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Dataset / Observations of Solar Analog Field Stars from the Hamilton Echelle Spectrograph at …

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Title
Observations of Solar Analog Field Stars from the Hamilton Echelle Spectrograph at Lick Observatory
Creator
Lubin, Dan
Contributor
Holden, Bradford P.
Melis, Carl
Stock, Camille
Tytler, David
Date Created and/or Issued
2013 to 2014
Contributing Institution
UC San Diego, Research Data Curation Program
Collection
Observations of Solar Analog Field Stars from the Hamilton Echelle Spectrograph at Lick Observatory
Rights Information
Under copyright
Constraint(s) on Use: This work is protected by the U.S. Copyright Law (Title 17, U.S.C.). Use of this work beyond that allowed by "fair use" or any license applied to this work requires written permission of the copyright holder(s). Responsibility for obtaining permissions and any use and distribution of this work rests exclusively with the user and not the UC San Diego Library. Inquiries can be made to the UC San Diego Library program having custody of the work.
Use: This work is available from the UC San Diego Library. This digital copy of the work is intended to support research, teaching, and private study.
Rights Holder and Contact
UC Regents
Description
This observing program used the Hamilton Echelle Spectrograph on the three meter Shane telescope at Lick Observatory to obtain high resolution spectroscopic observations of 211 solar analog field stars. Observations were made over 22 nights between February 2013 and January 2014. Our criteria for selecting solar analogs include: (1) effective temperature within ±500 K of solar; (2) -0.3 < [Fe/H] < +0.3; (3) absolute magnitude within ±0.5 of the Hipparcos main sequence (Wright 2004: AJ, 128, 1273). Effective temperatures were taken from the third version of the Geneva-Copenhagen survey (Holmberg et al. (2009: A&A, 501, 941), with temperature, metallicity and isochrone age estimates refined by Casagrande et al. (2011: A&A, A138). An additional selection criterion is that a star have no indication in the SIMBAD Astronomical Database of being part of a double or multiple system, or being a chromospherically active variable such as type RS CVn or BY Dra (note that SIMBAD entries are periodically updated and users should recheck this criterion). Table 1 (in the Readme) lists the program stars. Each ascii text file in this collection contains one spectrum, with the star's Hipparcos catalog identifier (HIP) as the filename. The columns in each file are, left to right: (1) Hamilton Echelle Spectrograph order number (integer); (2) Wavelength (Ångstroms); (3) Flux (machine units); (4) Variance (such that the signal-to-noise ratio and be estimated as the Flux divided by the square root of the Variance). Information about the Hamilton Echelle Spectrograph, including the table of orders, can be found at https://mthamilton.ucolick.org/techdocs/instruments/hamspec/index.html/
NASA 80NSSC21K1947 and 80NSSC20K0441.
Research Data Curation Program, UC San Diego, La Jolla, 92093-0175 (https://lib.ucsd.edu/rdcp)
Lubin, Dan; Holden, Bradford P.; Stock, Camille; Melis, Carl; Tytler, David. (2023). Observations of Solar Analog Field Stars from the Hamilton Echelle Spectrograph at Lick Observatory. UC San Diego Library Digital Collections. https://doi.org/10.6075/J0X34XN2
Type
dataset
Identifier
ark:/20775/bb9942679r
Subject
Stellar astrophysics
Solar analogs
Echelle spectrograph
Spectroscopy
Hamilton Echelle Spectrograph
Lick Observatory
C. Donald Shane Telescope

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