The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)

The Hobby–Eberly Telescope (HET) VIRUS Parallel Survey (HETVIPS) is a blind spectroscopic program that sparsely covers approximately two-thirds of the celestial sphere and consists of roughly 252 million fiber spectra. The spectra were taken in parallel mode with the Visible Integral-field Replicabl...

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Main Authors: Gregory R. Zeimann, Maya H. Debski, Donald P. Schneider, William P. Bowman, Niv Drory, Gary J. Hill, Hanshin Lee, Phillip MacQueen, Matthew Shetrone
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad35b8
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author Gregory R. Zeimann
Maya H. Debski
Donald P. Schneider
William P. Bowman
Niv Drory
Gary J. Hill
Hanshin Lee
Phillip MacQueen
Matthew Shetrone
author_facet Gregory R. Zeimann
Maya H. Debski
Donald P. Schneider
William P. Bowman
Niv Drory
Gary J. Hill
Hanshin Lee
Phillip MacQueen
Matthew Shetrone
author_sort Gregory R. Zeimann
collection DOAJ
description The Hobby–Eberly Telescope (HET) VIRUS Parallel Survey (HETVIPS) is a blind spectroscopic program that sparsely covers approximately two-thirds of the celestial sphere and consists of roughly 252 million fiber spectra. The spectra were taken in parallel mode with the Visible Integral-field Replicable Unit Spectrograph (VIRUS) instrument when the HET was observing a primary target with other HET facility instruments. VIRUS can simultaneously obtain approximately 35,000 spectra covering 3470–5540 Å at a spectral resolution of ≈800. Although the vast majority of these spectra cover blank sky, we used the Pan-STARRS1 Data Release 2 Stacked Catalog to identify objects encompassed in the HETVIPS pointings and extract their spectra. This paper presents the first HETVIPS data release, containing 493,012 flux-calibrated spectra obtained through 2023 March 31, as well as a description of the data processing technique. Each of the object spectra were classified, resulting in a catalog of 74,196 galaxies, 4,087 quasars, 259,396 stars, and 154,543 unknown sources.
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spelling doaj.art-197ef1cf29bb4d948d8417b50b62da832024-04-23T14:47:49ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-0196611410.3847/1538-4357/ad35b8The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)Gregory R. Zeimann0https://orcid.org/0000-0003-2307-0629Maya H. Debski1Donald P. Schneider2https://orcid.org/0000-0001-7240-7449William P. Bowman3https://orcid.org/0000-0003-4381-5245Niv Drory4https://orcid.org/0000-0002-7339-3170Gary J. Hill5https://orcid.org/0000-0001-6717-7685Hanshin Lee6https://orcid.org/0000-0002-3559-5310Phillip MacQueen7Matthew Shetrone8https://orcid.org/0000-0003-0509-2656Hobby Eberly Telescope, University of Texas , Austin, Austin, TX, 78712, USA ; gregz@astro.as.utexas.eduDepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Austin, TX 78712, USADepartment of Astronomy & Astrophysics, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University , University Park, PA 16802, USADepartment of Astronomy, Yale University , New Haven, CT 06511, USAMcDonald Observatory, The University of Texas at Austin , Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Austin, TX 78712, USA; McDonald Observatory, The University of Texas at Austin , Austin, TX 78712, USAMcDonald Observatory, The University of Texas at Austin , Austin, TX 78712, USAMcDonald Observatory, The University of Texas at Austin , Austin, TX 78712, USAUniversity of California Observatories, University of California Santa Cruz , Santa Cruz, CA 95064, USAThe Hobby–Eberly Telescope (HET) VIRUS Parallel Survey (HETVIPS) is a blind spectroscopic program that sparsely covers approximately two-thirds of the celestial sphere and consists of roughly 252 million fiber spectra. The spectra were taken in parallel mode with the Visible Integral-field Replicable Unit Spectrograph (VIRUS) instrument when the HET was observing a primary target with other HET facility instruments. VIRUS can simultaneously obtain approximately 35,000 spectra covering 3470–5540 Å at a spectral resolution of ≈800. Although the vast majority of these spectra cover blank sky, we used the Pan-STARRS1 Data Release 2 Stacked Catalog to identify objects encompassed in the HETVIPS pointings and extract their spectra. This paper presents the first HETVIPS data release, containing 493,012 flux-calibrated spectra obtained through 2023 March 31, as well as a description of the data processing technique. Each of the object spectra were classified, resulting in a catalog of 74,196 galaxies, 4,087 quasars, 259,396 stars, and 154,543 unknown sources.https://doi.org/10.3847/1538-4357/ad35b8SurveysRedshift surveysStellar classificationSky surveysCatalogs
spellingShingle Gregory R. Zeimann
Maya H. Debski
Donald P. Schneider
William P. Bowman
Niv Drory
Gary J. Hill
Hanshin Lee
Phillip MacQueen
Matthew Shetrone
The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)
The Astrophysical Journal
Surveys
Redshift surveys
Stellar classification
Sky surveys
Catalogs
title The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)
title_full The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)
title_fullStr The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)
title_full_unstemmed The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)
title_short The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)
title_sort hobby eberly telescope virus parallel survey hetvips
topic Surveys
Redshift surveys
Stellar classification
Sky surveys
Catalogs
url https://doi.org/10.3847/1538-4357/ad35b8
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