The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies

The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections. To assist in these tasks, we visually inspect DESI spectra of approximately 2500 bright galaxies, 3500 luminous red galaxies...

Full description

Autores:
Ting-Wen Lan
Tojeiro, R.
Armengaud, E.
Prochaska, J. Xavier
Davis, T. M.
Alexander, David M.
Raichoor, A.
Zhou, Rongpu
Yèche, Christophe
Balland, C.
BenZvi, S.
Berti, A.
Carr, A.
Chittenden, H.
Cole, S.
Cousinou, M. C.
Dawson, K.
Dey, Biprateep
Douglass, K.
Edge, A.
Escoffier, S.
Glanville, A.
Gontcho A Gontcho, Satya
Guy, J.
Hahn, C.
Howlett, C.
Hwang, Ho Seong
Jiang, L.
Kovács, A.
Mezcua, M.
Moor, S.
Nadathur, S.
Oh, M.
Parkinson, D.
Rocher, A.
Ross, A. J.
Ruhlmann-Kleider, V.
Sabiu, C. G.
Said, K.
Saulder, C.
Sierra-Porta, D.
Weiner, B.
Yu, J.
Zarrouk, Pauline
Zhang, Y.
Zou, Hu
Ahlen, S.
Bailey, S.
Cooper, A. P.
De la Macorra, A.
Dey, A.
Dhungana, G.
Doel, P.
Eftekharzadeh, S.
Fanning, K.
Font-Ribera, A.
Garrison, L.
Gaztañaga, E.
Kehoe, R.
Kisner, T.
Kremin, A.
Landriau, M.
Le Guillou, L.
Levi, Michael E.
Magneville, C.
Meisner, Aaron M.
Miquel, R.
Moustakas, J.
Myers, Adam D.
Newman, Jeffrey A.
Nie, J. D.
Palanque-Delabrouille, N.
Percival, W. J.
Poppett, C.
Prada, F.
Schubnell, M.
Tarlé, Gregory
Weaver, B. A.
Zhang, K.
Zhou, Zhimin
Tipo de recurso:
Fecha de publicación:
2023
Institución:
Universidad Tecnológica de Bolívar
Repositorio:
Repositorio Institucional UTB
Idioma:
eng
OAI Identifier:
oai:repositorio.utb.edu.co:20.500.12585/12083
Acceso en línea:
https://hdl.handle.net/20.500.12585/12083
Palabra clave:
Galaxy spectroscopy
Observational cosmology
LEMB
Rights
openAccess
License
http://creativecommons.org/publicdomain/zero/1.0/
id UTB2_8da6c4f92a4b40f5e00a66cdd25137da
oai_identifier_str oai:repositorio.utb.edu.co:20.500.12585/12083
network_acronym_str UTB2
network_name_str Repositorio Institucional UTB
repository_id_str
dc.title.spa.fl_str_mv The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
title The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
spellingShingle The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
Galaxy spectroscopy
Observational cosmology
LEMB
title_short The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
title_full The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
title_fullStr The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
title_full_unstemmed The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
title_sort The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies
dc.creator.fl_str_mv Ting-Wen Lan
Tojeiro, R.
Armengaud, E.
Prochaska, J. Xavier
Davis, T. M.
Alexander, David M.
Raichoor, A.
Zhou, Rongpu
Yèche, Christophe
Balland, C.
BenZvi, S.
Berti, A.
Carr, A.
Chittenden, H.
Cole, S.
Cousinou, M. C.
Dawson, K.
Dey, Biprateep
Douglass, K.
Edge, A.
Escoffier, S.
Glanville, A.
Gontcho A Gontcho, Satya
Guy, J.
Hahn, C.
Howlett, C.
Hwang, Ho Seong
Jiang, L.
Kovács, A.
Mezcua, M.
Moor, S.
Nadathur, S.
Oh, M.
Parkinson, D.
Rocher, A.
Ross, A. J.
Ruhlmann-Kleider, V.
Sabiu, C. G.
Said, K.
Saulder, C.
Sierra-Porta, D.
Weiner, B.
Yu, J.
Zarrouk, Pauline
Zhang, Y.
Zou, Hu
Ahlen, S.
Bailey, S.
Cooper, A. P.
De la Macorra, A.
Dey, A.
Dhungana, G.
Doel, P.
Eftekharzadeh, S.
