THE APOGEE RED-CLUMP CATALOG: PRECISE DISTANCES, VELOCITIES, AND HIGH-RESOLUTION ELEMENTAL ABUNDANCES OVER A LARGE AREA OF THE MILKY WAY'S DISK

The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we prese...

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Vydané v:The Astrophysical journal Ročník 790; číslo 2; s. 127 - 21
Hlavní autori: Bovy, Jo, Nidever, David L., Rix, Hans-Walter, Girardi, Léo, Zasowski, Gail, Chojnowski, S. Drew, Holtzman, Jon, Epstein, Courtney, Frinchaboy, Peter M., Hayden, Michael R., Rodrigues, Thaíse S., Majewski, Steven R., Johnson, Jennifer A., Pinsonneault, Marc H., Stello, Dennis, Allende Prieto, Carlos, Andrews, Brett, Basu, Sarbani, Beers, Timothy C., Bizyaev, Dmitry, Burton, Adam, Chaplin, William J., Cunha, Katia, Elsworth, Yvonne, García, Rafael A., García-Herńandez, Domingo A., García Pérez, Ana E., Hearty, Fred R., Hekker, Saskia, Kallinger, Thomas, Kinemuchi, Karen, Koesterke, Lars, Mészáros, Szabolcs, Mosser, Benoît, O'Connell, Robert W., Oravetz, Daniel, Pan, Kaike, Robin, Annie C., Schiavon, Ricardo P., Schneider, Donald P., Schultheis, Mathias, Serenelli, Aldo, Shetrone, Matthew, Silva Aguirre, Victor, Simmons, Audrey, Skrutskie, Michael, Smith, Verne V., Stassun, Keivan, Weinberg, David H., Wilson, John C., Zamora, Olga
Médium: Journal Article
Jazyk:English
Vydavateľské údaje: United States American Astronomical Society 01.08.2014
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ISSN:0004-637X, 1538-4357
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Abstract The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we present a sample of 10,341 likely red-clump stars (RC) from the first two years of APOGEE operations, selected based on their position in color- metallicity-surface-gravity-effective-temperature space using a new method calibrated using stellar evolution models and high-quality asteroseismology data. The narrowness of the RC locus in color-metallicity-luminosity space allows us to assign distances to the stars with an accuracy of 5%-10%. The sample extends to typical distances of about 3 kpc from the Sun, with some stars out to 8 kpc, and spans a volume of approximately 100 kpc super(3) over 5 kpc [lap] R [lap] 14 kpc, |Z| [lap] 2 kpc, and -15[degrees] [lap] Galactocentric azimuth [lap] 30[degrees]. The APOGEE red-clump (APOGEE-RC) catalog contains photometry from the Two Micron All Sky Survey, reddening estimates, distances, line-of-sight velocities, stellar parameters and elemental abundances determined from the high-resolution APOGEE spectra, and matches to major proper motion catalogs. We determine the survey selection function for this data set and discuss how the RC selection samples the underlying stellar populations. We use this sample to limit any azimuthal variations in the median metallicity within the approximately 45[degrees] azimuthal region covered by the current sample to be [< or =, slant]0.02 dex, which is more than an order of magnitude smaller than the radial metallicity gradient. This result constrains coherent non-axisymmetric flows within a few kiloparsecs from the Sun.
AbstractList The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we present a sample of 10,341 likely red-clump stars (RC) from the first two years of APOGEE operations, selected based on their position in color-metallicity-surface-gravity-effective-temperature space using a new method calibrated using stellar evolution models and high-quality asteroseismology data. The narrowness of the RC locus in color-metallicity-luminosity space allows us to assign distances to the stars with an accuracy of 5%-10%. The sample extends to typical distances of about 3 kpc from the Sun, with some stars out to 8 kpc, and spans a volume of approximately 100 kpc{sup 3} over 5 kpc ≲ R ≲ 14 kpc, |Z| ≲ 2 kpc, and –15° ≲ Galactocentric azimuth ≲ 30°. The APOGEE red-clump (APOGEE-RC) catalog contains photometry from the Two Micron All Sky Survey, reddening estimates, distances, line-of-sight velocities, stellar parameters and elemental abundances determined from the high-resolution APOGEE spectra, and matches to major proper motion catalogs. We determine the survey selection function for this data set and discuss how the RC selection samples the underlying stellar populations. We use this sample to limit any azimuthal variations in the median metallicity within the ≈45° azimuthal region covered by the current sample to be ≤0.02 dex, which is more than an order of magnitude smaller than the radial metallicity gradient. This result constrains coherent non-axisymmetric flows within a few kiloparsecs from the Sun.
The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we present a sample of 10,341 likely red-clump stars (RC) from the first two years of APOGEE operations, selected based on their position in color- metallicity-surface-gravity-effective-temperature space using a new method calibrated using stellar evolution models and high-quality asteroseismology data. The narrowness of the RC locus in color-metallicity-luminosity space allows us to assign distances to the stars with an accuracy of 5%-10%. The sample extends to typical distances of about 3 kpc from the Sun, with some stars out to 8 kpc, and spans a volume of approximately 100 kpc super(3) over 5 kpc [lap] R [lap] 14 kpc, |Z| [lap] 2 kpc, and -15[degrees] [lap] Galactocentric azimuth [lap] 30[degrees]. The APOGEE red-clump (APOGEE-RC) catalog contains photometry from the Two Micron All Sky Survey, reddening estimates, distances, line-of-sight velocities, stellar parameters and elemental abundances determined from the high-resolution APOGEE spectra, and matches to major proper motion catalogs. We determine the survey selection function for this data set and discuss how the RC selection samples the underlying stellar populations. We use this sample to limit any azimuthal variations in the median metallicity within the approximately 45[degrees] azimuthal region covered by the current sample to be [< or =, slant]0.02 dex, which is more than an order of magnitude smaller than the radial metallicity gradient. This result constrains coherent non-axisymmetric flows within a few kiloparsecs from the Sun.
