Observational Star Templates

Observational Star Templates

Stellar templates
Bayo et al, M types from Collinder 69
 Complete M spectral type sequence for a sample of confirm young sources (members of Collinder 69, ~5-20 Myr). Be aware that most spectra are not flux calibrated.
High-resolution optical library of late type subdwarfs
 A high-resolution (R = 40000), flux calibrated, optical+NIR (6400-8900A) library of late type subdwarfs, from late K to M9.5, obtained with UVES at VLT. The library is described in Rajpurohit et al. (2014)
Keck LRIS spectra of late-M, L and T dwarfs
 These spectra were obtained between 1997 and 1999; they are all flux calibrated and generally span the wavelength range 6000-10,000 A. Spectral types are on the Kirkpatrick et al system as defined in Kirkpatrick et al ApJS, 77, 417 (1991 - for M dwarfs) and Kirkpatrick et al ApJ 519, 802 (1999 - L dwarfs). While not all of these stars are primary spectral standards, they are all bright and should provide an adequate reference sequence.
Kesseli et al.
 An empirical library of stellar spectra created using spectra from the Sloan Digital Sky Survey’s Baryon Oscillation Spectroscopic Survey (BOSS).
L and T dwarf data archive
 L and T dwarf data from Chiu et al. 2006, Golimowski et al. 2004 and Knapp et al. 2004
MILES
 ~1000 stars spanning a large range in atmospheric parameters. The spectra were obtained at the 2.5m INT telescope and cover the range 3525-7500 Å at 2.5 Å (FWHM) spectral resolution
The NIRSPEC Brown Dwarf Spectroscopic Survey
 The Brown Dwarf Spectroscopic Survey (BDSS), established in 1998 by Dr. Ian McLean in collaboration with Dr. J. Davy Kirkpatrick at IPAC, is designed to study near-infrared moderate-to-high resolution spectra for a large sample of low-mass stars and sub-stellar mass objects in the M and newly defined L and T dwarf classes.
The SpeX Prism Spectral Libraries
 The SpeX Prism Spectral Libraries

 

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