ALMA 26 Arcmin2 Survey of GOODS-S at One Millimeter (ASAGAO): Average Morphology of High-z Dusty Star-forming Galaxies in an Exponential Disk (n ≃ 1)
暂无分享,去创建一个
Ichi Tanaka | Kotaro Kohno | Tao Wang | Yoshiaki Taniguchi | Bunyo Hatsukade | R. J. Ivison | Daniel Espada | Seiji Fujimoto | Masami Ouchi | Kouichiro Nakanishi | Takatoshi Shibuya | Yoshihiro Ueda | Ken-ichi Tadaki | J. S. Dunlop | Sune Toft | Taira Oogi | J. Dunlop | T. Nagao | K. Kohno | Y. Taniguchi | Y. Ueda | R. Ivison | M. Ouchi | Tao Wang | B. Hatsukade | K. Tadaki | I. Tanaka | Minju M. Lee | Y. Tamura | H. Umehata | Wei-hao Wang | S. Toft | W. Rujopakarn | D. Espada | Y. Ao | K. Nakanishi | S. Fujimoto | Yoichi Tamura | T. Shibuya | Yiping Ao | Tohru Nagao | T. Oogi | S. Inoue | Y. Yamaguchi | C. Gómez-Guijarro | Yuki Yamaguchi | Shigeki Inoue | Carlos Gómez-Guijarro | Hideki Umehata | Wiphu Rujopakarn | Wei-hao Wang | Shigeki Inoue
[1] David Crampton,et al. The Canada-United Kingdom Deep Submillimeter Survey. II. First Identifications, Redshifts, and Implications for Galaxy Evolution* , 1999 .
[2] N. Hathi,et al. Starburst Intensity Limit of Galaxies at z ≃ 5–6 , 2007, 0709.0520.
[3] J. Conway,et al. Stacking of large interferometric data sets in the image- and uv-domain - a comparative study , 2014, 1411.1410.
[4] R. Bouwens,et al. The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223 , 2016, 1607.03808.
[5] Andrew Hopkins,et al. Compact continuum source finding for next generation radio surveys , 2012, 1202.4500.
[6] S. Wuyts,et al. BULGE-FORMING GALAXIES WITH AN EXTENDED ROTATING DISK AT z ∼ 2 , 2016, 1608.05412.
[7] I. Smail,et al. SHARC-2 350 μm Observations of Distant Submillimeter-selected Galaxies , 2006, The Astrophysical Journal.
[8] J. Sérsic,et al. Influence of the atmospheric and instrumental dispersion on the brightness distribution in a galaxy , 1963 .
[9] Henry C. Ferguson,et al. The size evolution of high-redshift galaxies , 2004 .
[10] C. Steinhardt,et al. A Massive Dead Disk Galaxy in the Young Universe , 2017, Nature.
[11] Masami Ouchi,et al. MORPHOLOGIES OF ∼190,000 GALAXIES AT z = 0–10 REVEALED WITH HST LEGACY DATA. I. SIZE EVOLUTION , 2015, 1503.07481.
[12] D. Elbaz,et al. A simple model to interpret the ultraviolet, optical and infrared emission from galaxies , 2008, 0806.1020.
[13] A. Dekel,et al. An analytic solution for the minimal bathtub toy model: challenges in the star formation history of high-z galaxies , 2014, 1402.2283.
[14] A. Koekemoer,et al. GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR–MASS PLANE FROM z ∼ 2.5 TO z ∼ 0.1 , 2011, 1107.0317.
[15] Reinhard Genzel,et al. Spatially Resolved Millimeter Interferometry of SMM J02399–0136: A Very Massive Galaxy at z = 2.8 , 2002, astro-ph/0210449.
[16] G. Chabrier. Galactic Stellar and Substellar Initial Mass Function , 2003, astro-ph/0304382.
[17] M. C. Cooper,et al. High molecular gas fractions in normal massive star-forming galaxies in the young Universe , 2010, Nature.
[18] M. Oguri,et al. THE SIZES OF z ∼ 6–8 LENSED GALAXIES FROM THE HUBBLE FRONTIER FIELDS ABELL 2744 DATA , 2014, 1410.1535.
[19] J. Trump,et al. SUB-KILOPARSEC ALMA IMAGING OF COMPACT STAR-FORMING GALAXIES AT z ∼ 2.5: REVEALING THE FORMATION OF DENSE GALACTIC CORES IN THE PROGENITORS OF COMPACT QUIESCENT GALAXIES , 2016, 1607.01011.
