ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar mass, and star formation rate from z=1 to z=5

被引：0

作者：

Jolly, Jean-Baptiste ^{[1
,2
]}

Knudsen, Kirsten ^{[2
]}

Laporte, Nicolas ^{[3
]}

Guerrero, Andrea ^{[4
]}

Fujimoto, Seiji ^{[5
,6
]}

Kohno, Kotaro ^{[7
,8
]}

Kokorev, Vasily ^{[9
]}

Lagos, Claudia del P. ^{[10
]}

Schirmer, Thiebaut-Antoine ^{[2
]}

Bauer, Franz ^{[11
,12
,13
]}

Dessauge-Zavadsky, Miroslava ^{[14
]}

Espada, Daniel ^{[15
,16
]}

Hatsukade, Bunyo ^{[7
]}

Koekemoer, Anton M. ^{[17
]}

Richard, Johan ^{[18
]}

Sun, Fengwu ^{[19
]}

Wu, John F. ^{[17
,20
]}

机构：

[1] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[2] Chalmers Univ Technol, Dept Space Earth & Environm, SE-412 96 Gothenburg, Sweden

[3] Aix Marseille Univ, CNRS, CNES, LAM Lab Astrophys Marseille,UMR 7326, F-13388 Marseille, France

[4] Univ Concepcion, Astron Dept, Barrio Univ S-N, Concepcion, Chile

[5] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[6] Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, DK-2200 Copenhagen N, Denmark

[7] Univ Tokyo, Inst Astron, Grad Sch Sci, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan

[8] Univ Tokyo, Grad Sch Sci, Res Ctr Early Universe, 7-3-1 Hongo,Bunkyo ku, Tokyo 1130033, Japan

[9] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands

[10] Univ Western Australia, Int Ctr Radio Astron Res ICRAR, M468 35 Stirling Hwy, Crawley, WA 6009, Australia

[11] Pontificia Univ Catolica Chile, Fac Educ, Campus San Joaquin Av Vicuna Mackenna 4860, Santiago 7820436, Chile

[12] Pontificia Univ Catolica Chile, Fac Educ, Campus San Joaquin,Av Vicuna Mackenna 4860, Santiago 7820436, Chile

[13] Millennium Inst Astrophys, Nuncio Monsenor Sotero Sanz 100,104, Santiago, Chile

[14] Univ Geneva, Observ Geneve, 51 Ch Maillettes, CH-1290 Versoix, Switzerland

[15] Univ Granada, Dept Fis Teor & Cosmos, Campus Fuentenueva,Edificio Mecenas, E-18071 Granada, Spain

[16] Univ Granada, Fac Ciencias, Granada 18071, Spain

[17] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[18] Univ Lyon 1, CRAL, Observ Lyon, 9 Ave Ch Andre, F-69561 St Genis Laval, France

[19] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[20] Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2025年 / 693卷

基金：

瑞典研究理事会;

关键词：

dust; extinction; galaxies: evolution; galaxies: ISM; galaxies: statistics; SPECTRAL ENERGY-DISTRIBUTIONS; ULTRA DEEP FIELD; SPECTROSCOPIC SURVEY; INTERSTELLAR-MEDIUM; FORMING GALAXIES; MOLECULAR GAS; TO-GAS; PHYSICAL-PROPERTIES; EVOLUTION; METALLICITY;

D O I：

10.1051/0004-6361/202346239

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Context. Understanding the dust content of galaxies, its evolution with redshift and its relation to stars and star formation is fundamental for our understanding of galaxy evolution. Dust acts as a catalyst of star formation and as a shield for star light. Advanced millimeter facilities like ALMA have made dust observation ever more accessible, even at high redshift. However, dust emission is typically very faint, making the use of stacking techniques is instrumental in the study of dust in statistically sound samples. Aims. Using the ALMA Lensing Cluster Survey (ALCS) wide-area band-6 continuum dataset (similar to 110 arcmin(2) across 33 lensing clusters), we constrain the dust-mass evolution with redshift, stellar mass, and star formation rate (SFR). Methods. After binning sources according to redshift, SFR, and stellar mass as extracted from an HST-IRAC catalog, we performed a set of continuum-stacking analyses in the image domain using LINESTACKER on sources between z = 1 and z = 5, which further improved the depth of our data. The large field of view provided by the ALCS allowed us to reach a final sample of similar to 4000 galaxies with known coordinates and SED-derived physical parameters. We stacked sources with an SFR between 10(-3) and 10(3) M-circle dot per year and a stellar mass between 10(8) and 10(12) M-circle dot, and we split them into different stellar mass and SFR bins. Through stacking, we retrieved the continuum 1.2 mm flux, which is a known dust-mass tracer. This allowed us to derive the dust-mass evolution with redshift and its relation to the SFR and stellar mass. Results. We clearly detect the continuum in most of the subsamples. From the nondetections, we derive 3 sigma upper limits. We observe a steady decline in the average dust mass with redshift. Moreover, sources with a higher stellar mass or SFR have a higher dust mass on average. This allows us to derive scaling relations. Our results mostly agree well with models at z similar to 1-3, but they indicate a typically lower dust mass than predicted at higher redshift.

引用

页数：12

共 85 条

[11] Molecular gas in distant galaxies from ALMA studies [J].

Combes, Francoise .

