Zobrazeno 1 - 10
of 93
pro vyhledávání: '"Steven P. Willner"'
Autor:
Rafael Ortiz III, Rogier A. Windhorst, Seth H. Cohen, Steven P. Willner, Rolf A. Jansen, Timothy Carleton, Patrick S. Kamieneski, Michael J. Rutkowski, Brent M. Smith, Jake Summers, Cheng Cheng, Dan Coe, Christopher J. Conselice, Jose M. Diego, Simon P. Driver, Jordan C. J. D’Silva, Brenda L. Frye, Hansung B. Gim, Norman A. Grogin, Heidi B. Hammel, Nimish P. Hathi, Benne W. Holwerda, Minhee Hyun, Myungshin Im, William C. Keel, Anton M. Koekemoer, Juno Li, Madeline A. Marshall, Tyler J. McCabe, Noah J. McLeod, Stefanie N. Milam, Rosalia O’Brien, Nor Pirzkal, Aaron S. G. Robotham, Russell E. Ryan Jr., Christopher N. A. Willmer, Haojing Yan, Min S. Yun, Adi Zitrin
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 258 (2024)
The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as seen in the longer-wavelength filters. We visually identified a sample of 66 galaxies (
Externí odkaz:
https://doaj.org/article/40b70f48947e4a0d892f9aa2e2d11536
Autor:
A. Maragkoudakis, Steven P. Willner, P. Bonfini, K. Kouroumpatzakis, Matthew L. N. Ashby, Paul H. Sell, A. Zezas, Thomas H. Jarrett
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:3079-3097
We present new H$\alpha$ photometry for the Star-Formation Reference Survey (SFRS), a representative sample of star-forming galaxies in the local Universe. Combining these data with the panchromatic coverage of the SFRS, we provide calibrations of H$
Autor:
Wolfgang Brandner, A. Jiménez-Rosales, Mark Gurwell, Stefan Hippler, Christian Straubmeier, Th. Henning, Fiona A. Harrison, Jason Dexter, N. M. Förster Schreiber, F. Vincent, Pierre Kervella, Daryl Haggard, S. Yazici, Silvia Scheithauer, Oliver Pfuhl, Y. Dallilar, T. Taro Shimizu, Idel Waisberg, Odele Straub, K. Foster, Felix Widmann, Sera Markoff, Dieter Lutz, J.-B. Le Bouquin, M. Bauböck, Matthew Horrobin, Yann Clénet, P. T. de Zeeuw, Gabriele Ghisellini, Howard A. Smith, Frederick K. Baganoff, Daniel Stern, Thibaut Paumard, Eckhard Sturm, Ric Davies, M. Nowak, Andreas Eckart, Andreas Kaufer, Sebastian Rabien, Laurent Jocou, Paulo J. V. Garcia, Ekkehard Wieprecht, Reinhard Genzel, Jinyi Shangguan, G. Rodríguez-Coira, Patrick Lowrance, C. J. Hailey, Thomas Ott, S. Zhang, A. Drescher, G. Ponti, Giovanni G. Fazio, Steven P. Willner, S. D. von Fellenberg, Linda J. Tacconi, Maryam Habibi, H. Bonnet, Julien Woillez, V. Lapeyrère, Sylvestre Lacour, António Amorim, Erich Wiezorrek, Xavier Haubois, Guy Perrin, J. Neilsen, K. Mori, Eric Gendron, Frank Eisenhauer, G. Heißel, Pierre Léna, Joseph L. Hora, Karine Perraut, Charles F. Gammie, Feng Gao, G. Witzel, Gérard Zins, Mark Morris, André Young, Julia Stadler, Jean-Phillipe Berger, Hope Boyce, Stefan Gillessen, Lieselotte Jochum, Roberto Abuter
Publikováno v:
Astronomy and Astrophysics, 654, 1-18
Astronomy & Astrophysics, 654:A22. EDP Sciences
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A22. ⟨10.1051/0004-6361/202140981⟩
Astronomy & Astrophysics
Astronomy & Astrophysics, 654:A22. EDP Sciences
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A22. ⟨10.1051/0004-6361/202140981⟩
Astronomy & Astrophysics
We report the time-resolved spectral analysis of a bright near-infrared and moderate X-ray flare of Sgr A*. We obtained light curves in the $M$-, $K$-, and $H$-bands in the mid- and near-infrared and in the $2-8~\mathrm{keV}$ and $2-70~\mathrm{keV}$
Autor:
Howard A. Smith, Rubén Herrero-Illana, Andrea M. Ghez, Nicola Marchili, Tuan Do, Hope Boyce, Mark Gurwell, Mark Morris, Giovanni G. Fazio, Daryl Haggard, Zhiyuan Li, J. A. Zensus, Steven P. Willner, M. Subroweit, Joseph L. Hora, Andreas Eckart, G. Witzel, E. E. Becklin, Gregory D. Martinez, Jun Liu
Sagittarius A* (Sgr A*) is the variable radio, near-infrared (NIR), and X-ray source associated with accretion onto the Galactic center black hole. We have analyzed a comprehensive submillimeter (including new observations simultaneous with NIR monit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c1788398bc669b1188e2aba006b34ee
http://hdl.handle.net/20.500.12386/31788
http://hdl.handle.net/20.500.12386/31788
Autor:
P. Bonfini, Konstantinos Kovlakas, A. Zezas, Steven P. Willner, Thomas H. Jarrett, Paul H. Sell, A. Maragkoudakis, Matthew L. N. Ashby, K. Kouroumpatzakis
Publikováno v:
Web of Science
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
X-ray luminosity ($L_X$) originating from high-mass X-ray binaries (HMXBs) is tightly correlated with the host galaxy's star-formation rate (SFR). We explore this connection at sub-galactic scales spanning ${\sim}$7 dex in SFR and ${\sim}$8 dex in sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3668b04d437a002247ce838d29cbb79c
http://arxiv.org/abs/2004.09873
http://arxiv.org/abs/2004.09873
Autor:
Steven P. Willner, Zohreh Ghaffari, Roberto De Propris, Hendrik Hildebrandt, Michael J. West, Rolf Chini, Martin Haas, Marco Chiaberge
To properly understand the evolution of high-redshift galaxy clusters, both passive and star-forming galaxies have to be considered. Here we study the clustering environment of 21 radio galaxies and quasars at 1 1.6, red overdensities at 1.2
Com
Com
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc92070429ebc28cc776ca874f836cb2
Autor:
Giovanni G. Fazio, Howard A. Smith, Joseph L. Hora, Sera Markoff, Mark Morris, Steven P. Willner, J. Neilsen, G. Witzel, Gabriele Ponti, Daryl Haggard, Hope Boyce, E. E. Becklin, Frederick K. Baganoff, Patrick J. Lowrance
Publikováno v:
Astrophys J
The Astrophysical journal, vol 871, iss 2
Astrophysical Journal, 871(2):161. IOP Publishing Ltd.
