GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

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Standard

GOODS-ALMA 2.0 : Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies. / Gomez-Guijarro, C.; Elbaz, D.; Xiao, M.; Bethermin, M.; Franco, M.; Magnelli, B.; Daddi, E.; Dickinson, M.; Demarco, R.; Inami, H.; Rujopakarn, W.; Magdis, G. E.; Shu, X.; Chary, R.; Zhou, L.; Alexander, D. M.; Bournaud, F.; Ciesla, L.; Ferguson, H. C.; Finkelstein, S. L.; Giavalisco, M.; Iono, D.; Juneau, S.; Kartaltepe, J. S.; Lagache, G.; Le Floc'h, E.; Leiton, R.; Lin, L.; Motohara, K.; Mullaney, J.; Okumura, K.; Pannella, M.; Papovich, C.; Pope, A.; Sargent, M. T.; Silverman, J. D.; Treister, E.; Wang, T.

I: Astronomy & Astrophysics, Bind 658, A43, 31.01.2022.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Gomez-Guijarro, C, Elbaz, D, Xiao, M, Bethermin, M, Franco, M, Magnelli, B, Daddi, E, Dickinson, M, Demarco, R, Inami, H, Rujopakarn, W, Magdis, GE, Shu, X, Chary, R, Zhou, L, Alexander, DM, Bournaud, F, Ciesla, L, Ferguson, HC, Finkelstein, SL, Giavalisco, M, Iono, D, Juneau, S, Kartaltepe, JS, Lagache, G, Le Floc'h, E, Leiton, R, Lin, L, Motohara, K, Mullaney, J, Okumura, K, Pannella, M, Papovich, C, Pope, A, Sargent, MT, Silverman, JD, Treister, E & Wang, T 2022, 'GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies', Astronomy & Astrophysics, bind 658, A43. https://doi.org/10.1051/0004-6361/202141615

APA

Gomez-Guijarro, C., Elbaz, D., Xiao, M., Bethermin, M., Franco, M., Magnelli, B., Daddi, E., Dickinson, M., Demarco, R., Inami, H., Rujopakarn, W., Magdis, G. E., Shu, X., Chary, R., Zhou, L., Alexander, D. M., Bournaud, F., Ciesla, L., Ferguson, H. C., ... Wang, T. (2022). GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies. Astronomy & Astrophysics, 658, [A43]. https://doi.org/10.1051/0004-6361/202141615

Vancouver

Gomez-Guijarro C, Elbaz D, Xiao M, Bethermin M, Franco M, Magnelli B o.a. GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies. Astronomy & Astrophysics. 2022 jan. 31;658. A43. https://doi.org/10.1051/0004-6361/202141615

Author

Gomez-Guijarro, C. ; Elbaz, D. ; Xiao, M. ; Bethermin, M. ; Franco, M. ; Magnelli, B. ; Daddi, E. ; Dickinson, M. ; Demarco, R. ; Inami, H. ; Rujopakarn, W. ; Magdis, G. E. ; Shu, X. ; Chary, R. ; Zhou, L. ; Alexander, D. M. ; Bournaud, F. ; Ciesla, L. ; Ferguson, H. C. ; Finkelstein, S. L. ; Giavalisco, M. ; Iono, D. ; Juneau, S. ; Kartaltepe, J. S. ; Lagache, G. ; Le Floc'h, E. ; Leiton, R. ; Lin, L. ; Motohara, K. ; Mullaney, J. ; Okumura, K. ; Pannella, M. ; Papovich, C. ; Pope, A. ; Sargent, M. T. ; Silverman, J. D. ; Treister, E. ; Wang, T. / GOODS-ALMA 2.0 : Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies. I: Astronomy & Astrophysics. 2022 ; Bind 658.

Bibtex

@article{b780a6b37c444f5e8907167442dbc56c,
title = "GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies",
abstract = "Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally occurs in compact regions smaller than the stellar distribution. However, it remains to be understood how systematic these findings are. Studies often lack homogeneity in the sample selection, target discontinuous areas with inhomogeneous sensitivities, and suffer from modest uv coverage coming from single array configurations. GOODS-ALMA is a 1.1 mm galaxy survey over a continuous area of 72.42 arcmin(2) at a homogeneous sensitivity. In this version 2.0, we present a new low resolution dataset and its combination with the previous high resolution dataset from the survey, improving the uv coverage and sensitivity reaching an average of sigma = 68.4 mu Jy beam(-1). A total of 88 galaxies are detected in a blind search (compared to 35 in the high resolution dataset alone), 50% at S/N-peak >= 5 and 50% at 3.5 1 mJy, compact dust continuum emission at 1.1 mm prevails, and sizes as extended as typical star-forming stellar disks are rare. The S-1.1mm < 1 mJy sources appear slightly more extended at 1.1 mm, although they are still generally compact below the sizes of typical star-forming stellar disks.",
keywords = "galaxies: evolution, galaxies: high-redshift, galaxies: photometry, galaxies: star formation, galaxies: structure, submillimeter: galaxies, DEEP FIELD-SOUTH, STAR-FORMING GALAXIES, GMASS ULTRADEEP SPECTROSCOPY, DEGREE EXTRAGALACTIC SURVEY, FAR-INFRARED PROPERTIES, SUBMILLIMETER GALAXIES, MASSIVE GALAXIES, PHYSICAL-PROPERTIES, LUMINOSITY FUNCTION, MAIN-SEQUENCE",
author = "C. Gomez-Guijarro and D. Elbaz and M. Xiao and M. Bethermin and M. Franco and B. Magnelli and E. Daddi and M. Dickinson and R. Demarco and H. Inami and W. Rujopakarn and Magdis, {G. E.} and X. Shu and R. Chary and L. Zhou and Alexander, {D. M.} and F. Bournaud and L. Ciesla and Ferguson, {H. C.} and Finkelstein, {S. L.} and M. Giavalisco and D. Iono and S. Juneau and Kartaltepe, {J. S.} and G. Lagache and {Le Floc'h}, E. and R. Leiton and L. Lin and K. Motohara and J. Mullaney and K. Okumura and M. Pannella and C. Papovich and A. Pope and Sargent, {M. T.} and Silverman, {J. D.} and E. Treister and T. Wang",
year = "2022",
month = jan,
day = "31",
doi = "10.1051/0004-6361/202141615",
language = "English",
volume = "658",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - GOODS-ALMA 2.0

