The LBT Yp Project: MODS Optical Spectra of Metal-Poor Nebulae
Authors/Creators
Description
1d wavelength- and flux-calibrated optical spectra from 3300-10,000A of 58 low-metallicity galaxies from the Large Binocular Telescope (LBT) Multi-Object Double Spectrographs (MODS1 and MODS2). These data were used by the LBT Yp Project, and described in Paper II (Rogers et al., 2026, ApJ, 1008, 238 (doi.org/10.3847/1538-4357/ae87a0).
The LBT Yp Project papers were released as an ApJ Focus Issue.
These are FITS bintable format files of the 1d spectra (wavelength, flux, and errors). All spectra are on a linear wavelength scale with 0.5A/pixel.
- Wavelengths are observed wavelength in Angstroms
- Fluxes are relative flux in F_lambda units. 0.0 means "no data"
- Flux errors in relative F_lambda units. 0.0 means "no data"
Most of the spectra were acquired with both MODS1 and MODS2, but some were taken with MODS1 or MODS2 alone when the other spectrograph was unavailable (e.g., offline for maintenance). See Rogers et al. 2026 for the full details of the spectral reduction and analysis.
Primary HDU
The primary header data units (HDUs) of the FITS files have additional metadata describing the individual observations:
OBJECT - galaxy name (e.g., Markarian 71)
OBJRA,OBJDEC - object J2000 celestial coordinates
EQUINOX, RADECSYS - celestial coordinate equinox and system
DATE-OBS - observing date and time in UTC at start of the observation sequence
MJDOBS - modified UTC Julian Date at start of the observation sequence
EXPTIME - unit exposure time in seconds of each individual spectrum
POSANGLE - celestial position angle of the slit in degrees east of north
EXPTOTAL - total accumulated exposure time in seconds summed over all combined dither positions. If both MODS were used, this is the total exposure time for both (e.g., 7200 sec = 2x3600s on MODS1 and MODS2)
PROJECT, PI_NAMES - Project name and PIs
PIPELINE - spectral data reduction pipeline software and version used
PUBTITLE - title of the associated journal paper
AUTHOR - lead author of the associated journal paper
PUBDOI - publication DOI for the associated ApJ paper
REPODOI - this data repository's DOI (Zenodo)
DATE - UTC data/time this FITS file was created
CREATOR - software used to create this FITS file
TELESCOP - Telescope for the observations
OBSERVAT - Observatory site where the telescope is located
INSTRUME - Instrument(s) used for the observations. Value is MODS1+2 if data are co-added from both MODS, otherwise MODS1 or MODS2 if only one MODS was available for use
SLITMASK - MODS segmented long-slit mask identifier, LS = long-slit mask, followed by format code NxLxW; N = number of slits, L = slit length in arcseconds, W = slit width in arcseconds
SLITWID - mask slit width in arcseconds
RGRATING/BGRATING - MODS red/blue channel grating used
RGRORDER/BGRORDER - MODS red/blue channel grating order (integer)
RCENLAM/BCENLAM - nominal central wavelength for the red/blue grating in Angstroms
LAMPIX - the linear dispersion in angstroms/pixel of the 1d spectrum
Files
Files
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Additional details
Related works
- Is cited by
- Journal article: 10.3847/1538-4357/ae879b (DOI)
- Journal article: 10.3847/1538-4357/ae869c (DOI)
- Is described by
- Journal article: 10.3847/1538-4357/ae879f (DOI)
- Is published in
- Journal article: 10.3847/1538-4357/ae87a0 (DOI)
- Is supplemented by
- Dataset: 10.5281/zenodo.19681448 (DOI)
Funding
- U.S. National Science Foundation
- Collaborative Research: A Better Measurement of the Primordial Helium Abundance AST-2205817
- U.S. National Science Foundation
- Collaborative Research: A Better Measurement of the Primordial Helium Abundance AST-2205864
- U.S. National Science Foundation
- Collaborative Research: A Better Measurement of the Primordial Helium Abundance AST-2205958