core of Abell 2218

AU - Cardiel, N.

AU - Sánchez, S. F.

AU - Verheijen, M. A. W.

AU - Pedraz, S.

AU - Covone, G.

N1 - Stellar Populations as Building Blocks of Galaxies, Proceedings of IAU Symposium #241. Edited by A. Vazdekis and R. F. Peletier. Cambridge: Cambridge University Press, 2007, pp.561-562

PY - 2007/8/1

Y1 - 2007/8/1

N2 - We present a study of the morphologies and stellar content of the galaxies in the central ∼ 74”×64” region of the galaxy cluster Abell 2218 (see Fig. 1). The spectroscopic data were obtained with the integral field unit PMAS (Roth et al. 2005) in the PPAK mode (Verheijen et al. 2004; Kelz et al. 2006), at the 3.5 m telescope of the Calar Alto Observatory. The covered wavelength range was 4650–8000 Å, with a spectral resolution FWHM∼ 10Å. These data were combined with with deep HST/ACS F475W, F555W, F625W and F850LP imaging, and additional data from the literature.

AB - We present a study of the morphologies and stellar content of the galaxies in the central ∼ 74”×64” region of the galaxy cluster Abell 2218 (see Fig. 1). The spectroscopic data were obtained with the integral field unit PMAS (Roth et al. 2005) in the PPAK mode (Verheijen et al. 2004; Kelz et al. 2006), at the 3.5 m telescope of the Calar Alto Observatory. The covered wavelength range was 4650–8000 Å, with a spectral resolution FWHM∼ 10Å. These data were combined with with deep HST/ACS F475W, F555W, F625W and F850LP imaging, and additional data from the literature.

U2 - 10.1017/S1743921307009118

DO - 10.1017/S1743921307009118

M3 - Conference contribution

VL - 241

SP - 561

EP - 562

BT - Stellar Populations as Building Blocks of Galaxies

PB - Cambridge University Press

ER -

IFU observations of the core of Abell 2218

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