相关论文: PEP: first Herschel probe of dusty galaxy evolutio…

The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4

We exploit the deep and extended far infrared data sets (at 70, 100 and 160 um) of the Herschel GTO PACS Evolutionary Probe (PEP) Survey, in combination with the HERschel Multi tiered Extragalactic Survey (HerMES) data at 250, 350 and 500…

宇宙学与河外天体物理 · 物理学 2015-06-15 C. Gruppioni , F. Pozzi , G. Rodighiero , I. Delvecchio , S. Berta , L. Pozzetti , G. Zamorani , P. Andreani , A. Cimatti , O. Ilbert , E. Le Floch , D. Lutz , B. Magnelli , L. Marchetti , P. Monaco , R. Nordon , S. Oliver , P. Popesso , L. Riguccini , I. Roseboom , D. J. Rosario , M. Sargent , M. Vaccari , B. Altieri , H. Aussel , A. Bongiovanni , J. Cepa , E. Daddi , H. Dominguez-Sanchez , D. Elbaz , N. Forster-Schreiber , R. Genzel , A. Iribarrem , M. Magliocchetti , R. Maiolino , A. Poglitsch , A. Perez Garcia , M. Sanchez-Portal , E. Sturm , L. Tacconi , I. Valtchanov , A. Amblard , V. Arumugam , M. Bethermin , J. Bock , A. Boselli , V. Buat , D. Burgarella , N. Castro-Rodriguez , A. Cava , P. Chanial , D. L. Clements , A. Conley , A. Cooray , C. D. Dowell , E. Dwek , S. Eales , A. Franceschini , J. Glenn , M. Griffin , E. Hatziminaoglou , E. Ibar , K. Isaak , R. J. Ivison , G. Lagache , L. Levenson , N. Lu , S. Madden , B. Maffei , G. Mainetti , H. T. Nguyen , B. O Halloran , M. J. Page , P. Panuzzo , A. Papageorgiou , C. P. Pearson , I. Perez-Fournon , M. Pohlen , D. Rigopoulou , M. Rowan-Robinson , B. Schulz , D. Scott , N. Seymour , D. L. Shupe , A. J. Smith , J. A. Stevens , M. Symeonidis , M. Trichas , K. E. Tugwell , L. Vigroux , L. Wang , G. Wright , C. K. Xu , M. Zemcov , S. Bardelli , M. Carollo , T. Contini , O. Le Fevre , S. Lilly , V. Mainieri , A. Renzini , M. Scodeggio , E. Zucca

Herschel unveils a puzzling uniformity of distant dusty galaxies

The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the…

宇宙学与河外天体物理 · 物理学 2015-05-19 D. Elbaz , H. S. Hwang , B. Magnelli , E. Daddi , H. Aussel , B. Altieri , A. Amblard , P. Andreani , V. Arumugam , R. Auld , T. Babbedge , S. Berta , A. Blain , J. Bock , A. Bongiovanni , A. Boselli , V. Buat , D. Burgarella , N. Castro-Rodriguez , A. Cava , J. Cepa , P. Chanial , R. -R. Chary , A. Cimatti , D. L. Clements , A. Conley , L. Conversi , A. Cooray , M. Dickinson , H. Dominguez , C. D. Dowell , J. S. Dunlop , E. Dwek , S. Eales , D. Farrah , N. Forster Schreiber , M. Fox , A. Franceschini , W. Gear , R. Genzel , J. Glenn , M. Griffin , C. Gruppioni , M. Halpern , E. Hatziminaoglou , E. Ibar , K. Isaak , R. J. Ivison , G. Lagache , D. Le Borgne , E. Le Floc'h , L. Levenson , N. Lu , D. Lutz , S. Madden , B. Maffei , G. Magdis , G. Mainetti , R. Maiolino , L. Marchetti , A. M. J. Mortier , H. T. Nguyen , R. Nordon , B. O'Halloran , K. Okumura , S. J. Oliver , A. Omont , M. J. Page , P. Panuzzo , A. Papageorgiou , C. P. Pearson , I. Perez Fournon , A. M. Perez Garcıa , A. Poglitsch , M. Pohlen , P. Popesso , F. Pozzi , J. I. Rawlings , D. Rigopoulou , L. Riguccini , D. Rizzo , G. Rodighiero , I. G. Roseboom , M. Rowan-Robinson , A. Saintonge , M. Sanchez-Portal , P. Santini , M. Sauvage , B. Schulz , Douglas Scott , N. Seymour , L. Shao , D. L. Shupe , A. J. Smith , J. A. Stevens , E. Sturm , M. Symeonidis , L. Tacconi , M. Trichas , K. E. Tugwell , M. Vaccari , I. Valtchanov , J. Vieira , L. Vigroux , L. Wang , R. Ward , G. Wright , C. K. Xu , M. Zemcov