Fanning, K.
Font-Ribera, A.
Garrison, L.
Gaztañaga, E.
Kehoe, R.
Kisner, T.
Kremin, A.
Landriau, M.
Le Guillou, L.
Levi, Michael E.
Magneville, C.
Meisner, Aaron M.
Miquel, R.
Moustakas, J.
Myers, Adam D.
Newman, Jeffrey A.
Nie, J. D.
Palanque-Delabrouille, N.
Percival, W. J.
Poppett, C.
Prada, F.
Schubnell, M.
Tarlé, Gregory
Weaver, B. A.
Zhang, K.
Zhou, Zhimin
dc.contributor.author.none.fl_str_mv Ting-Wen Lan
Tojeiro, R.
Armengaud, E.
Prochaska, J. Xavier
Davis, T. M.
Alexander, David M.
Raichoor, A.
Zhou, Rongpu
Yèche, Christophe
Balland, C.
BenZvi, S.
Berti, A.
Carr, A.
Chittenden, H.
Cole, S.
Cousinou, M. C.
Dawson, K.
Dey, Biprateep
Douglass, K.
Edge, A.
Escoffier, S.
Glanville, A.
Gontcho A Gontcho, Satya
Guy, J.
Hahn, C.
Howlett, C.
Hwang, Ho Seong
Jiang, L.
Kovács, A.
Mezcua, M.
Moor, S.
Nadathur, S.
Oh, M.
Parkinson, D.
Rocher, A.
Ross, A. J.
Ruhlmann-Kleider, V.
Sabiu, C. G.
Said, K.
Saulder, C.
Sierra-Porta, D.
Weiner, B.
Yu, J.
Zarrouk, Pauline
Zhang, Y.
Zou, Hu
Ahlen, S.
Bailey, S.
Cooper, A. P.
De la Macorra, A.
Dey, A.
Dhungana, G.
Doel, P.
Eftekharzadeh, S.
Fanning, K.
Font-Ribera, A.
Garrison, L.
Gaztañaga, E.
Kehoe, R.
Kisner, T.
Kremin, A.
Landriau, M.
Le Guillou, L.
Levi, Michael E.
Magneville, C.
Meisner, Aaron M.
Miquel, R.
Moustakas, J.
Myers, Adam D.
Newman, Jeffrey A.
Nie, J. D.
Palanque-Delabrouille, N.
Percival, W. J.
Poppett, C.
Prada, F.
Schubnell, M.
Tarlé, Gregory
Weaver, B. A.
Zhang, K.
Zhou, Zhimin
dc.subject.keywords.spa.fl_str_mv Galaxy spectroscopy
Observational cosmology
topic Galaxy spectroscopy
Observational cosmology
LEMB
dc.subject.armarc.none.fl_str_mv LEMB
description The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections. To assist in these tasks, we visually inspect DESI spectra of approximately 2500 bright galaxies, 3500 luminous red galaxies (LRGs), and 10,000 emission-line galaxies (ELGs) to obtain robust redshift identifications. We then utilize the visually inspected redshift information to characterize the performance of the DESI operation. Based on the visual inspection (VI) catalogs, our results show that the final survey design yields samples of bright galaxies, LRGs, and ELGs with purity greater than 99%. Moreover, we demonstrate that the precision of the redshift measurements is approximately 10 km s−1 for bright galaxies and ELGs and approximately 40 km s−1 for LRGs. The average redshift accuracy is within 10 km s−1 for the three types of galaxies. The VI process also helps improve the quality of the DESI data by identifying spurious spectral features introduced by the pipeline. Finally, we show examples of unexpected real astronomical objects, such as Lyα emitters and strong lensing candidates, identified by VI. These results demonstrate the importance and utility of visually inspecting data from incoming and upcoming surveys, especially during their early operation phases.
