Mapping the Stellar Halo with the H3 Spectroscopic Survey

Charlie Conroy, Ana Bonaca, Phillip Cargile, Benjamin D. Johnson, Nelson Caldwell, Rohan P. Naidu, Dennis Zaritsky, Daniel Fabricant, Sean Moran, Jaehyon Rhee, Andrew Szentgyorgyi, Perry Berlind, Michael L. Calkins, Shianne Kattner, Chun Ly

Research output: Contribution to journalArticle

Abstract

Modern theories of galaxy formation predict that the Galactic stellar halo was hierarchically assembled from the accretion and disruption of smaller systems. This hierarchical assembly is expected to produce a high degree of structure in the combined phase and chemistry space; this structure should provide a relatively direct probe of the accretion history of our Galaxy. Revealing this structure requires precise 3D positions (including distances), 3D velocities, and chemistry for large samples of stars. The Gaia satellite is delivering proper motions and parallaxes for >1 billion stars to G ≈ 20. However, radial velocities and metallicities will only be available to G ≈ 15, which is insufficient to probe the outer stellar halo (⪆10 kpc). Moreover, parallaxes will not be precise enough to deliver high-quality distances for stars beyond ∼10 kpc. Identifying accreted systems throughout the stellar halo therefore requires a large ground-based spectroscopic survey to complement Gaia. Here we provide an overview of the H3 Stellar Spectroscopic Survey, which will deliver precise stellar parameters and spectrophotometric distances for ≈200,000 stars to r = 18. Spectra are obtained with the Hectochelle instrument at the MMT, which is configured for the H3 Survey to deliver resolution R ≈ 23,000 spectra covering the wavelength range 5150-5300 Å. The survey is optimized for stellar halo science and therefore focuses on high Galactic latitude fields (), sparsely sampling 15,000 sq. degrees. Targets are selected on the basis of Gaia parallaxes, enabling very efficient selection of bona fide halo stars. The survey began in the fall of 2017 and has collected 88,000 spectra to-date. All of the data, including the derived stellar parameters, will eventually be made publicly available via the survey website: h3survey.rc.fas.harvard.edu.

Original languageEnglish (US)
Article number107
JournalAstrophysical Journal
Volume883
Issue number1
DOIs
StatePublished - Sep 20 2019

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halos
stars
accretion
probe
chemistry
probes
proper motion
galactic evolution
radial velocity
complement
metallicity
coverings
assembly
sampling
histories
galaxies
wavelength
history
wavelengths
parameter

Keywords

  • Galaxy: halo
  • Galaxy: kinematics and dynamics

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Conroy, C., Bonaca, A., Cargile, P., Johnson, B. D., Caldwell, N., Naidu, R. P., ... Ly, C. (2019). Mapping the Stellar Halo with the H3 Spectroscopic Survey. Astrophysical Journal, 883(1), [107]. https://doi.org/10.3847/1538-4357/ab38b8

Mapping the Stellar Halo with the H3 Spectroscopic Survey. / Conroy, Charlie; Bonaca, Ana; Cargile, Phillip; Johnson, Benjamin D.; Caldwell, Nelson; Naidu, Rohan P.; Zaritsky, Dennis; Fabricant, Daniel; Moran, Sean; Rhee, Jaehyon; Szentgyorgyi, Andrew; Berlind, Perry; Calkins, Michael L.; Kattner, Shianne; Ly, Chun.

In: Astrophysical Journal, Vol. 883, No. 1, 107, 20.09.2019.

Research output: Contribution to journalArticle

Conroy, C, Bonaca, A, Cargile, P, Johnson, BD, Caldwell, N, Naidu, RP, Zaritsky, D, Fabricant, D, Moran, S, Rhee, J, Szentgyorgyi, A, Berlind, P, Calkins, ML, Kattner, S & Ly, C 2019, 'Mapping the Stellar Halo with the H3 Spectroscopic Survey', Astrophysical Journal, vol. 883, no. 1, 107. https://doi.org/10.3847/1538-4357/ab38b8
Conroy C, Bonaca A, Cargile P, Johnson BD, Caldwell N, Naidu RP et al. Mapping the Stellar Halo with the H3 Spectroscopic Survey. Astrophysical Journal. 2019 Sep 20;883(1). 107. https://doi.org/10.3847/1538-4357/ab38b8
Conroy, Charlie ; Bonaca, Ana ; Cargile, Phillip ; Johnson, Benjamin D. ; Caldwell, Nelson ; Naidu, Rohan P. ; Zaritsky, Dennis ; Fabricant, Daniel ; Moran, Sean ; Rhee, Jaehyon ; Szentgyorgyi, Andrew ; Berlind, Perry ; Calkins, Michael L. ; Kattner, Shianne ; Ly, Chun. / Mapping the Stellar Halo with the H3 Spectroscopic Survey. In: Astrophysical Journal. 2019 ; Vol. 883, No. 1.
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abstract = "Modern theories of galaxy formation predict that the Galactic stellar halo was hierarchically assembled from the accretion and disruption of smaller systems. This hierarchical assembly is expected to produce a high degree of structure in the combined phase and chemistry space; this structure should provide a relatively direct probe of the accretion history of our Galaxy. Revealing this structure requires precise 3D positions (including distances), 3D velocities, and chemistry for large samples of stars. The Gaia satellite is delivering proper motions and parallaxes for >1 billion stars to G ≈ 20. However, radial velocities and metallicities will only be available to G ≈ 15, which is insufficient to probe the outer stellar halo (⪆10 kpc). Moreover, parallaxes will not be precise enough to deliver high-quality distances for stars beyond ∼10 kpc. Identifying accreted systems throughout the stellar halo therefore requires a large ground-based spectroscopic survey to complement Gaia. Here we provide an overview of the H3 Stellar Spectroscopic Survey, which will deliver precise stellar parameters and spectrophotometric distances for ≈200,000 stars to r = 18. Spectra are obtained with the Hectochelle instrument at the MMT, which is configured for the H3 Survey to deliver resolution R ≈ 23,000 spectra covering the wavelength range 5150-5300 {\AA}. The survey is optimized for stellar halo science and therefore focuses on high Galactic latitude fields (), sparsely sampling 15,000 sq. degrees. Targets are selected on the basis of Gaia parallaxes, enabling very efficient selection of bona fide halo stars. The survey began in the fall of 2017 and has collected 88,000 spectra to-date. All of the data, including the derived stellar parameters, will eventually be made publicly available via the survey website: h3survey.rc.fas.harvard.edu.",
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