A Full Resolution of the 450 μm Extragalactic Background Light

Autor: Qi-Ning Hsu, L. L. Cowie, Chian-Chou Chen, A. J. Barger

Publikováno v: The Astrophysical Journal Letters, Vol 964, Iss 2, p L32 (2024)

The extragalactic background light (EBL) is the cumulative radiation outside the Milky Way. The determination of its corresponding primary emitting sources as well as its total energy level across the entire electromagnetic spectrum has profound impl

Externí odkaz: https://doaj.org/article/aa89494655d24f909a531724354f96cf

Confirmation of a Substantial Discrepancy between Radio and UV–IR Measures of the Star Formation Rate Density at 0.2 < z < 1.3

Autor: A. M. Matthews, D. D. Kelson, A. B. Newman, F. Camilo, J. J. Condon, W. D. Cotton, M. Dickinson, T. H. Jarrett, M. Lacy

Publikováno v: The Astrophysical Journal, Vol 966, Iss 2, p 194 (2024)

We present the initial sample of redshifts for 3839 galaxies in the MeerKAT DEEP2 field—the most sensitive ∼1.4 GHz radio field yet observed with σ _n = 0.55 μ Jy beam ^−1 , reaching the confusion limit. Using a spectrophotometric technique c

Externí odkaz: https://doaj.org/article/80055ff3c5374ee2bfdb659d5b87a959

HEROES: The Hawaii eROSITA Ecliptic Pole Survey Catalog

Autor: A. J. Taylor, A. J. Barger, L. L. Cowie, G. Hasinger, E. M. Hu, A. Songaila

Publikováno v: The Astrophysical Journal Supplement Series, Vol 266, Iss 2, p 24 (2023)

We present a seven-band ( g , r , i , z , y , NB816, NB921) catalog derived from a Subaru Hyper Suprime-Cam (HSC) imaging survey of the North Ecliptic Pole (NEP). The survey, known as HEROES, consists of 44 deg ^2 of contiguous imaging reaching media

Externí odkaz: https://doaj.org/article/be9515934f204b468aaf4ff94055c3f5

JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

Autor: Rogier A. Windhorst, Seth H. Cohen, Rolf A. Jansen, Jake Summers, Scott Tompkins, Christopher J. Conselice, Simon P. Driver, Haojing Yan, Dan Coe, Brenda Frye, Norman Grogin, Anton Koekemoer, Madeline A. Marshall, Rosalia O’Brien, Nor Pirzkal, Aaron Robotham, Russell E. Ryan Jr., Christopher N. A. Willmer, Timothy Carleton, Jose M. Diego, William C. Keel, Paolo Porto, Caleb Redshaw, Sydney Scheller, Stephen M. Wilkins, S. P. Willner, Adi Zitrin, Nathan J. Adams, Duncan Austin, Richard G. Arendt, John F. Beacom, Rachana A. Bhatawdekar, Larry D. Bradley, Tom Broadhurst, Cheng Cheng, Francesca Civano, Liang Dai, Hervé Dole, Jordan C. J. D’Silva, Kenneth J. Duncan, Giovanni G. Fazio, Giovanni Ferrami, Leonardo Ferreira, Steven L. Finkelstein, Lukas J. Furtak, Hansung B. Gim, Alex Griffiths, Heidi B. Hammel, Kevin C. Harrington, Nimish P. Hathi, Benne W. Holwerda, Rachel Honor, Jia-Sheng Huang, Minhee Hyun, Myungshin Im, Bhavin A. Joshi, Patrick S. Kamieneski, Patrick Kelly, Rebecca L. Larson, Juno Li, Jeremy Lim, Zhiyuan Ma, Peter Maksym, Giorgio Manzoni, Ashish Kumar Meena, Stefanie N. Milam, Mario Nonino, Massimo Pascale, Andreea Petric, Justin D. R. Pierel, Maria del Carmen Polletta, Huub J. A. Röttgering, Michael J. Rutkowski, Ian Smail, Amber N. Straughn, Louis-Gregory Strolger, Andi Swirbul, James A. A. Trussler, Lifan Wang, Brian Welch, J. Stuart B. Wyithe, Min Yun, Erik Zackrisson, Jiashuo Zhang, Xiurui Zhao

Publikováno v: The Astronomical Journal, Vol 165, Iss 1, p 13 (2022)

We give an overview and describe the rationale, methods, and first results from NIRCam images of the JWST “Prime Extragalactic Areas for Reionization and Lensing Science” (PEARLS) project. PEARLS uses up to eight NIRCam filters to survey several

Externí odkaz: https://doaj.org/article/6b7efde15f394593836702cfc97340de

The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years

Autor: M. S. Yun, Manuel Aravena, Nick Scoville, Ezequiel Treister, D. B. Sanders, Joaquin Vieira, David L. Clements, J. A. Hodge, Matthieu Béthermin, Jorge A. Zavala, Christopher C. Hayward, E. da Cunha, Anton M. Koekemoer, Kartik Sheth, Patrick Drew, Johannes Staguhn, Sune Toft, Kirsten Kraiberg Knudsen, Georgios E. Magdis, Sinclaire M. Manning, Arianna S. Long, Jeyhan S. Kartaltepe, Gergö Popping, Caitlin M. Casey, Steve Finkelstein, Allison W. S. Man, Seiji Fujimoto, Karina Caputi

Publikováno v: The Astrophysical Journal
The Astrophysical Journal, 2021, 909, 15 pp. ⟨10.3847/1538-4357/abdb27⟩
Astrophysical Journal, 909(2):165. IOP PUBLISHING LTD
The Astrophysical Journal, 909(2)
Zavala, J A, Casey, C M, Manning, S M, Aravena, M, Bethermin, M, Caputi, K I, Clements, D L, Cunha, E D, Drew, P, Finkelstein, S L, Fujimoto, S, Hayward, C, Hodge, J, Kartaltepe, J S, Knudsen, K, Koekemoer, A M, Long, A S, Magdis, G E, Man, A W S, Popping, G, Sanders, D, Scoville, N, Sheth, K, Staguhn, J, Toft, S, Treister, E, Vieira, J D & Yun, M S 2021, ' The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years ', Astrophysical Journal, vol. 909, no. 2, 165 . https://doi.org/10.3847/1538-4357/abdb27

We present the first results from the 2mm Mapping Obscuration to Reionization (MORA) survey, the largest ALMA contiguous blank-field survey to-date with a total area of 184 sq. arcmin and the only at 2mm to search for dusty star-forming galaxies (DSF

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b3c21f3e9d0d5ced6c1e9983c9cf717
https://hdl.handle.net/11370/2d1a729e-ce3e-4b10-b363-d482b944da60