Herschel PEP: The star-formation rates of 1.5<z<2.5 massive galaxies

The star formation rate (SFR) is a key parameter in the study of galaxy evolution. The accuracy of SFR measurements at z~2 has been questioned following a disagreement between observations and theoretical models. The latter predict SFRs at…

宇宙学与河外天体物理 · 物理学 2015-05-18 R. Nordon , D. Lutz , L. Shao , B. Magnelli , S. Berta , B. Altieri , P. Andreani , H. Aussel , A. Bongiovanni , A. Cava , J. Cepa , A. Cimatti , E. Daddi , H. Dominguez , D. Elbaz , N. M. Forster Schreiber , R. Genzel , A. Grazian , G. Magdis , R. Maiolino , A. M. Perez Garcia , A. Poglitsch , P. Popesso , F. Pozzi , L. Riguccini , G. Rodighiero , A. Saintonge , M. Sanchez-Portal , P. Santini , E. Sturm , L. Tacconi , I. Valtchanov , M. Wetzstein , E. Wieprecht

Evolution of the dusty infrared luminosity function from z=0 to z=2.3 using observations from Spitzer

We derive the evolution of the infrared (IR) luminosity function (LF) over the last 4/5ths of cosmic time, using deep 24um and 70um imaging of the GOODS North and South fields. We use an extraction technique based on prior source positions…

宇宙学与河外天体物理 · 物理学 2015-05-27 B. Magnelli , D. Elbaz , R. R. Chary , M. Dickinson , D. Le Borgne , D. T. Frayer , C. N. A. Willmer

The K20 survey. V The evolution of the near-IR Luminosity Function

We present the galaxy rest-frame near-IR Luminosity Function (LF) and its cosmic evolution to z=1.5 based on a spectroscopic survey of a magnitude limited sample of galaxies with Ks<20 (the K20 survey, Cimatti et al. 2002b). The LFs have…

天体物理学 · 物理学 2009-11-07 L. Pozzetti , A. Cimatti , G. Zamorani , E. Daddi , N. Menci , A. Fontana , A. Renzini , M. Mignoli , F. Poli , P. Saracco , T. Broadhurst , S. Cristiani , S. D'Odorico , E. Giallongo , R. Gilmozzi

Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6

We present a new determination of the evolving far-infrared galaxy luminosity function (FIR LF) and the resulting inferred evolution of dust-obscured star-formation rate density (SFRD) out to redshift z~6. To establish the evolving…

星系天体物理 · 物理学 2026-03-03 M. P. Koprowski , J. V. Wijesekera , J. S. Dunlop , K. Lisiecki , D. J. McLeod , R. J. McLure , M. J. Michałowski , M. Solar

Herschel-ATLAS Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies

Exploiting the Herschel-ATLAS Science Demonstration Phase (SDP) survey data, we have determined the luminosity functions (LFs) at rest-frame wavelengths of 100 and 250 micron and at several redshifts z>1, for bright sub-mm galaxies with…

