Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS★
暂无分享,去创建一个
S. Maddox | B. Altieri | S. Serjeant | E. Pascale | M. Jarvis | J. Vieira | A. Bolatto | D. Riechers | I. Smail | M. Gurwell | D. Smith | B. Swinyard | J. Carpenter | G. Zotti | D. Scott | M. Baes | R. Lupu | D. Benford | L. Dunne | D. Frayer | C. Pearson | P. D. Werf | S. Eales | M. Michałowski | H. Dannerbauer | R. Auld | A. Cooray | H. Gomez | M. Pohlen | E. Rigby | M. Vaccari | D. Rigopoulou | I. Valtchanov | A. Dariush | R. Ivison | M. Negrello | L. Conversi | E. D. Cunha | E. Ibar | A. Cava | G. Rodighiero | M. S. Portal | S. Dye | R. Hopwood | L. Leeuw | S. Buttiglione | J. Fritz | P. Temi | M. Birkinshaw | M. Thompson | A. Marston | D. Coia | J. Virdee | D. Clements | L. Leeuw | M. Thompson | D. Scott | P. Werf | D. Scott | D. Smith | D. Scott | Mattia Vaccari
[1] S. Maddox,et al. MEASUREMENTS OF CO REDSHIFTS WITH Z-SPEC FOR LENSED SUBMILLIMETER GALAXIES DISCOVERED IN THE H-ATLAS SURVEY , 2010, 1009.5983.
[2] E. Kontar,et al. RELATIONSHIP BETWEEN HARD AND SOFT X-RAY EMISSION COMPONENTS OF A SOLAR FLARE , 2010, 1012.4346.
[3] P. P. van der Werf,et al. SPITZER IMAGING OF HERSCHEL-ATLAS GRAVITATIONALLY LENSED SUBMILLIMETER SOURCES , 2010, 1011.4940.
[4] S. Maddox,et al. GREEN BANK TELESCOPE ZPECTROMETER CO(1–0) OBSERVATIONS OF THE STRONGLY LENSED SUBMILLIMETER GALAXIES FROM THE HERSCHEL ATLAS , 2010, 1009.2194.
[5] P. P. van der Werf,et al. The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies , 2010, Science.
[6] S. Maddox,et al. Herschel-ATLAS: First data release of the Science Demonstration Phase source catalogues , 2010, 1010.5787.
[7] S. Maddox,et al. The first release of data from the Herschel ATLAS: the SPIRE images , 2010, 1010.5782.
[8] S. Bamford,et al. Herschel-ATLAS: the far-infrared-radio correlation at z < 0.5 , 2010, 1009.5390.
[9] 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.
[10] S. Maddox,et al. H-ATLAS : PACS imaging for the Science Demonstration Phase , 2010, 1009.0262.
[11] Bonn,et al. The properties of the interstellar medium within a star-forming galaxy at z= 2.3 , 2010, Monthly Notices of the Royal Astronomical Society.
[12] F. Walter,et al. [CII] line emission in BRI 1335-0417 at z = 4.4 , 2010, 1008.1578.
[13] Marc Ferlet,et al. In-orbit performance of the Herschel/SPIRE imaging Fourier transform spectrometer , 2010, Astronomical Telescopes + Instrumentation.
[14] C. Carilli,et al. A MASSIVE MOLECULAR GAS RESERVOIR IN THE z = 5.3 SUBMILLIMETER GALAXY AzTEC-3 , 2010, 1008.0389.
[15] S. Bamford,et al. Herschel–ATLAS: counterparts from the ultraviolet–near-infrared in the science demonstration phase catalogue , 2010, 1007.5260.
[16] S. Ott,et al. Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.
[17] H. Roussel,et al. In-flight calibration of the Herschel-SPIRE instrument , 2010, 1005.5073.
[18] 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 .
[19] M. Sauvage,et al. The effects of star formation on the low-metallicity ISM: NGC 4214 mapped with Herschel/PACS spectroscopy , 2010, 1005.1942.
[20] A. Cimatti,et al. The far-infrared/radio correlation as probed by Herschel , 2010, 1005.1072.