T2 - Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

AU - Gomez-Guijarro, C.

AU - Elbaz, D.

AU - Xiao, M.

AU - Bethermin, M.

AU - Franco, M.

AU - Magnelli, B.

AU - Daddi, E.

AU - Dickinson, M.

AU - Demarco, R.

AU - Inami, H.

AU - Rujopakarn, W.

AU - Magdis, G. E.

AU - Shu, X.

AU - Chary, R.

AU - Zhou, L.

AU - Alexander, D. M.

AU - Bournaud, F.

AU - Ciesla, L.

AU - Ferguson, H. C.

AU - Finkelstein, S. L.

AU - Giavalisco, M.

AU - Iono, D.

AU - Juneau, S.

AU - Kartaltepe, J. S.

AU - Lagache, G.

AU - Le Floc'h, E.

AU - Leiton, R.

AU - Lin, L.

AU - Motohara, K.

AU - Mullaney, J.

AU - Okumura, K.

AU - Pannella, M.

AU - Papovich, C.

AU - Pope, A.

AU - Sargent, M. T.

AU - Silverman, J. D.

AU - Treister, E.

AU - Wang, T.

PY - 2022/1/31

Y1 - 2022/1/31

N2 - Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally occurs in compact regions smaller than the stellar distribution. However, it remains to be understood how systematic these findings are. Studies often lack homogeneity in the sample selection, target discontinuous areas with inhomogeneous sensitivities, and suffer from modest uv coverage coming from single array configurations. GOODS-ALMA is a 1.1 mm galaxy survey over a continuous area of 72.42 arcmin(2) at a homogeneous sensitivity. In this version 2.0, we present a new low resolution dataset and its combination with the previous high resolution dataset from the survey, improving the uv coverage and sensitivity reaching an average of sigma = 68.4 mu Jy beam(-1). A total of 88 galaxies are detected in a blind search (compared to 35 in the high resolution dataset alone), 50% at S/N-peak >= 5 and 50% at 3.5 1 mJy, compact dust continuum emission at 1.1 mm prevails, and sizes as extended as typical star-forming stellar disks are rare. The S-1.1mm < 1 mJy sources appear slightly more extended at 1.1 mm, although they are still generally compact below the sizes of typical star-forming stellar disks.

AB - Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally occurs in compact regions smaller than the stellar distribution. However, it remains to be understood how systematic these findings are. Studies often lack homogeneity in the sample selection, target discontinuous areas with inhomogeneous sensitivities, and suffer from modest uv coverage coming from single array configurations. GOODS-ALMA is a 1.1 mm galaxy survey over a continuous area of 72.42 arcmin(2) at a homogeneous sensitivity. In this version 2.0, we present a new low resolution dataset and its combination with the previous high resolution dataset from the survey, improving the uv coverage and sensitivity reaching an average of sigma = 68.4 mu Jy beam(-1). A total of 88 galaxies are detected in a blind search (compared to 35 in the high resolution dataset alone), 50% at S/N-peak >= 5 and 50% at 3.5 1 mJy, compact dust continuum emission at 1.1 mm prevails, and sizes as extended as typical star-forming stellar disks are rare. The S-1.1mm < 1 mJy sources appear slightly more extended at 1.1 mm, although they are still generally compact below the sizes of typical star-forming stellar disks.

KW - galaxies: evolution

KW - galaxies: high-redshift

KW - galaxies: photometry

KW - galaxies: star formation

KW - galaxies: structure

KW - submillimeter: galaxies

KW - DEEP FIELD-SOUTH

KW - STAR-FORMING GALAXIES

KW - GMASS ULTRADEEP SPECTROSCOPY

KW - DEGREE EXTRAGALACTIC SURVEY

KW - FAR-INFRARED PROPERTIES

KW - SUBMILLIMETER GALAXIES

KW - MASSIVE GALAXIES

KW - PHYSICAL-PROPERTIES

KW - LUMINOSITY FUNCTION

KW - MAIN-SEQUENCE

U2 - 10.1051/0004-6361/202141615

DO - 10.1051/0004-6361/202141615

M3 - Journal article

VL - 658

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A43

ER -

ID: 303677773