ASTRONOMY AND ASTROPHYSICS REVIEW, 2018, 26

[12] AN ALMA SURVEY OF SUB-MILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: PHYSICAL PROPERTIES DERIVED FROM ULTRAVIOLET-TO-RADIO MODELING [J].

da Cunha, E. ;

Walter, F. ;

Smail, I. R. ;

Swinbank, A. M. ;

Simpson, J. M. ;

Decarli, R. ;

Hodge, J. A. ;

Weiss, A. ;

van der Werf, P. P. ;

Bertoldi, F. ;

Chapman, S. C. ;

Cox, P. ;

Danielson, A. L. R. ;

Dannerbauer, H. ;

Greve, T. R. ;

Ivison, R. J. ;

Karim, A. ;

Thomson, A. .

ASTROPHYSICAL JOURNAL, 2015, 806 (01)

[13] ON THE EFFECT OF THE COSMIC MICROWAVE BACKGROUND IN HIGH-REDSHIFT (SUB-)MILLIMETER OBSERVATIONS [J].

da Cunha, Elisabete ;

Groves, Brent ;

Walter, Fabian ;

Decarli, Roberto ;

Weiss, Axel ;

Bertoldi, Frank ;

Carilli, Chris ;

Daddi, Emanuele ;

Elbaz, David ;

Ivison, Rob ;

Maiolino, Roberto ;

Riechers, Dominik ;

Rix, Hans-Walter ;

Sargent, Mark ;

Smail, Ian .

ASTROPHYSICAL JOURNAL, 2013, 766 (01)

[14] New insight into the relation between star formation activity and dust content in galaxies [J].

da Cunha, Elisabete ;

Eminian, Celine ;

Charlot, Stephane ;

Blaizot, Jeremy .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 403 (04) :1894-1908

[15] Dust masses, PAH abundances, and starlight intensities in the SINGS galaxy sample [J].

Draine, B. T. ;

Dale, D. A. ;

Bendo, G. ;

Gordon, K. D. ;

Smith, J. D. T. ;

Armus, L. ;

Engelbracht, C. W. ;

Helou, G. ;

Kennicutt, R. C., Jr. ;

Li, A. ;

Roussel, H. ;

Walter, F. ;

Calzetti, D. ;

Moustakas, J. ;

Murphy, E. J. ;

Rieke, G. H. ;

Bot, C. ;

Hollenbach, D. J. ;

Sheth, K. ;

Teplitz, H. I. .

ASTROPHYSICAL JOURNAL, 2007, 663 (02) :866-894

[16]

Draine BT, 2011, PR S ASTROP, P1

[17] GAMA/G10-COSMOS/3D-HST: the 0 < z < 5 cosmic star formation history, stellar-mass, and dust-mass densities [J].

Driver, Simon P. ;

Andrews, Stephen K. ;

da Cunha, Elisabete ;

Davies, Luke J. ;

Lagos, Claudia ;

Robotham, Aaron S. G. ;

Vinsen, Kevin ;

Wright, Angus H. ;

Alpaslan, Mehmet ;

Bland-Hawthorn, Joss ;

Bourne, Nathan ;

Brough, Sarah ;

Bremer, Malcolm N. ;

Cluver, Michelle ;

Colless, Matthew ;

Conselice, Christopher J. ;

Dunne, Loretta ;

Eales, Steve A. ;

Gomez, Haley ;

Holwerda, Benne ;

Hopkins, Andrew M. ;

Kafle, Prajwal R. ;

Kelvin, Lee S. ;

Loveday, Jon ;

Liske, Jochen ;

Maddox, Steve J. ;

Phillipps, Steven ;

Pimbblet, Kevin ;

Rowlands, Kate ;

Sansom, Anne E. ;

Taylor, Edward ;

Wang, Lingyu ;

Wilkins, Stephen M. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 475 (03) :2891-2935

[18] Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS [J].

Dudzeviciute, U. ;

Smail, Ian ;

Swinbank, A. M. ;

Lim, C-F ;

Wang, W-H ;

Simpson, J. M. ;

Ao, Y. ;

Chapman, S. C. ;

Chen, C-C ;

Clements, D. ;

Dannerbauer, H. ;

Ho, L. C. ;

Hwang, H. S. ;

Koprowski, M. ;

Lee, C-H ;

Scott, D. ;

Shim, H. ;

Shirley, R. ;

Toba, Y. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 500 (01) :942-961

[19] An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies [J].

Dudzeviciute, U. ;

Smail, Ian ;

Swinbank, A. M. ;

Stach, S. M. ;

Almaini, O. ;

da Cunha, E. ;

An, Fang Xia ;

Arumugam, V ;

Birkin, J. ;

Blain, A. W. ;

Chapman, S. C. ;

Chen, C-C ;

Conselice, C. J. ;

Coppin, K. E. K. ;

Dunlop, J. S. ;

Farrah, D. ;

Geach, J. E. ;

Gullberg, B. ;

Hartley, W. G. ;

Hodge, J. A. ;

Ivison, R. J. ;

Maltby, D. T. ;

Scott, D. ;

Simpson, C. J. ;

Simpson, J. M. ;

Thomson, A. P. ;

Walter, F. ;

Wardlow, J. L. ;

Weiss, A. ;

van der Werf, P. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 494 (03) :3828-3860

[20] Metallicity effects on dust properties in starbursting galaxies [J].

Engelbracht, C. W. ;

Rieke, G. H. ;

Gordon, K. D. ;

Smith, J. -D. T. ;

Werner, M. W. ;

Moustakas, J. ;

Willmer, C. N. A. ;

Vanzi, L. .

ASTROPHYSICAL JOURNAL, 2008, 678 (02) :804-827

← 1 2 3 4 5 6 7 8 9 →