[21] K. Coppin,et al. Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3 , 2010, 1005.1071.
[22] G. J. Stacey,et al. FIRST DETECTION OF THE [O iii] 88 μm LINE AT HIGH REDSHIFTS: CHARACTERIZING THE STARBURST AND NARROW-LINE REGIONS IN EXTREME LUMINOSITY SYSTEMS , 2010, 1003.4296.
[23] Harvard,et al. Intense star formation within resolved compact regions in a galaxy at z = 2.3 , 2010, Nature.
[24] C. Tucker,et al. DETECTION OF THE 158 μm [C ii] TRANSITION AT z = 1.3: EVIDENCE FOR A GALAXY-WIDE STARBURST , 2010, 1003.2174.
[25] R. Davé,et al. IMAGING THE MOLECULAR GAS IN A SUBMILLIMETER GALAXY AT z = 4.05: COLD MODE ACCRETION OR A MAJOR MERGER? , 2010, 1002.3838.
[26] A. M. Swinbank,et al. Gas, dust and stars in the SCUBA galaxy, SMM J02399−0136: the EVLA reveals a colossal galactic nursery , 2009, 0912.1591.
[27] S. Maddox,et al. The Herschel ATLAS , 2009, 0910.4279.
[28] J. Dunlop,et al. Deep multi-frequency radio imaging in the Lockman Hole â II. The spectral index of submillimetre galaxies: The radio spectral index of sub-mm galaxies , 2010 .
[29] Mark Clampin,et al. Space telescopes and instrumentation 2012 : optical, infrared, and millimeter wave : 1-6 July 2012, Amsterdam, Netherlands , 2010 .
[30] Gunma Astronomical Observatory,et al. Properties of active galactic star-forming regions probed by imaging spectroscopy with the Fourier transform spectrometer (FTS) onboard AKARI , 2009, 0911.3409.
[31] Testing PDR models against ISO fine structure line data for extragalactic sources , 2010, 1001.4035.
[32] R. Rosenfeld. Nature , 2009, Otolaryngology--head and neck surgery : official journal of American Academy of Otolaryngology-Head and Neck Surgery.
[33] Jens Hjorth,et al. Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly , 2009, 0905.4499.
[34] C. De Breuck,et al. Strong (CII) emission at high redshift , 2009, 0904.3793.
[35] Itziar Aretxaga,et al. Over half of the far-infrared background light comes from galaxies at z ≥ 1.2 , 2009, Nature.
[36] N. Abel,et al. DUST-BOUNDED ULTRALUMINOUS INFRARED GALAXIES: MODEL PREDICTIONS FOR INFRARED SPECTROSCOPIC SURVEYS , 2009, 0903.4643.
[37] D. Elbaz,et al. A CO EMISSION LINE FROM THE OPTICAL AND NEAR-IR UNDETECTED SUBMILLIMETER GALAXY GN10 , 2009, 0903.3046.
[38] F. Walter,et al. A kiloparsec-scale hyper-starburst in a quasar host less than 1 gigayear after the Big Bang , 2009, Nature.
[39] D. Elbaz,et al. TWO BRIGHT SUBMILLIMETER GALAXIES IN A z = 4.05 PROTOCLUSTER IN GOODS-NORTH, AND ACCURATE RADIO-INFRARED PHOTOMETRIC REDSHIFTS , 2008, 0810.3108.
[40] F. Walter,et al. A SENSITIVE SEARCH FOR [N ii]205 μm EMISSION IN A z = 6.4 QUASAR HOST GALAXY , 2008, 0812.3956.
[41] P. S. Bunclark,et al. Astronomical Data Analysis Software and Systems , 2008 .
[42] G. Helou,et al. A Compendium of Far-Infrared Line and Continuum Emission for 227 Galaxies Observed by the Infrared Space Observatory , 2008, 0805.2930.
[43] 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.
[44] Thomas Henning,et al. The Photodetector Array Camera and Spectrometer (PACS) for the Herschel Space Observatory , 2004, Astronomical Telescopes + Instrumentation.
[45] David A. Naylor,et al. Apodizing functions for Fourier transform spectroscopy , 2007 .