[20] D. Elbaz,et al. VLA AND ALMA IMAGING OF INTENSE GALAXY-WIDE STAR FORMATION IN z ∼ 2 GALAXIES , 2016, The Astrophysical Journal.
[21] J. Brinchmann,et al. Hubble Space Telescope imaging of the CFRS and LDSS redshift surveys—IV. Influence of mergers in the evolution of faint field galaxies from z∼1 , 1999, astro-ph/9909211.
[22] K. Schawinski,et al. SUBMILLIMETER GALAXIES AS PROGENITORS OF COMPACT QUIESCENT GALAXIES , 2014, 1401.1510.
[23] Edinburgh,et al. THE SCUBA-2 COSMOLOGY LEGACY SURVEY: ALMA RESOLVES THE REST-FRAME FAR-INFRARED EMISSION OF SUB-MILLIMETER GALAXIES , 2014, The Astrophysical Journal.
[24] Observatoire de la Côte d'Azur,et al. Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties , 2016, 1609.04172.
[25] D. Elbaz,et al. Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 Gyr , 2016, 1601.04226.
[26] Garth D. Illingworth,et al. Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse , 2008, 0802.4094.
[27] S. Wuyts,et al. Rotating Starburst Cores in Massive Galaxies at z = 2.5 , 2017, 1703.10197.
[28] David Elbaz,et al. ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: SURVEY DESCRIPTION , 2016, 1607.06768.
[29] J. B. Oke,et al. Secondary standard stars for absolute spectrophotometry , 1983 .
[30] M. Ouchi,et al. Demonstrating a New Census of Infrared Galaxies with ALMA (DANCING-ALMA). I. FIR Size and Luminosity Relation at z = 0–6 Revealed with 1034 ALMA Sources , 2017, 1703.02138.
[31] John A. Peacock,et al. The Parkes selected regions: powerful radio galaxies and quasars at high redshifts , 1986 .
[32] D.Lutz,et al. PHIBSS: MOLECULAR GAS CONTENT AND SCALING RELATIONS IN z ∼ 1-3 MASSIVE, MAIN-SEQUENCE STAR-FORMING GALAXIES* , 2012 .
[33] D. Calzetti,et al. GOODS–Herschel: an infrared main sequence for star-forming galaxies , 2011, 1105.2537.
[34] M. Halpern,et al. An AzTEC 1.1 mm survey of the GOODS‐N field – II. Multiwavelength identifications and redshift distribution , 2009, 0906.4561.
[35] R. B. Barreiro,et al. Planck early results. XXI. Properties of the interstellar mediumin the Galactic plane , 2011, 1101.2032.
[36] S. M. Fall,et al. A Simple Model for the Absorption of Starlight by Dust in Galaxies , 2000, astro-ph/0003128.
[37] Chien Y. Peng,et al. STRUCTURAL PARAMETERS OF GALAXIES IN CANDELS , 2012, 1211.6954.
[38] J. Dunlop,et al. SXDF-ALMA 2 arcmin2 deep survey: Resolving and characterizing the infrared extragalactic background light down to 0.5 mJy , 2016, 1607.02331.
[39] C. C. Chen,et al. KILOPARSEC-SCALE DUST DISKS IN HIGH-REDSHIFT LUMINOUS SUBMILLIMETER GALAXIES , 2016, The Astrophysical Journal.
[40] J. Kneib,et al. Molecular gas content in strongly lensed z similar to 1.5-3 star-forming galaxies with low infrared luminosities , 2014, 1408.0816.
[41] V. A. Bruce,et al. The properties of (sub-)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-south , 2012, 1208.3464.
[42] Wolfgang Voges,et al. The size distribution of galaxies in the Sloan Digital Sky Survey , 2003, astro-ph/0301527.
[43] Chien Y. Peng,et al. DETAILED DECOMPOSITION OF GALAXY IMAGES. II. BEYOND AXISYMMETRIC MODELS , 2009, 0912.0731.
[44] Edinburgh,et al. AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: NEAR-INFRARED MORPHOLOGIES AND STELLAR SIZES , 2014, 1412.0668.
[45] D. Wake,et al. 3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE–MASS DISTRIBUTION SINCE z = 3 , 2014, 1404.2844.
[46] A. Cimatti,et al. Submillimeter Galaxies at z ~ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO-H2 Conversion Factor , 2008, 0801.3650.
[47] H. Bischof,et al. The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory , 2010, 1005.1487.
[48] S. J. Liu,et al. Herschel : the first science highlights Special feature L etter to the E ditor The Herschel-SPIRE instrument and its in-flight performance , 2010 .
[49] A. M. Swinbank,et al. The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies , 2011, 1112.0321.