The Astrophysical journal, vol 871, iss 2
Astrophysical Journal, 871(2):161. IOP Publishing Ltd.
Emission from Sgr A* is highly variable at both X-ray and infrared (IR) wavelengths. Observations over the last ~20 years have revealed X-ray flares that rise above a quiescent thermal background about once per day, while faint X-ray flares from Sgr
Autor:
Smriti Mahajan, Somak Raychaudhury, Steven P. Willner, Giovanni G. Fazio, Andreas Zezas, A. Maragkoudakis, M. L. N. Ashby, Pauline Barmby
Publikováno v:
Physics and Astronomy Publications
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We present multi-wavelength global star formation rate (SFR) estimates for 326 galaxies from the Star Formation Reference Survey (SFRS) in order to determine the mutual scatter and range of validity of different indicators. The widely used empirical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::230131d0248f79f575efd65ef0e8abcc
https://ir.lib.uwo.ca/physicspub/56
https://ir.lib.uwo.ca/physicspub/56
Autor:
Giovanni G. Fazio, Sandra M. Faber, Audrey Galametz, Mauro Giavalisco, Steven P. Willner, Michael Peth, Carmen Eliche Moral, Lihwai Lin, Nestor Espino Briones, Dale D. Kocevski, Mauro Stefanon, Jeffrey A. Newman, Timothy Dolch, Janine Pforr, Ray A. Lucas, Nicolás Cardiel, Mara Salvato, Antonio Hernán-Caballero, Jennifer L. Donley, Marco Castellano, Gabriel Brammer, Guillermo Barro, Norman A. Grogin, David C. Koo, Anton M. Koekemoer, Pablo G. Pérez-González, Mark Dickinson, Andrea Grazian, Kyoung-Soo Lee, Stijn Wuyts, Helena Domínguez-Sánchez, Dritan Kodra, Kirpal Nandra, Henry C. Ferguson, Steve Finkelstein, Jonathan R. Trump, Jonathan P. Gardner, Belén Alcalde Pampliega, Elizabeth J. McGrath, Christopher J. Conselice, Bahram Mobasher, Matthew L. N. Ashby, Yicheng Guo, Arjen van der Wel, P. Esquej, Hooshang Nayyeri, Tommy Wiklind, Adriano Fontana, Antonio Cava, Eric Gawiser, L. Rodríguez-Muñoz, Nimish P. Hathi, Marc Rafelski, Viraj Pandya, Shoubaneh Hemmati
Publikováno v:
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
2019, ' The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates ', The Astrophysical Journal Supplement Series, vol. 243, no. 2, pp. 22 . https://doi.org/10.3847/1538-4365/ab23f2
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series, 243(2), 22
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
2019, ' The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates ', The Astrophysical Journal Supplement Series, vol. 243, no. 2, pp. 22 . https://doi.org/10.3847/1538-4365/ab23f2
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series, 243(2), 22
We present a WFC3 F160W ($H$-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts and stellar parameters derived from the analysis of the multi-wavelength
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::888fc6cea59a33f04f35eaab998b6801
https://hdl.handle.net/1854/LU-8624499
https://hdl.handle.net/1854/LU-8624499
Autor:
Klaus Meisenheimer, Steven P. Willner, Peter Barthel, Rolf Chini, Joanna Kuraszkiewicz, Belinda Jane Wilkes, Martin Haas, P. Podigachoski, Ralf Siebenmorgen, C. Westhues, Christian Leipski
Publikováno v:
The Astronomical Journal, 151(5), 120-172. IOP PUBLISHING LTD
Using the Herschel Space Observatory we have observed a representative sample of 87 powerful 3CR sources at redshift z < 1. The far-infrared (FIR, 70-500 micron) photometry is combined with mid-infrared (MIR) photometry from the Wide-Field Infrared S