[46] C. Baccigalupi,et al. Astrophysical and cosmological information from large-scale submillimetre surveys of extragalactic sources , 2007, astro-ph/0703210.
[47] R. Meijerink,et al. Diagnostics of irradiated dense gas in galaxy nuclei. II. A grid of XDR and PDR models , 2006, astro-ph/0610360.
[48] A. Stark,et al. Detection of the 205 μm [N II] Line from the Carina Nebula , 2006, astro-ph/0610636.
[49] University of Sydney,et al. The Link between Submillimetre Galaxies and Luminous Ellipticals: Near-Infrared IFU Spectroscopy of Submillimetre Galaxies , 2006 .
[50] Bruce M. Swinyard,et al. Performance evaluation of the Herschel/SPIRE imaging Fourier transform spectrometer through ground-based measurements , 2006, SPIE Astronomical Telescopes + Instrumentation.
[51] F. Bertoldi,et al. High-Resolution Millimeter Imaging of Submillimeter Galaxies , 2005 .
[52] First detection of [CII]158 μm at high redshift : vigorous star formation in the early universe , 2005, astro-ph/0508064.
[53] R. Maiolino,et al. Improved Templates for Photometric Redshifts of Submillimeter Sources , 2005, astro-ph/0505128.
[54] Edinburgh,et al. An interferometric CO survey of luminous submillimetre galaxies , 2005 .
[55] Alessandro Bressan,et al. Can the faint submillimetre galaxies be explained in the Λ cold dark matter model , 2005 .
[56] D. Mesa,et al. Predictions for high-frequency radio surveys of extragalactic sources , 2004, astro-ph/0410709.
[57] C. Kramer,et al. Emission of CO, C i, and C ii in W3 Main , 2004, astro-ph/0406141.
[58] M. Wolfire,et al. The [C II] 158 Micron Line Deficit in Ultraluminous Infrared Galaxies Revisited , 2003, astro-ph/0305520.
[59] S. Malhotra,et al. ISO LWS Observations of the Two Nearby Spiral Galaxies NGC 6946 and NGC 1313 , 2002, astro-ph/0204241.
[60] S. Malhotra,et al. Far-Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium , 2001, astro-ph/0106485.
[61] Effects of Massive Star Formation on the ISM of Dwarf Galaxies , 2000, astro-ph/0002046.
[62] G. J. Stacey,et al. ISO Far-IR spectroscopy of IR-bright galaxies and ULIRGs , 1999 .
[63] NASA Ames Research Center,et al. Far-Infrared and Submillimeter Emission from Galactic and Extragalactic Photodissociation Regions , 1999, astro-ph/9907255.
[64] David Crampton,et al. The Canada-United Kingdom Deep Submillimeter Survey. II. First Identifications, Redshifts, and Implications for Galaxy Evolution* , 1999 .
[65] Alexander G. G. M. Tielens,et al. Dense Photodissociation Regions (PDRs) , 1997 .
[66] I. Smail,et al. A Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution , 1997, astro-ph/9708135.
[67] A. Blain. Galaxy—galaxy gravitational lensing in the millimetre/submillimetre waveband , 1996 .
[68] Kenneth R. Sembach,et al. INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE , 1996 .
[69] Richard L. White,et al. The FIRST Survey: Faint Images of the Radio Sky at twenty centimeters , 1995 .
[70] A. Poglitsch,et al. The 158 micron forbidden C II line - A measure of global star formation activity in galaxies , 1991 .
[71] A. Tielens,et al. Physical Conditions in Photodissociation Regions - Application to Galactic Nuclei , 1990 .
[72] R. Rubin. The Effect of Density Variations on Elemental Abundance Ratios in Gaseous Nebulae , 1989 .
[73] Charles H. Townes,et al. Far-infrared spectroscopy of galaxies - The 158 micron C(+) line and the energy balance of molecular clouds , 1985 .
[74] R. Rubin. Models of H II regions - Heavy element opacity, variation of temperature , 1985 .
[75] È. Roueff,et al. Fine-structure excitation of ground-state C+ ions by hydrogen atoms , 1977 .