SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Jed McKinney; Caitlin M. Casey; Arianna S. Long; Olivia R. Cooper; Sinclaire M. Manning; Maximilien Franco; Hollis Akin; Erini Lambrides; Elaine Gammon; Camila Silva; Fabrizio Gentile; Jorge A. Zavala; Aristeidis Amvrosiadis; Irham Taufik Andika; Malte Brinch; Jaclyn B. Champagne; Nima Chartab; Nicole E. Drakos; Andreas L. Faisst; Seiji Fujimoto; Steven Gillman; Ghassem Gozaliasl; Thomas R. Greve; Santosh Harish; Christopher C. Hayward; Michaela Hirschmann; Olivier Ilbert; Boris S. Kalita; Jeyhan S. Kartaltepe; Anton M. Koekemoer; Vasily Kokorev; Daizhong Liu; Georgios Magdis; Henry Joy McCracken; Jason Rhodes; Brant E. Robertson; Margherita Talia; Francesco Valentino; Aswin P. Vijayan

SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Jed McKinney, Caitlin M. Casey, Arianna S. Long, Olivia R. Cooper, Sinclaire M. Manning, Maximilien Franco, Hollis Akin, Erini Lambrides, Elaine Gammon, Camila Silva, Fabrizio Gentile, Jorge A. Zavala, Aristeidis Amvrosiadis, Irham Taufik Andika, Malte Brinch, Jaclyn B. Champagne, Nima Chartab, Nicole E. Drakos, Andreas L. Faisst, Seiji FujimotoSteven Gillman, Ghassem Gozaliasl, Thomas R. Greve, Santosh Harish, Christopher C. Hayward, Michaela Hirschmann, Olivier Ilbert, Boris S. Kalita, Jeyhan S. Kartaltepe, Anton M. Koekemoer, Vasily Kokorev, Daizhong Liu, Georgios Magdis, Henry Joy McCracken, Jason Rhodes, Brant E. Robertson, Margherita Talia, Francesco Valentino, Aswin P. Vijayan

Department of Computer Science

Research output: Contribution to journal › Article › Scientific

2 Downloads (Pure)

Abstract

JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter galaxies with detailed joint ALMA and JWST constraints in the COSMOS field. Sources are originally selected using the SCUBA-2 instrument and have archival ALMA observations from various programs. Their JWST NIRCam imaging is from COSMOS-Web and PRIMER. We extract multi-wavelength photometry in a manner that leverages the unprecedented near-infrared spatial resolution of JWST, and fit the data with spectral energy distribution models to derive photometric redshifts, stellar masses, star-formation rates and optical attenuation. The sample has an average z=2.6, A_V=2.5, SFR=270 and log(M*)=11.1. There are 81 (30%) galaxies that have no previous optical/near-infrared detections, including 75% of the z>4 sub-sample (n=28). The faintest observed near-infrared sources have the highest redshifts and largest A_V=4. In a preliminary morphology analysis we find that ~10% of our sample exhibit spiral arms and 5% host stellar bars, with one candidate bar found at z>3. Finally, we find that the clustering of JWST galaxies within 10 arcseconds of a sub-mm galaxy is a factor of 2 greater than what is expected based on either random clustering or the distribution of sources around any red galaxy irrespective of a sub-mm detection.

Original language	English
Journal	arXiv.org
Publication status	Accepted/In press - 1 Aug 2024
MoE publication type	B1 Non-refereed journal articles

Keywords

Astrophysics - Astrophysics of Galaxies

Access to Document

pdf

http://adsabs.harvard.edu/abs/2024arXiv240808346M

Cite this

McKinney, J., Casey, C. M., Long, A. S., Cooper, O. R., Manning, S. M., Franco, M., Akin, H., Lambrides, E., Gammon, E., Silva, C., Gentile, F., Zavala, J. A., Amvrosiadis, A., Andika, I. T., Brinch, M., Champagne, J. B., Chartab, N., Drakos, N. E., Faisst, A. L., ... Vijayan, A. P. (Accepted/In press). SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web. arXiv.org. http://adsabs.harvard.edu/abs/2024arXiv240808346M