宇宙学与河外天体物理 · 物理学 2015-05-30 A. Lapi , J. Gonzalez-Nuevo , L. Fan , A. Bressan , G. De Zotti , L. Danese , M. Negrello , L. Dunne , S. Eales , S. Maddox , R. Auld , M. Baes , D. G. Bonfield , S. Buttiglione , A. Cava , D. L. Clements , A. Cooray , A. Dariush , S. Dye , J. Fritz , D. Herranz , R. Hopwood , E. Ibar , R. Ivison , M. J. Jarvis , S. Kaviraj , M. Lopez-Caniego , M. Massardi , M. J. Michalowski , E. Pascale , M. Pohlen , E. Rigby , G. Rodighiero , S. Serjeant , D. J. B. Smith , P. Temi , J. Wardlow , P. van der Werf

Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?

Ly-alpha emitters (LAEs) are seen everywhere in the redshift domain from local to z~7. Far-infrared (FIR) counterparts of LAEs at different epochs could provide direct clues on dust content, extinction, and spectral energy distribution…

宇宙学与河外天体物理 · 物理学 2013-08-28 A. Bongiovanni , I. Oteo , J. Cepa , A. M. Perez Garcia , M. Sanchez-Portal , A. Ederoclite , J. A. L. Aguerri , E. J. Alfaro , B. Altieri , P. Andreani , M. T. Aparicio-Villegas , H. Aussel , N. Benitez , S. Berta , T. Broadhurst , J. Cabrera-Cano , F. J. Castander , A. Cava , M. Cervino , H. Chulani , A. Cimatti , D. Cristobal-Hornillos , E. Daddi , H. Dominguez , D. Elbaz , A. Fernandez-Soto , N. Forster Schreiber , R. Genzel , M. F. Gomez , R. M. Gonzalez Delgado , A. Grazian , C. Gruppioni , J. M. Herreros , S. Iglesias-Groth , L. Infante , D. Lutz , B. Magnelli , G. Magdis , R. Maiolino , I. Marquez , V. J. Martinez , J. Masegosa , M. Moles , A. Molino , R. Nordon , A. del Olmo , J. Perea , A. Poglitsch , P. Popesso , F. Pozzi , F. Prada , J. M. Quintana , L. Riguccini , G. Rodighiero , A. Saintonge , S. F. Sanchez , P. Santini , L. Shao , E. Sturm , L. Tacconi , I. Valtchanov

Tracing the cosmic growth of super massive black holes to z ~ 3 with Herschel

We study a sample of Herschel-PACS selected galaxies within the GOODS-South and the COSMOS fields in the framework of the PACS Evolutionary Probe (PEP) project. Starting from the rich multi-wavelength photometric data-sets available in both…

星系天体物理 · 物理学 2014-06-19 I. Delvecchio , C. Gruppioni , F. Pozzi , S. Berta , G. Zamorani , A. Cimatti , D. Lutz , D. Scott , C. Vignali , G. Cresci , A. Feltre , A. Cooray , M. Vaccari , J. Fritz , E. Le Floc'h , B. Magnelli , P. Popesso , S. Oliver , J. Bock , M. Carollo , T. Contini , O. Le Févre , S. Lilly , V. Mainieri , A. Renzini , M. Scodeggio

FIR measurements of Ly-$\alpha$ emitters at z$\lesssim$1.0: dust attenuation from PACS-\emph{Herschel}

One remaining open question regarding the physical properties of Ly$\alpha$ emitters (LAEs) is their dust content and its evolution with redshift. The variety of results is large and with those reported by now is difficult to establish…

宇宙学与河外天体物理 · 物理学 2015-05-30 I. Oteo , A. Bongiovanni , A. M. Pérez García , J. Cepa , A. Ederoclite , M. Sánchez-Portal , I. Pintos-Castro , D. Lutz , S. Berta , E. Le Floc'h , B. Magnelli , P. Popesso , F. Pozzi , L. Riguccini , B. Altieri , P. Andreani , H. Aussel , A. Cimatti , E. Daddi , D. Elbaz , N. Förster Schreiber , R. Genzel , R. Maiolino , A. Poglitsch , E. Sturm , L. Tacconi , I. Valtchanov

