The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec

We present new results on the rest-frame UV luminosity function (UVLF) and stellar mass-to-light ( M / L ) ratio of bright ( M _UV  ≲ −20 mag) spectroscopically confirmed galaxies at z  = 7–9 derived from the BoRG-JWST survey, a unique data set of NIRSpec prism follow-up of Hubble Space Telescope (H...

Full description

Saved in:
Bibliographic Details
Main Authors: Sofía Rojas-Ruiz, Micaela Bagley, Guido Roberts-Borsani, Tommaso Treu, Steven L. Finkelstein, Takahiro Morishita, Nicha Leethochawalit, Charlotte Mason, Eduardo Bañados, Michele Trenti, Massimo Stiavelli, L. Y. Aaron Yung, Pablo Arrabal Haro, Rachel S. Somerville, Christian Soto
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adc67d
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1850134831382396928
author Sofía Rojas-Ruiz
Micaela Bagley
Guido Roberts-Borsani
Tommaso Treu
Steven L. Finkelstein
Takahiro Morishita
Nicha Leethochawalit
Charlotte Mason
Eduardo Bañados
Michele Trenti
Massimo Stiavelli
L. Y. Aaron Yung
Pablo Arrabal Haro
Rachel S. Somerville
Christian Soto
author_facet Sofía Rojas-Ruiz
Micaela Bagley
Guido Roberts-Borsani
Tommaso Treu
Steven L. Finkelstein
Takahiro Morishita
Nicha Leethochawalit
Charlotte Mason
Eduardo Bañados
Michele Trenti
Massimo Stiavelli
L. Y. Aaron Yung
Pablo Arrabal Haro
Rachel S. Somerville
Christian Soto
author_sort Sofía Rojas-Ruiz
collection DOAJ
description We present new results on the rest-frame UV luminosity function (UVLF) and stellar mass-to-light ( M / L ) ratio of bright ( M _UV  ≲ −20 mag) spectroscopically confirmed galaxies at z  = 7–9 derived from the BoRG-JWST survey, a unique data set of NIRSpec prism follow-up of Hubble Space Telescope (HST)–selected sources from random-pointing imaging. By selecting galaxies from over 300 independent sight lines, the survey minimizes cosmic variance, ensuring a statistically robust sample of the bright-galaxy population during the epoch of reionization. The data are used to constrain, for the first time, the bright end of the UVLF at z  = 7–9 from spectroscopically confirmed galaxies over eight independent fields. We find that the bright end of the UVLF is higher than found using imaging over JWST legacy fields, suggesting that the latter may be significantly affected by cosmic variance, and thus reducing the tension with recent findings from JWST at z  > 10 and comparable to models invoking little dust attenuation and bursty star formation. Additionally, we use the galaxies’ JWST spectra to infer their stellar masses and M / L ratios relative to other HST and JWST studies. We show that the stellar mass scales almost linearly with UV luminosity ( M ${}_{* }\propto {L}_{{\rm{UV}}}^{0.85\pm 0.12}$ ), albeit with large (∼0.5 dex) intrinsic scatter, consistent with stochastic bursts of star formation in early galaxy formation.
format Article
id doaj-art-9a4741c745114b82bd45ca1937dddc56
institution OA Journals
issn 1538-4357
language English
publishDate 2025-01-01
publisher IOP Publishing
record_format Article
series The Astrophysical Journal
spelling doaj-art-9a4741c745114b82bd45ca1937dddc562025-08-20T02:31:37ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-0198518010.3847/1538-4357/adc67dThe BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpecSofía Rojas-Ruiz0https://orcid.org/0000-0003-2349-9310Micaela Bagley1https://orcid.org/0000-0002-9921-9218Guido Roberts-Borsani2https://orcid.org/0000-0002-4140-1367Tommaso Treu3https://orcid.org/0000-0002-8460-0390Steven L. Finkelstein4https://orcid.org/0000-0001-8519-1130Takahiro Morishita5https://orcid.org/0000-0002-8512-1404Nicha Leethochawalit6https://orcid.org/0000-0003-4570-3159Charlotte Mason7https://orcid.org/0000-0002-3407-1785Eduardo Bañados8https://orcid.org/0000-0002-2931-7824Michele Trenti9https://orcid.org/0000-0001-9391-305XMassimo Stiavelli10https://orcid.org/0000-0001-9935-6047L. Y. Aaron Yung11https://orcid.org/0000-0003-3466-035XPablo Arrabal Haro12https://orcid.org/0000-0002-7959-8783Rachel S. Somerville13https://orcid.org/0000-0002-6748-6821Christian Soto14https://orcid.org/0000-0001-7840-2972Department of Physics and Astronomy, University of California , Los Angeles, 430 Portola Plaza, Los Angeles, CA 90095, USA ; rojas@astro.ucla.eduDepartment of Astronomy, The University of Texas at Austin , 2515 Speedway, Austin, TX 78712, USA; Astrophysics Science Division, NASA Goddard Space Flight Center , 8800 Greenbelt Rd., Greenbelt, MD 20771, USADepartment of Astronomy, University of Geneva , Chemin Pegasi 51, 1290 Versoix, SwitzerlandDepartment of Physics and Astronomy, University of California , Los Angeles, 430 Portola Plaza, Los Angeles, CA 90095, USA ; rojas@astro.ucla.eduDepartment of Astronomy, The University of Texas at Austin , 2515 Speedway, Austin, TX 78712, USAIPAC, California Institute of Technology , MC 314-6, 1200 E. California Boulevard, Pasadena, CA 91125, USANational Astronomical Research Institute of Thailand (NARIT) , Mae Rim, Chiang Mai, 50180, ThailandCosmic Dawn Center (DAWN); Niels Bohr Institute, University of Copenhagen , Jagtvej 128, DK-2200, Copenhagen N, DenmarkMax Planck Institut für Astronomie , Königstuhl 17, D-69117, Heidelberg, GermanySchool of Physics, University of Melbourne , Parkville 3010, VIC, Australia; ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) , AustraliaSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA; Department