@article{c8244fa3465c4c80b7b8b1400806a616,

title = "SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web",

abstract = "JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter galaxies with detailed joint ALMA and JWST constraints in the COSMOS field. Sources are originally selected using the SCUBA-2 instrument and have archival ALMA observations from various programs. Their JWST NIRCam imaging is from COSMOS-Web and PRIMER. We extract multi-wavelength photometry in a manner that leverages the unprecedented near-infrared spatial resolution of JWST, and fit the data with spectral energy distribution models to derive photometric redshifts, stellar masses, star-formation rates and optical attenuation. The sample has an average z=2.6, A_V=2.5, SFR=270 and log(M*)=11.1. There are 81 (30%) galaxies that have no previous optical/near-infrared detections, including 75% of the z>4 sub-sample (n=28). The faintest observed near-infrared sources have the highest redshifts and largest A_V=4. In a preliminary morphology analysis we find that ~10% of our sample exhibit spiral arms and 5% host stellar bars, with one candidate bar found at z>3. Finally, we find that the clustering of JWST galaxies within 10 arcseconds of a sub-mm galaxy is a factor of 2 greater than what is expected based on either random clustering or the distribution of sources around any red galaxy irrespective of a sub-mm detection.",

keywords = "Astrophysics - Astrophysics of Galaxies",

author = "Jed McKinney and Casey, {Caitlin M.} and Long, {Arianna S.} and Cooper, {Olivia R.} and Manning, {Sinclaire M.} and Maximilien Franco and Hollis Akin and Erini Lambrides and Elaine Gammon and Camila Silva and Fabrizio Gentile and Zavala, {Jorge A.} and Aristeidis Amvrosiadis and Andika, {Irham Taufik} and Malte Brinch and Champagne, {Jaclyn B.} and Nima Chartab and Drakos, {Nicole E.} and Faisst, {Andreas L.} and Seiji Fujimoto and Steven Gillman and Ghassem Gozaliasl and Greve, {Thomas R.} and Santosh Harish and Hayward, {Christopher C.} and Michaela Hirschmann and Olivier Ilbert and Kalita, {Boris S.} and Kartaltepe, {Jeyhan S.} and Koekemoer, {Anton M.} and Vasily Kokorev and Daizhong Liu and Georgios Magdis and McCracken, {Henry Joy} and Jason Rhodes and Robertson, {Brant E.} and Margherita Talia and Francesco Valentino and Vijayan, {Aswin P.}",

year = "2024",

month = aug,

day = "1",

language = "English",

journal = "arXiv.org",

issn = "2331-8422",

publisher = "Cornell University",

}

McKinney, J, Casey, CM, Long, AS, Cooper, OR, Manning, SM, Franco, M, Akin, H, Lambrides, E, Gammon, E, Silva, C, Gentile, F, Zavala, JA, Amvrosiadis, A, Andika, IT, Brinch, M, Champagne, JB, Chartab, N, Drakos, NE, Faisst, AL, Fujimoto, S, Gillman, S, Gozaliasl, G, Greve, TR, Harish, S, Hayward, CC, Hirschmann, M, Ilbert, O, Kalita, BS, Kartaltepe, JS, Koekemoer, AM, Kokorev, V, Liu, D, Magdis, G, McCracken, HJ, Rhodes, J, Robertson, BE, Talia, M, Valentino, F & Vijayan, AP 2024, 'SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web', arXiv.org. <http://adsabs.harvard.edu/abs/2024arXiv240808346M>

TY - JOUR

T1 - SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

AU - McKinney, Jed

AU - Casey, Caitlin M.

AU - Long, Arianna S.