The Herschel Virgo Cluster Survey. XIX. Physical properties of low luminosity FIR sources at $z <$ 0.5

The Star formation rate (SFR) is a crucial parameter to investigate galaxy evolution. At low redshift the cosmic SFR density declines smoothly, and massive active galaxies become passive, reducing their star formation activity. This implies…

星系天体物理 · 物理学 2016-04-06 Ciro Pappalardo , Luca Bizzocchi , Jacopo Fritz , Alessandro Boselli , Mederic Boquien , Samuel Boissier , Maarten Baes , Laure Ciesla , Simone Bianchi , Marcel Clemens , Sebastien Viaene , George J. Bendo , Ilse De Looze , Matthew W. L. Smith , Jonathan Davies

The evolving far-IR galaxy luminosity function and dust-obscured star-formation rate density out to z~5

We present a new measurement of the evolving galaxy far-IR luminosity function (LF) extending out to redshifts z~5, with resulting implications for the level of dust-obscured star-formation density in the young Universe. To achieve this we…

星系天体物理 · 物理学 2019-10-25 M. P. Koprowski , J. S. Dunlop , M. J. Michałowski , K. E. K. Coppin , J. E. Geach , R. J. McLure , D. Scott , P. P. van der Werf

The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands

We present the redshift evolution of the restframe galaxy luminosity function (LF) in the red r', i', and z' bands as derived from the FORS Deep Field (FDF). Using the deep and homogeneous I-band selected dataset of the FDF we are able to…

天体物理学 · 物理学 2009-11-11 A. Gabasch , U. Hopp , G. Feulner , R. Bender , S. Seitz , R. P. Saglia , J. Snigula , N. Drory , I. Appenzeller , J. Heidt , D. Mehlert , S. Noll , A. Boehm , K. Jaeger , B. Ziegler

Panchromatic spectral energy distributions of Herschel sources

(abridged) Far-infrared Herschel photometry from the PEP and HerMES programs is combined with ancillary datasets in the GOODS-N, GOODS-S, and COSMOS fields. Based on this rich dataset, we reproduce the restframe UV to FIR ten-colors…

宇宙学与河外天体物理 · 物理学 2015-06-12 S. Berta , D. Lutz , P. Santini , S. Wuyts , D. Rosario , D. Brisbin , A. Cooray , A. Franceschini , C. Gruppioni , E. Hatziminaoglou , H. S. Hwang , E. Le Floc'h , B. Magnelli , R. Nordon , S. Oliver , M. J. Page , P. Popesso , L. Pozzetti , F. Pozzi , L. Riguccini , G. Rodighiero , I. Roseboom , Douglas Scott , M. Symeonidis , I. Valtchanov , M. Viero , L. Wang

Insights on star formation histories and physical properties of $1.2 \leq z \lesssim 4 $ Herschel-detected galaxies

We test the impact of using variable star forming histories (SFHs) and the use of the IR luminosity (LIR) as a constrain on the physical parameters of high redshift dusty star-forming galaxies. We explore in particular the stellar…

星系天体物理 · 物理学 2017-09-13 P. Sklias , D. Schaerer , D. Elbaz , M. Pannella , C. Schreiber , A. Cava

Spitzer Imaging of Strongly-Lensed Herschel-Selected Dusty Star Forming Galaxies

We present the rest-frame optical spectral energy distribution and stellar masses of six Herschel- selected gravitationally lensed dusty, star-forming galaxies (DSFGs) at 1 < z < 3. These galaxies were first identified with Herschel/SPIRE…