of Physics & Astronomy, Johns Hopkins University , Baltimore, MD 21218, USA; Department of Astronomy, University of Maryland , College Park, MD 20742, USASpace Telescope Science Institute , 3700 San Martin Dr., Baltimore, MD 21218, USANSF’s National Optical-Infrared Astronomy Research Laboratory , 950 N. Cherry Ave., Tucson, AZ 85719, USACenter for Computational Astrophysics, Flatiron Institute , 162 5th Avenue, New York, NY 10010, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USAWe present new results on the rest-frame UV luminosity function (UVLF) and stellar mass-to-light ( M / L ) ratio of bright ( M _UV  ≲ −20 mag) spectroscopically confirmed galaxies at z  = 7–9 derived from the BoRG-JWST survey, a unique data set of NIRSpec prism follow-up of Hubble Space Telescope (HST)–selected sources from random-pointing imaging. By selecting galaxies from over 300 independent sight lines, the survey minimizes cosmic variance, ensuring a statistically robust sample of the bright-galaxy population during the epoch of reionization. The data are used to constrain, for the first time, the bright end of the UVLF at z  = 7–9 from spectroscopically confirmed galaxies over eight independent fields. We find that the bright end of the UVLF is higher than found using imaging over JWST legacy fields, suggesting that the latter may be significantly affected by cosmic variance, and thus reducing the tension with recent findings from JWST at z  > 10 and comparable to models invoking little dust attenuation and bursty star formation. Additionally, we use the galaxies’ JWST spectra to infer their stellar masses and M / L ratios relative to other HST and JWST studies. We show that the stellar mass scales almost linearly with UV luminosity ( M ${}_{* }\propto {L}_{{\rm{UV}}}^{0.85\pm 0.12}$ ), albeit with large (∼0.5 dex) intrinsic scatter, consistent with stochastic bursts of star formation in early galaxy formation.https://doi.org/10.3847/1538-4357/adc67dHigh-redshift galaxiesStar formationReionizationCosmologyObservational astronomy
spellingShingle Sofía Rojas-Ruiz
Micaela Bagley
Guido Roberts-Borsani
Tommaso Treu
Steven L. Finkelstein
Takahiro Morishita
Nicha Leethochawalit
Charlotte Mason
Eduardo Bañados
Michele Trenti
Massimo Stiavelli
L. Y. Aaron Yung
Pablo Arrabal Haro
Rachel S. Somerville
Christian Soto
The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec
The Astrophysical Journal
High-redshift galaxies
Star formation
Reionization
Cosmology
Observational astronomy
title The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec
title_full The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec
title_fullStr The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec
title_full_unstemmed The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec
title_short The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec
title_sort borg jwst survey abundance and mass to light ratio of luminous z 7 9 galaxies from independent sight lines with nirspec
topic High-redshift galaxies
Star formation
Reionization
Cosmology
Observational astronomy
url https://doi.org/10.3847/1538-4357/adc67d
work_keys_str_mv AT sofiarojasruiz theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT micaelabagley theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT guidorobertsborsani theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT tommasotreu theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT stevenlfinkelstein theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT takahiromorishita theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT nichaleethochawalit theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT charlottemason theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT eduardobanados theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT micheletrenti theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT massimostiavelli theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT lyaaronyung theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT pabloarrabalharo theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT rachelssomerville theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT christiansoto theborgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT sofiarojasruiz borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT micaelabagley borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT guidorobertsborsani borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT tommasotreu borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT stevenlfinkelstein borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT takahiromorishita borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT nichaleethochawalit borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT charlottemason borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT eduardobanados borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT micheletrenti borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT massimostiavelli borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT lyaaronyung borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT pabloarrabalharo borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT rachelssomerville borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec
AT christiansoto borgjwstsurveyabundanceandmasstolightratioofluminousz79galaxiesfromindependentsightlineswithnirspec