AU - Cooper, Olivia R.

AU - Manning, Sinclaire M.

AU - Franco, Maximilien

AU - Akin, Hollis

AU - Lambrides, Erini

AU - Gammon, Elaine

AU - Silva, Camila

AU - Gentile, Fabrizio

AU - Zavala, Jorge A.

AU - Amvrosiadis, Aristeidis

AU - Andika, Irham Taufik

AU - Brinch, Malte

AU - Champagne, Jaclyn B.

AU - Chartab, Nima

AU - Drakos, Nicole E.

AU - Faisst, Andreas L.

AU - Fujimoto, Seiji

AU - Gillman, Steven

AU - Gozaliasl, Ghassem

AU - Greve, Thomas R.

AU - Harish, Santosh

AU - Hayward, Christopher C.

AU - Hirschmann, Michaela

AU - Ilbert, Olivier

AU - Kalita, Boris S.

AU - Kartaltepe, Jeyhan S.

AU - Koekemoer, Anton M.

AU - Kokorev, Vasily

AU - Liu, Daizhong

AU - Magdis, Georgios

AU - McCracken, Henry Joy

AU - Rhodes, Jason

AU - Robertson, Brant E.

AU - Talia, Margherita

AU - Valentino, Francesco

AU - Vijayan, Aswin P.

PY - 2024/8/1

Y1 - 2024/8/1

N2 - JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter galaxies with detailed joint ALMA and JWST constraints in the COSMOS field. Sources are originally selected using the SCUBA-2 instrument and have archival ALMA observations from various programs. Their JWST NIRCam imaging is from COSMOS-Web and PRIMER. We extract multi-wavelength photometry in a manner that leverages the unprecedented near-infrared spatial resolution of JWST, and fit the data with spectral energy distribution models to derive photometric redshifts, stellar masses, star-formation rates and optical attenuation. The sample has an average z=2.6, A_V=2.5, SFR=270 and log(M*)=11.1. There are 81 (30%) galaxies that have no previous optical/near-infrared detections, including 75% of the z>4 sub-sample (n=28). The faintest observed near-infrared sources have the highest redshifts and largest A_V=4. In a preliminary morphology analysis we find that ~10% of our sample exhibit spiral arms and 5% host stellar bars, with one candidate bar found at z>3. Finally, we find that the clustering of JWST galaxies within 10 arcseconds of a sub-mm galaxy is a factor of 2 greater than what is expected based on either random clustering or the distribution of sources around any red galaxy irrespective of a sub-mm detection.

AB - JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter galaxies with detailed joint ALMA and JWST constraints in the COSMOS field. Sources are originally selected using the SCUBA-2 instrument and have archival ALMA observations from various programs. Their JWST NIRCam imaging is from COSMOS-Web and PRIMER. We extract multi-wavelength photometry in a manner that leverages the unprecedented near-infrared spatial resolution of JWST, and fit the data with spectral energy distribution models to derive photometric redshifts, stellar masses, star-formation rates and optical attenuation. The sample has an average z=2.6, A_V=2.5, SFR=270 and log(M*)=11.1. There are 81 (30%) galaxies that have no previous optical/near-infrared detections, including 75% of the z>4 sub-sample (n=28). The faintest observed near-infrared sources have the highest redshifts and largest A_V=4. In a preliminary morphology analysis we find that ~10% of our sample exhibit spiral arms and 5% host stellar bars, with one candidate bar found at z>3. Finally, we find that the clustering of JWST galaxies within 10 arcseconds of a sub-mm galaxy is a factor of 2 greater than what is expected based on either random clustering or the distribution of sources around any red galaxy irrespective of a sub-mm detection.

KW - Astrophysics - Astrophysics of Galaxies

M3 - Article

SN - 2331-8422

JO - arXiv.org

JF - arXiv.org

ER -

SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Abstract

Keywords

Access to Document

Fingerprint

Cite this