星系天体物理 · 物理学 2015-11-18 Brian Ma , Asantha Cooray , J. A. Calanog , H. Nayyeri , N. Timmons , C. Casey , M. Baes , S. Chapman , H. Dannerbauer , E. L. Da Cunha , G. De Zotti , L. Dunne , D. Farrah , Hai Fu , J. Gonzalez-Nuevo , G. Magdis , M. J. Michalowski , I. Oteo , D. A. Riechers , D. Scott , M. W. L. Smith , L. Wang , J. Wardlow , M. Vaccari , S. Viaene , J. D. Vieira , M. Vaccari

The Herschel census of infrared SEDs through cosmic time

Using Herschel data from the deepest SPIRE and PACS surveys (HerMES and PEP) in COSMOS and GOODS (N+S), we examine the dust properties of IR-luminous (L_IR>10^10 L_sun) galaxies at 0.1<z<2 and determine how these evolve with cosmic time.…

宇宙学与河外天体物理 · 物理学 2015-06-15 Myrto Symeonidis , M. Vaccari , S. Berta , M. J. Page , D. Lutz , V. Arumugam , H. Aussel , J. Bock , A. Boselli , V. Buat , P. L. Capak , D. L. Clements , A. Conley , L. Conversi , A. Cooray , C. D. Dowell , D. Farrah , A. Franceschini , E. Giovannoli , J. Glenn , M. Griffin , E. Hatziminaoglou , H. -S. Hwang , E. Ibar , O. Ilbert , R. J. Ivison , E. Le Floc'h , S. Lilly , J. S. Kartaltepe , B. Magnelli , G. Magdis , L. Marchetti , H. T. Nguyen , R. Nordon , B. O'Halloran , S. J. Oliver , A. Omont , A. Papageorgiou , H. Patel , C. P. Pearson , I. Perez-Fournon , M. Pohlen , P. Popesso , F. Pozzi , D. Rigopoulou , L. Riguccini , D. Rosario , I. G. Roseboom , M. Rowan-Robinson , M. Salvato , B. Schulz , Douglas Scott , N. Seymour , D. L. Shupe , A. J. Smith , I. Valtchanov , L. Wang , C. K. Xu , M. Zemcov , S. Wuyts

Galaxy evolution at low redshift? II. Number counts and optical identifications of faint IRAS sources

We analyse a Far InfraRed (FIR) catalogue of galaxies at 60 microns with a flux limit of approx. 110 mJy, extracted from a deep subsample of the IRAS Faint Source Survey. Monte-Carlo simulations and optical identification statistics are…

天体物理学 · 物理学 2007-05-23 E. Bertin , M. Dennefeld , M. Moshir

The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems

By making use of Herschel-PEP observations of the COSMOS and Extended Groth Strip fields, we have estimated the dependence of the clustering properties of FIR-selected sources on their 100um fluxes. Our analysis shows a tendency for the…

宇宙学与河外天体物理 · 物理学 2015-06-15 M. Magliocchetti , P. Popesso , D. Rosario , D. Lutz , H. Aussel , S. Berta , B. Altieri , P. Andreani , J. Cepa , H. Castaneda , A. Cimatti , D. Elbaz , R. Genzel , A. Grazian , C. Gruppioni , O. Ilbert , E. Le Floc'h , B. Magnelli , R. Maiolino , R. Nordon , A. Poglitsch , F. Pozzi , L. Riguccini , G. Rodighiero , M. Sanchez-Portal , P. Santini , N. M. Forster Schreiber , E. Sturm , L. Tacconi , I. Valtchanov

Far-infrared And Nebular Star-formation Rates Of Dusty Star Forming Galaxies From Herschel And 3d-hst At Z~1

We present results of a multi-band Spectral Energy Distribution (SED) and nebular emission line analysis of a sample of 1147 spectroscopically identified dusty star-forming galaxies at 0.49 < z < 2.24 from Herschel/SPIRE and HST/WFC3 grism…

星系天体物理 · 物理学 2018-10-24 Farhanul Hasan , Hooshang Nayyeri , Asantha C. Cooray