يعرض 1 - 10 نتائج من 284 نتيجة بحث عن '"MASSIVE GALAXIES"', وقت الاستعلام: 0.77s تنقيح النتائج
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    دورية أكاديمية

    المساهمون: Particle Physics and Astrophysics

    وصف الملف: application/pdf

    العلاقة: We thank the anonymous referee for invaluable feedback that improved the paper greatly. We thank Anthony Holloway, Sotirios Sanidas, and Phil Perry for critical and timely help with computer infrastructure that made this work possible. We acknowledge support from the ERC Advanced Investigator Grant EPOCHS (788113), as well as a studentship from STFC. L.F. acknowledges financial support from Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior-Brazil (CAPES) in the form of a PhD studentship. D.I. acknowledges support by the European Research Council via ERC Consolidator Grant KETJU (Co. 818930). C.C.L. acknowledges support from the Royal Society under grant RGF/EA/181016. C.T. acknowledges funding from the Science and Technology Facilities Council (STFC). This work is based on observations made with the NASA/ESA Hubble Space Telescope (HST) and NASA/ESA/CSA James Webb Space Telescope (JWST) obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST, and NAS 5-26555 for HST. The specific observations analyzed can be accessed via doi:10.17909/ xm8m-tt59.; Ferreira , L , Conselice , C J , Sazonova , E , Ferrari , F , Caruana , J , Tohill , C-B , Lucatelli , G , Adams , N , Irodotou , D , Marshall , M A , Roper , W J , Lovell , C C , Verma , A , Austin , D , Trussler , J & Wilkins , S M 2023 , ' The JWST Hubble Sequence : The Rest-frame Optical Evolution of Galaxy Structure at 1.5 < z < 6.5 ' , Astrophysical Journal , vol. 955 , no. 2 , 94 . https://doi.org/10.3847/1538-4357/acec76Test; ORCID: /0000-0003-2946-8080/work/153474688; 85173932154; e2a5eb21-01d2-4bba-936f-5c2e18895b5b; http://hdl.handle.net/10138/571170Test; 001071729200001

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    دورية أكاديمية

    المساهمون: Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)

    المصدر: ISSN: 0004-6361.

    العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2308.14489; hal-04245687; https://hal.science/hal-04245687Test; https://hal.science/hal-04245687/documentTest; https://hal.science/hal-04245687/file/aa46732-23.pdfTest; ARXIV: 2308.14489; INSPIRE: 2691599

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    مؤتمر
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    دورية أكاديمية

    المساهمون: Department of Physics

    وصف الملف: application/pdf

    العلاقة: We thank the referee for their constructive comments, which helped contextualize the manuscript with other works and clarify the message. J.M. would like to thank C. Williams for making the SED of COS-3 mm-1 readily available, and the NRAO/ALMA Helpdesk team for making archival data easy to access. This work is based [in part] on observations made with the NASA/ESA/CSA JWST. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program ID 1727. Support for program 1727 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. This paper makes use of the following ALMA data: ADS/JAO.ALMA:2013.1.00118.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under a cooperative agreement by Associated Universities, Inc. This work used the CANDIDE computer system at the IAP supported by grants from the PNCG, CNES, and the DIM-ACAV and maintained by S. Rouberol.; McKinney , J , Manning , S M , Cooper , O R , Long , A S , Akins , H , Casey , C M , Faisst , A L , Franco , M , Hayward , C C , Lambrides , E , Magdis , G , Whitaker , K E , Yun , M , Champagne , J B , Drakos , N E , Gentile , F , Gillman , S , Gozaliasl , G , Ilbert , O , Jin , S , Koekemoer , A M , Kokorev , V , Liu , D , Rich , R M , Robertson , B E , Valentino , F , Weaver , J R , Zavala , J A , Allen , N , Kartaltepe , J S , McCracken , H J , Paquereau , L , Rhodes , J , Shuntov , M & Toft , S 2023 , ' A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web ' , Astrophysical Journal , vol. 956 , no. 2 , 72 . https://doi.org/10.3847/1538-4357/acf614Test; c629d5ff-dbfb-40c6-a66c-0cfd46f1345f; http://hdl.handle.net/10138/567335Test; 001083672600001

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    دورية أكاديمية
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    دورية أكاديمية

    المصدر: Ciesla , L , Gomez-Guijarro , C , Buat , V , Elbaz , D , Jin , S , Bethermin , M , Daddi , E , Franco , M , Inami , H , Magdis , G , Magnelli , B & Xiao , M 2023 , ' GOODS-ALMA 2.0 : Last gigayear star formation histories of the so-called starbursts within the main sequence ' , Astronomy & Astrophysics , vol. 672 , A191 . https://doi.org/10.1051/0004-6361/202245376Test

    وصف الملف: application/pdf

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    دورية أكاديمية

    المصدر: Jacobs , C , Glazebrook , K , Calabro , A , Treu , T , Nannayakkara , T , Jones , T , Merlin , E , Abraham , R , Stevens , A R H , Vulcani , B , Yang , L , Bonchi , A , Boyett , K , Bradac , M , Castellano , M , Fontana , A , Marchesini , D , Malkan , M , Mason , C , Morishita , T , Paris , D , Santini , P , Trenti , M & Wang , X 2023 , ....

    وصف الملف: application/pdf

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    دورية أكاديمية

    المصدر: McKinney , J , Finnerty , L , Casey , C M , Franco , M , Long , A S , Fujimoto , S , Zavala , J A , Cooper , O , Akins , H , Pope , A , Armus , L , Soifer , B T , Larson , K , Matthews , K , Melbourne , J & Cushing , M 2023 , ' Broad Emission Lines in Optical Spectra of Hot, Dust-obscured Galaxies Can Contribute Significantly to JWST/NIRCam Photometry ' , Astrophysical Journal Letters , vol. 946 , no. 2 , 39 ....

    وصف الملف: application/pdf

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    دورية أكاديمية
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    دورية أكاديمية

    المصدر: Kokorev , V , Jin , S , Magdis , G E , Caputi , K I , Valentino , F , Dayal , P , Trebitsch , M , Brammer , G , Fujimoto , S , Bauer , F , Iani , E , Kohno , K , Sese , D B , Gomez-Guijarro , C , Rinaldi , P & Navarro-Carrera , R 2023 , ' JWST Insight into a Lensed HST-dark Galaxy and Its Quiescent Companion at z=2.58 ' , Astrophysical Journal Letters , vol. 945 , no. 2 , 25 . https://doi.org/10.3847/2041-8213/acbd9dTest

    وصف الملف: application/pdf