The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we present a sample of 10,341 likely red-clump stars (RC) from the first two years of APOGEE operations, selected based on their position in color–metallicity–surface-gravity–effective-temperature space using a new method calibrated using stellar evolution models and high-quality asteroseismology data. The narrowness of the RC locus in color–metallicity–luminosity space allows us to assign distances to the stars with an accuracy of 5%–10%. The sample extends to typical distances of about 3 kpc from the Sun, with some stars out to 8 kpc, and spans a volume of approximately 100 kpc3 over 5 kpc ≲ R ≲ 14 kpc, |Z| ≲ 2 kpc, and −15° ≲ Galactocentric azimuth ≲ 30°. The APOGEE red-clump (APOGEE-RC) catalog contains photometry from the Two Micron All Sky Survey, reddening estimates, distances, line-of-sight velocities, stellar parameters and elemental abundances determined from the high-resolution APOGEE spectra, and matches to major proper motion catalogs. We determine the survey selection function for this data set and discuss how the RC selection samples the underlying stellar populations. We use this sample to limit any azimuthal variations in the median metallicity within the ≈45° azimuthal region covered by the current sample to be ⩽0.02 dex, which is more than an order of magnitude smaller than the radial metallicity gradient. This result constrains coherent non-axisymmetric flows within a few kiloparsecs from the Sun.
Author Cunha, Katia
Stassun, Keivan
Robin, Annie C.
Serenelli, Aldo
Kallinger, Thomas
Chaplin, William J.
Girardi, Léo
Holtzman, Jon
Frinchaboy, Peter M.
Mosser, Benoît
Shetrone, Matthew
Zasowski, Gail
Allende Prieto, Carlos
Johnson, Jennifer A.
Pinsonneault, Marc H.
Schiavon, Ricardo P.
Stello, Dennis
Pan, Kaike
Burton, Adam
O'Connell, Robert W.
Simmons, Audrey
Zamora, Olga
Bizyaev, Dmitry
Smith, Verne V.
Bovy, Jo
Andrews, Brett
Silva Aguirre, Victor
Epstein, Courtney
Nidever, David L.
Chojnowski, S. Drew
Mészáros, Szabolcs
Skrutskie, Michael
Basu, Sarbani
García Pérez, Ana E.
Weinberg, David H.
Kinemuchi, Karen
Oravetz, Daniel
Rix, Hans-Walter
Schultheis, Mathias
Hayden, Michael R.
Majewski, Steven R.
Hearty, Fred R.
Elsworth, Yvonne
García-Herńandez, Domingo A.
Schneider, Donald P.
Koesterke, Lars
Wilson, John C.
Hekker, Saskia
Rodrigues, Thaíse S.
Beers, Timothy C.
García, Rafael A.
Author_xml – sequence: 1
  givenname: Jo
  orcidid: 0000-0001-6855-442X
  surname: Bovy
  fullname: Bovy, Jo
– sequence: 2
  givenname: David L.
  surname: Nidever
  fullname: Nidever, David L.
– sequence: 3
  givenname: Hans-Walter
  orcidid: 0000-0003-4996-9069
  surname: Rix
  fullname: Rix, Hans-Walter
– sequence: 4
  givenname: Léo
  surname: Girardi
  fullname: Girardi, Léo
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  givenname: Gail
  surname: Zasowski
  fullname: Zasowski, Gail
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  givenname: S. Drew
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  surname: Chojnowski
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  givenname: Michael R.
  surname: Hayden
  fullname: Hayden, Michael R.
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  givenname: Thaíse S.
  surname: Rodrigues
  fullname: Rodrigues, Thaíse S.
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  givenname: Steven R.
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  fullname: Majewski, Steven R.
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  givenname: Jennifer A.
  surname: Johnson
  fullname: Johnson, Jennifer A.
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  givenname: Marc H.
  surname: Pinsonneault
  fullname: Pinsonneault, Marc H.
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  surname: Elsworth
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  givenname: Rafael A.
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  givenname: Domingo A.
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  surname: García Pérez
  fullname: García Pérez, Ana E.
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  givenname: Fred R.
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  givenname: Thomas
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  givenname: Karen
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  givenname: Annie C.
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  givenname: Ricardo P.
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  givenname: Donald P.
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  orcidid: 0000-0002-6590-1657
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  givenname: Aldo
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BackLink https://hal.science/hal-01275555$$DView record in HAL
https://www.osti.gov/biblio/22365489$$D View this record in Osti.gov
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Snippet The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey...
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SubjectTerms ABUNDANCE
Apogees
APPROXIMATIONS
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
COLOR
Disks
DISTANCE
DUSTS
GALACTIC EVOLUTION
Glass transition temperature
GRAVITATION
ISOCHRONOUS CYCLOTRONS
LUMINOSITY
Mathematical models
METALLICITY
MILKY WAY
PHOTOMETRY
Physics
PROPER MOTION
Sciences of the Universe
SPACE DEPENDENCE
SPECTRA
STAR EVOLUTION
Stars
SUN
SURFACES
Title THE APOGEE RED-CLUMP CATALOG: PRECISE DISTANCES, VELOCITIES, AND HIGH-RESOLUTION ELEMENTAL ABUNDANCES OVER A LARGE AREA OF THE MILKY WAY'S DISK
URI https://www.proquest.com/docview/1712568276
https://www.proquest.com/docview/1744713739
https://hal.science/hal-01275555
https://www.osti.gov/biblio/22365489
Volume 790
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