[50] M. Oguri,et al. Size–Luminosity Relations and UV Luminosity Functions at z = 6–9 Simultaneously Derived from the Complete Hubble Frontier Fields Data , 2017, 1710.07301.
[51] Paul S. Smith,et al. The Multiband Imaging Photometer for Spitzer (MIPS) , 2004 .
[52] J. Trump,et al. CANDELS VISUAL CLASSIFICATIONS: SCHEME, DATA RELEASE, AND FIRST RESULTS , 2014, 1401.2455.
[53] D. Meier,et al. ALMA OBSERVATIONS OF THE SUBMILLIMETER DENSE MOLECULAR GAS TRACERS IN THE LUMINOUS TYPE-1 ACTIVE NUCLEUS OF NGC 7469 , 2015, 1508.05946.
[54] S. E. Persson,et al. THE FOURSTAR GALAXY EVOLUTION SURVEY (ZFOURGE): ULTRAVIOLET TO FAR-INFRARED CATALOGS, MEDIUM-BANDWIDTH PHOTOMETRIC REDSHIFTS WITH IMPROVED ACCURACY, STELLAR MASSES, AND CONFIRMATION OF QUIESCENT GALAXIES TO z ∼ 3.5 , 2016, 1608.07579.
[55] G. Bruzual,et al. Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.
[56] Research Center for the Early Universe,et al. COMPACT STARBURSTS IN z ∼ 3 ?> –6 SUBMILLIMETER GALAXIES REVEALED BY ALMA , 2014, The Astrophysical Journal.
[57] F. Walter,et al. AN ALMA SURVEY OF SUB-MILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: PHYSICAL PROPERTIES DERIVED FROM ULTRAVIOLET-TO-RADIO MODELING , 2015, 1504.04376.
[58] N. Hathi,et al. Starburst Intensity Limit of Galaxies at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[O , 2008 .
[59] D. Eisenstein,et al. MORPHOLOGY AND SIZE DIFFERENCES BETWEEN LOCAL AND HIGH-REDSHIFT LUMINOUS INFRARED GALAXIES , 2010, 1010.0675.
[60] N. Gehrels. Confidence limits for small numbers of events in astrophysical data , 1986 .
[61] Itziar Aretxaga,et al. The SCUBA HAlf Degree Extragalactic Survey – VI. 350-μm mapping of submillimetre galaxies , 2008 .
[62] Robert C. Kennicutt,et al. Secular Evolution and the Formation of Pseudobulges in Disk Galaxies , 2004, astro-ph/0407343.
[63] K. Ohta,et al. OPTICAL–INFRARED PROPERTIES OF FAINT 1.3 mm SOURCES DETECTED WITH ALMA , 2015, 1508.00644.
[64] Michele Cirasuolo,et al. EVOLUTION OF THE SIZES OF GALAXIES OVER 7 < z < 12 REVEALED BY THE 2012 HUBBLE ULTRA DEEP FIELD CAMPAIGN , 2012, 1212.3869.
[65] J. Dunlop,et al. Unveiling the nature of bright z ~ 7 galaxies with the Hubble Space Telescope , 2016, 1605.05325.
[66] H. Rix,et al. AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: SOURCE CATALOG AND MULTIPLICITY , 2013, 1304.4266.
[67] V. Springel,et al. The formation of massive, compact galaxies at z = 2 in the Illustris simulation , 2014, 1411.0667.
[68] J. Dunlop,et al. ALMA 26 arcmin2 Survey of GOODS-S at One-millimeter (ASAGAO): X-Ray AGN Properties of Millimeter-selected Galaxies , 2017, 1712.03350.
[69] M. Dickinson,et al. “Super-deblended” Dust Emission in Galaxies. I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6 , 2017, 1703.05281.
[70] S. Muller,et al. UVMULTIFIT: A versatile tool for fitting astronomical radio interferometric data , 2014, 1401.4984.
[71] J. Dunlop,et al. A near-infrared morphological comparison of high-redshift submillimetre and radio galaxies: massive star-forming discs versus relaxed spheroids , 2010, 1005.5176.
[72] B. Holwerda,et al. Herschel/SPIRE observations of the dusty disk of NGC 4244 , 2012, 1204.2936.
[73] F. Walter,et al. Cool Gas in High-Redshift Galaxies , 2013, 1301.0371.
[74] V. A. Bruce,et al. A deep ALMA image of the Hubble Ultra Deep Field , 2016, 1606.00227.
[75] H. Rix,et al. A massive galaxy in its core formation phase three billion years after the Big Bang , 2014, Nature.