Oscillator Strengths and Damping Constants for Atomic Lines in the J and H Bands

Abstract

We have built a line list in the near-infrared J and H bands (1.00-1.34, 1.49-1.80 um) by gathering a series of laboratory and computed line lists. Oscillator strengths and damping constants were computed or obtained by fitting the solar spectrum. The line list presented in this paper is, to our knowledge, the most complete one now available, and supersedes previous lists.

Accepted, Astrophysical Journal Supplement, tentatively scheduled for the Sep. 1999 Vol. 124 #1 issue. Text and tables also available at http://www.iagusp.usp.br/~jorge/

References in corpus (1)

• Mn I hyperfine structure in the near-infrared

Cited by in corpus (70)

• The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory
• A library of high resolution synthetic stellar spectra from 300nm to 1.8 micron with solar and alpha-enhanced composition
• The elemental composition of the Sun II. The iron group elements Sc to Ni
• Atmospheric Chemistry in Giant Planets, Brown Dwarfs, and Low-Mass Dwarf Stars III. Iron, Magnesium, and Silicon
• Precise radial velocities of giant stars. III. Spectroscopic stellar parameters
• Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca and Ti
• The remarkable solar twin HIP 56948: a prime target in the quest for other Earths
• The SDSS-III APOGEE Spectral Line List for H-band Spectroscopy
• Chemical Abundances in Field Red Giants from High-Resolution H-Band Spectra using the APOGEE Spectral Linelist
• The First Detailed Abundances for M giants in Baade's Window from Infrared Spectroscopy
• Chemical Evolution of the Galactic Bulge as Derived from High-Resolution Infrared Spectroscopy of K and M Red Giants
• High resolution infrared spectra of bulge globular clusters: Liller~1 and NGC 6553
• An H-band Spectroscopic Metallicity Calibration for M Dwarfs
• M-dwarf metallicities - A high-resolution spectroscopic study in the near infrared
• A near-infrared spectroscopic screening of the red giant populations in omega Centauri
• High resolution infrared spectra of bulge globular clusters: The extreme chemical abundances of Terzan 4 and Terzan 5
• Chemical abundance patterns in the inner Galaxy: the Scutum Red Supergiant Clusters
• Metallicities for 13 nearby open clusters from high-resolution spectroscopy of dwarf and giant stars. Stellar metallicity, stellar mass, and giant planets
• The chemical abundances in the Galactic Centre from the atmospheres of Red Supergiants
• Keck-Nirspec Infrared OH Lines: Oxygen Abundances in Metal-Poor Stars Down to [Fe/H] = -2.9
• Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553
• Sodium and Oxygen Abundances in the Open Cluster NGC 6791 from APOGEE H-Band Spectroscopy
• High resolution infrared spectroscopy of the old open cluster NGC6791
• Stellar and gaseous abundances in M82
• Oxygen Abundances in Metal-Poor Stars (-2.2 < [Fe/H] < -1.2) from Infrared OH lines
• Chemical abundances in giants stars of the tidally disrupted globular cluster NGC 6712 from high-resolution infrared spectroscopy
• Anatomy of a Young Massive Star Cluster: NGC 1569-B
• Another forbidden solar oxygen abundance: the [O I] 5577 A line
• Origin of $\alpha$-rich young stars: clues from C, N and O
• The Rise of the AGB in the Galactic Halo: Mg Isotopic Ratios and High Precision Elemental Abundances in M71 Giants
• Metallicity determination of M dwarfs - High-resolution IR spectroscopy
• Metallicity determination of M dwarfs - Expanded parameter range in metallicity and effective temperature
• Near-IR Spectroscopy of a Young Super-Star Cluster in NGC 6946: Chemical Abundances and Abundance Patterns
• A Low Solar Oxygen Abundance from the First Overtone OH Lines
• The Chemistry of the Trailing arm of the Sagittarius Dwarf Galaxy
• GIANO-TNG spectroscopy of red supergiants in the young star cluster RSGC2
• Infrared Spectroscopy of Symbiotic Stars. XII. The Neutron Star SyXB System 4U 1700+24 = V934 Herculis
• An abundance analysis of the symbiotic star CH Cyg
• Infrared Laboratory Oscillator Strengths of Fe I in the H-Band
• Method to Estimate the Effective Temperatures of Late-Type Giants using Line-Depth Ratios in the Wavelength Range 0.97-1.32$\mu$m
• Stellar population astrophysics (SPA) with the TNG. GIANO-B spectroscopy of red supergiants in Alicante 7 and Alicante 10
• FeI lines in 0.91-1.33 $\mu$m spectra of red giants for measuring the microturbulence and metallicities
• Chemical abundance analysis of symbiotic giants - III. Metallicity and CNO abundance patterns in 24 southern systems
• Tracers of Discs and Winds around Intermediate and High Mass Young Stellar Objects
• Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid
• Chemical abundance analysis of 13 southern symbiotic giants from high-resolution spectra at ~1.56 μm
• Metallicities for 6 nearby open clusters from high-resolution spectra of giant stars. [Fe/H] values for a planet search sample
• NIR spectroscopy of the Sun and HD20010 - Compiling a new linelist in the NIR
• NLTE Analysis of High Resolution H-band Spectra. II. Neutral Magnesium
• High-resolution CRIRES spectra of Terzan1: a metal-poor globular cluster toward the inner bulge
• Calculation of molecular line intensity in stellar atmospheres
• GIANO-TNG spectroscopy of red supergiants in the young star cluster RSGC3
• Identification of Absorption Lines of Heavy Metals in the Wavelength Range 0.97--1.32 Micron
• Stellar population astrophysics (SPA) with the TNG -- The Arcturus Lab
• The metallicity effect on line-depth ratios in APOGEE $H$-band spectra
• Line identification in high-resolution, near-infrared CRIRES spectra of chemically peculiar and Herbig Ae stars
• Absorption Lines in the 0.91-1.33 $\mu$m Spectra of Red Giants for Measuring Abundances of Mg, Si, Ca, Ti, Cr, and Ni
• Effective Temperature Estimations from Line Depth Ratios in the \H\ and \K-band Spectra of IGRINS
• Gemini/Phoenix H-band analysis of the globular cluster AL3
• Line-depth ratios as indicators of effective temperature and surface gravity
• Chemical abundance analysis of symbiotic giants. I. RW Hya and SY Mus
• Chemical abundance analysis of symbiotic giants. Metallicity and CNO abundance patterns in 14 northern S-type systems
• Chemical abundance analysis of symbiotic giants - II. AE Ara, BX Mon, KX TrA, and CL Sco
• MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars
• A Very Metal-poor RR Lyrae Star with a Disk Orbit Found in the Solar Neighborhood
• IR spectra of the microquasar GRS 1915+105 during a low state
• Possible progression of mass flow processes around young intermediate-mass stars based on high-resolution near-infrared spectroscopy. I. Taurus
• Prospects of Stellar Abundance Studies from Near-IR Spectra Observed with the E-ELT
• WINERED high-resolution near-infrared line catalog: A-type star
• On the lithium abundance of the visual binary components $\xi$ Boo A (G8V) and $\xi$ Boo B (K5V)