publishDate 2023
dc.date.accessioned.none.fl_str_mv 2023-06-02T18:21:45Z
dc.date.available.none.fl_str_mv 2023-06-02T18:21:45Z
dc.date.issued.none.fl_str_mv 2023-01-20
dc.date.submitted.none.fl_str_mv 2023-06-02
dc.type.coarversion.fl_str_mv http://purl.org/coar/version/c_b1a7d7d4d402bcce
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dc.type.driver.spa.fl_str_mv info:eu-repo/semantics/article
dc.type.hasversion.spa.fl_str_mv info:eu-repo/semantics/draft
dc.type.spa.spa.fl_str_mv http://purl.org/coar/resource_type/c_6501
status_str draft
dc.identifier.citation.spa.fl_str_mv Ting-Wen Lan et al 2023 ApJ 943 68
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12585/12083
dc.identifier.instname.spa.fl_str_mv Universidad Tecnológica de Bolívar
dc.identifier.reponame.spa.fl_str_mv Repositorio Universidad Tecnológica de Bolívar
identifier_str_mv Ting-Wen Lan et al 2023 ApJ 943 68
Universidad Tecnológica de Bolívar
Repositorio Universidad Tecnológica de Bolívar
url https://hdl.handle.net/20.500.12585/12083
dc.language.iso.spa.fl_str_mv eng
language eng
dc.rights.coar.fl_str_mv http://purl.org/coar/access_right/c_abf2
dc.rights.uri.*.fl_str_mv http://creativecommons.org/publicdomain/zero/1.0/
dc.rights.accessrights.spa.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.cc.*.fl_str_mv CC0 1.0 Universal
rights_invalid_str_mv http://creativecommons.org/publicdomain/zero/1.0/
CC0 1.0 Universal
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.extent.none.fl_str_mv 18 páginas
dc.format.mimetype.spa.fl_str_mv application/pdf
dc.publisher.place.spa.fl_str_mv Cartagena de Indias
dc.source.spa.fl_str_mv The Astrophysical Journal - Vol. 943 No. 1 (2023)
institution Universidad Tecnológica de Bolívar
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D.2be50d08-2edf-4eab-a6ce-e8ecdaa5e68fPalanque-Delabrouille, N.16ec333f-6c00-4b23-b9ff-bd7f8748d4acPercival, W. J.7b9180a7-f71d-42d8-a3ea-6dfbfd85ed1ePoppett, C.30e2b92a-0b65-4107-bcf7-b8c66f131a2aPrada, F.fa884f57-5ffa-4a2d-a73b-a82ef26d43d2Schubnell, M.2b60a3da-9853-458c-a665-2dad945056adTarlé, Gregorya50163ed-5b0f-4908-9e82-dbb1672b7cbcWeaver, B. A.f2142224-6c0f-4167-b627-a779e9b56d48Zhang, K.d914c273-a53a-40a7-a4d8-d93087feb385Zhou, Zhiminfa6d3668-9150-436e-a229-5839703a7e692023-06-02T18:21:45Z2023-06-02T18:21:45Z2023-01-202023-06-02Ting-Wen Lan et al 2023 ApJ 943 68https://hdl.handle.net/20.500.12585/12083Universidad Tecnológica de BolívarRepositorio Universidad Tecnológica de BolívarThe Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections. To assist in these tasks, we visually inspect DESI spectra of approximately 2500 bright galaxies, 3500 luminous red galaxies (LRGs), and 10,000 emission-line galaxies (ELGs) to obtain robust redshift identifications. We then utilize the visually inspected redshift information to characterize the performance of the DESI operation. Based on the visual inspection (VI) catalogs, our results show that the final survey design yields samples of bright galaxies, LRGs, and ELGs with purity greater than 99%. Moreover, we demonstrate that the precision of the redshift measurements is approximately 10 km s−1 for bright galaxies and ELGs and approximately 40 km s−1 for LRGs. The average redshift accuracy is within 10 km s−1 for the three types of galaxies. The VI process also helps improve the quality of the DESI data by identifying spurious spectral features introduced by the pipeline. Finally, we show examples of unexpected real astronomical objects, such as Lyα emitters and strong lensing candidates, identified by VI. These results demonstrate the importance and utility of