论文信息 - ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 - 字舞流文

ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7

International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the University of Bonn; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the University of Cologne; FONDECYT [1140099]; U.S. National Science Foundation [AST-1312950]; ERC Advanced Investigator programme DUSTYGAL [321334]; Simons Foundation; NSF [AST-1009452, AST-1445357]; NASA HST from the Space Telescope Science Institute [AR-13906.001]; NASA [NAS5-26555]; Cottrell College Science Award - Research Corporation for Science Advancement; Commonwealth of Australia; National Science Foundation [PLR-1248097]; Kavli Foundation; Gordon and Betty Moore Foundation [GBMF 947]; [PHY-1125897]

J. E. Carlstrom | M. L. N. Ashby | D. P. Marrone | J. D. Vieira | M. Aravena | C. De Breuck | K. M. Menten | C. M. Bradford | S. C. Chapman | E. J. Murphy | K. M. Rotermund | M. Malkan | Y. Hezaveh | J. Carlstrom | J. Vieira | C. Fassnacht | A. Weiss | D. Narayanan | K. Menten | C. Breuck | M. Malkan | S. Chapman | E. Murphy | D. Marrone | Y. Hezaveh | A. Weiss | B. Gullberg | Chian-Chou Chen | S. Chapman | M. Ashby | M. Aravena | M. Béthermin | C. Bradford | T. Greve | C. Hayward | K. Litke | K. Phadke | K. Rotermund | J. Spilker | M. B'ethermin | M. Bothwell | M. Strandet | D. Cunningham | Jingzhe Ma | J. Sreevani | M. B'ethermin | A. H. Gonzalez | C. D. Fassnacht | M. L. Strandet | A. Weiss | M. S. Bothwell | D. J. M. Cunningham | Chian-Chou Chen | T. R. Greve | B. Gullberg | C. C. Hayward | K. Litke | J. Ma | T. Miller | D. Narayanan | K. A. Phadke | J. S. Spilker | J. Sreevani | T. Miller | J. Ma | A. Gonzalez | Anthony H. Gonzalez

[1] C. A. Oxborrow,et al. Planck2015 results , 2015, Astronomy & Astrophysics.

[2] R. Bouwens. High-Redshift Galaxy Surveys and the Reionization of the Universe , 2015, 1511.01133.

[3] W. Everett,et al. THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES FROM THE SPT SURVEY , 2016, 1603.05094.

[4] Andrei Mesinger,et al. Understanding the Epoch of Cosmic Reionization , 2016 .

[5] J. Carlstrom,et al. ALMA IMAGING AND GRAVITATIONAL LENS MODELS OF SOUTH POLE TELESCOPE—SELECTED DUSTY, STAR-FORMING GALAXIES AT HIGH REDSHIFTS , 2016, 1604.05723.

[6] R. Wilson,et al. The relationship between carbon monoxide abundance and visual extinction in interstellar clouds. , 1982 .

[7] M. Rosenman,et al. SUBMILLIMETER OBSERVATIONS OF MILLIMETER BRIGHT GALAXIES DISCOVERED BY THE SOUTH POLE TELESCOPE , 2012, 1206.4550.

[8] Jr.,et al. The Global Schmidt law in star forming galaxies , 1997, astro-ph/9712213.

[9] Adrian T. Lee,et al. ALMA REDSHIFTS OF MILLIMETER-SELECTED GALAXIES FROM THE SPT SURVEY: THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES , 2013, 1303.2726.

[10] Adrian T. Lee,et al. The 10 Meter South Pole Telescope , 2009, 0907.4445.

[11] P. D. Werf,et al. The molecular gas in Luminous Infrared Galaxies I: CO lines, extreme physical conditions, and their drivers , 2011, 1109.4176.

[12] C. Henkel,et al. Atomic carbon at redshift ~2.5 , 2005 .

[13] Gilles Chabrier,et al. The Galactic Disk Mass Function: Reconciliation of the Hubble Space Telescope and Nearby Determinations , 2003, astro-ph/0302511.

[14] P. Solomon,et al. Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies , 1998, astro-ph/9806377.

[15] Duc Truong Pham,et al. The Bees Algorithm: Modelling foraging behaviour to solve continuous optimization problems , 2009 .

[16] D. Stark. Galaxies in the First Billion Years After the Big Bang , 2016 .

[17] P. P. van der Werf,et al. ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: THE INFRARED EXCESS OF UV-SELECTED z = 2–10 GALAXIES AS A FUNCTION OF UV-CONTINUUM SLOPE AND STELLAR MASS , 2016, 1606.05280.

[18] D. Narayanan,et al. Dusty Star Forming Galaxies at High Redshift , 2014, 1402.1456.

[19] P. Goldsmith. Molecular Depletion and Thermal Balance in Dark Cloud Cores , 2000 .

[20] Liverpool John Moores University,et al. DETECTION OF ATOMIC CARBON [C ii] 158 μm AND DUST EMISSION FROM A z = 7.1 QUASAR HOST GALAXY , 2012, 1203.5844.

[21] C. Henkel,et al. Highly-excited CO emission in APM 08279+5255 at z = 3.9 , 2007, astro-ph/0702669.

[22] S. Meyer,et al. Dusty starburst galaxies in the early Universe as revealed by gravitational lensing , 2013, Nature.

[23] S. Okamura,et al. STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS , 2010, 1007.2961.

[24] P. P. van der Werf,et al. THE HERSCHEL COMPREHENSIVE (U)LIRG EMISSION SURVEY (HERCULES): CO LADDERS, FINE STRUCTURE LINES, AND NEUTRAL GAS COOLING , 2015, 1501.02985.

[25] J. Carlstrom,et al. SUB-KILOPARSEC IMAGING OF COOL MOLECULAR GAS IN TWO STRONGLY LENSED DUSTY, STAR-FORMING GALAXIES , 2015, 1508.07369.

[26] Adrian T. Lee,et al. EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg2 OF THE SPT-SZ SURVEY , 2013, 1306.3470.

[27] D. Narayanan,et al. A physical model for the [C II]-FIR deficit in luminous galaxies , 2016, 1601.05803.

[28] N. Scoville. STARBURST AND AGN CONNECTIONS AND MODELS , 2003 .

[29] B. Altieri,et al. A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34 , 2013, Nature.

[30] D. Benford,et al. A 158 μm [C ii] LINE SURVEY OF GALAXIES AT z ∼ 1–2: AN INDICATOR OF STAR FORMATION IN THE EARLY UNIVERSE , 2010, 1009.4216.

[31] J. Carlstrom,et al. The nature of the [C II] emission in dusty star-forming galaxies from the SPT survey , 2015, 1501.06909.

[32] P. S. Bunclark,et al. Astronomical Data Analysis Software and Systems , 2008 .

[33] Nanjing,et al. Molecular Gas in Extreme Star-Forming Environments: The Starbursts Arp 220 and NGC 6240 as Case Studies , 2006, astro-ph/0610378.

[34] Todd A. Thompson,et al. Radiation Pressure-supported Starburst Disks and Active Galactic Nucleus Fueling , 2005 .