visually inspecting data from incoming and upcoming surveys, especially during their early operation phases.18 páginasapplication/pdfenghttp://creativecommons.org/publicdomain/zero/1.0/info:eu-repo/semantics/openAccessCC0 1.0 Universalhttp://purl.org/coar/access_right/c_abf2The Astrophysical Journal - Vol. 943 No. 1 (2023)The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxiesinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/drafthttp://purl.org/coar/resource_type/c_6501http://purl.org/coar/version/c_b1a7d7d4d402bccehttp://purl.org/coar/resource_type/c_2df8fbb1Galaxy spectroscopyObservational cosmologyLEMBCartagena de IndiasAbareshi B., Aguilar J., Ahlen S. et al. 2022 ApJ 164 62Aihara H., AlSayyad Y., Ando M. et al. 2019 PASJ 71 114Alexander D. M., Davis T. M., Chaussidon E. et al. 2022 arXiv:2208.08517Allende Prieto C., Cooper A. P., Dey A. et al. 2020 RNAAS 4 188Blake C., Davis T., Poole G. B. et al. 2011 MNRAS 415 2892Bolton A. S., Burles S., Koopmans L. V. E. et al. 2008 ApJ 682 964Brownstein J. R., Bolton A. S., Schlegel D. J. et al. 2012 ApJ 744 41Chaussidon E., Yèche C., Palanque-Delabrouille N. et al. 2022 arXiv:2208.08511Cirasuolo M. and MOONS Consortium 2016 ASP Conf. Ser. 507, Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields ed I. Skillen, M. Balcells and S. Trager (San Francisco, CA: ASP) 109Cooper A. P., Koposov S. E., Allende Prieto C. et al. 2022 arXiv:2208.08514Comparat J., Delubac T., Jouvel S. et al. 2016 A&A 592 A121Dawson K. S., Kneib J.-P., Percival W. J. et al. 2016 AJ 151 44de Jong R. S., Barden S. C., Bellido-Tirado O. et al. 2016 Proc. SPIE 9908 99081ODESI Collaboration, Aghamousa A., Aguilar A. et al. 2016a arXiv:1611.00036DESI Collaboration, Aghamousa A., Aguilar A. et al. 2016b arXiv:1611.00037Dey A., Schlegel D. J., Lang D. et al. 2019 AJ 157 168Driver S. P., Hill D. T., Kelvin L. S. et al. 2011 MNRAS 413 971Eisenstein D. J., Annis J., Gunn J. E. et al. 2001 AJ 122 2267Guy J., Bailey S., Kremin A. et al. 2022 arXiv: 2209.14482Eisenstein D. J., Zehavi I., Hogg D. W. et al. 2005 ApJ 633 560Hahn C., Wilson M. J., Ruiz-Macias O. et al. 2022 arXiv:2208.08512Hill G. J., Gebhardt K., Komatsu E. et al. 2008 ASP Conf. Ser. 399, Panoramic Views of Galaxy Formation and Evolution ed T. Kodama, T. Yomada and K. Aoki (San Francisco, CA: ASP) 115Kollmeier J. A., Zasowski G., Rix H.-W. et al. 2017 arXiv:1711.03234Leclercq F., Bacon R., Wisotzki L. et al. 2017 A&A 608 A8Levi M., Bebek C., Beers T. et al. 2013 arXiv:1308.0847Lyke B. W., Higley A. N., McLane J. N. et al. 2020 ApJS 250 8Myers A. D., Moustakas J., Bailey S. et al. 2023 AJ 165 50Newman J. A., Cooper M. C., Davis M. et al. 2013 ApJS 208 5Ouchi M., Ono Y. and Shibuya T. 2020 ARA&A 58 617Pâris I., Petitjean P., Aubourg É. et al. 2018 A&A 613 A51Prakash A., Licquia T. C., Newman J. A. et al. 2016 ApJS 224 34Raichoor A., de Mattia A., Ross A. J. et al. 2021 MNRAS 500 3254Raichoor A., Eisenstein D. J., Karim T. et al. 2020 RNAAS 4 180Raichoor A., Moustakas J., Newman J. A. et al. 2022 arXiv:2208.08513Reid B., Ho S., Padmanabhan N. et al. 2016 MNRAS 455 1553Ruiz-Macias O., Zarrouk P., Cole S. et al. 2020 RNAAS 4 187Silber J. H., Fagrelius P., Fanning K. et al. 2023 ApJ 165 40Strauss M. A., Weinberg D. H., Lupton R. H. et al. 2002 AJ 124 1810Takada M., Ellis R. S., Chiba M. et al. 2014 PASJ 66 R1Talbot M. S., Brownstein J. R., Bolton A. S. et al. 2018 MNRAS 477 195Yèche C., Palanque-Delabrouille N., Claveau C.-A. et al. 2020 RNAAS 4 179Zhou R., Dey B., Newman J. A. et al. 2022 arXiv:2208.08515Zhou R., Newman J. A., Dawson K. 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