Results 81 to 90 of about 36,712 (229)
Extragalactic Results from the Infrared Space Observatory
, 2000 More than a decade ago the IRAS satellite opened the realm of external
galaxies for studies in the 10 to 100 micron band and discovered emission from
tens of thousands of normal and active galaxies.Acosta-Pulido JA, Afonso C, Alexander T, Altieri B, Alton PB, Aussel H, Aussel H, Awaki H, Binette L, Boller T, Boselli A, Boselli A, Boulade O, Braine J, Catherine J. Cesarsky, Cesarsky CJ, Cesarsky D, Cesarsky D, Chapman SC, Clavel J, Clegg PE, Clements DL, Contursi A, de Graauw T, Desert FX, Desert FX, Doherty RM, Duley WW, Efstathiou A, Elbaz D, Fadda D, Fischer J, Flores H, Franceschini A, Gilmore G, Haas M, Haas M, Haas M, Hippelein H, Kawara K, Kegel WH, Kessler MF, Knapp GR, Krügel E, Kunze D, Lagache G, Lagache G, Lagache G, Lai O, Laureijs RJ, Laurent O, Laurent O, Lemke D, Lemonon L, Lord SD, Lutz D, Lutz D, Lutz D, Lutz D, Mattila K, Mattila K, Metcalfe L, Mirabel IF, Mirabel IF, Moorwood AFM, Moorwood AFM, Najarro F, Nakagawa T, Oliva E, Pagani L, Pfenniger D, Puget JL, Puget JL, Radovich M, Reinhard Genzel, Rigopoulou D, Rigopoulou D, Rigopoulou D, Rodriguez Espinosa JM, Rouan D, Roussel H, Rowan-Robinson M, Schaerer D, Scott D, Scoville NZ, Serjeant S, Siebenmorgen R, Stickel M, Sturm E, Sturm E, Taniguchi Y, Taniguchi Y, Tecza M, Thornley MD, Tran DQ, Tuffs RJ, Unger SJ, Valentijn EA, Verstraete L, Viegas SM, Vignati P, Vigroux L, Walter R, Wilkes BJ +103 morecore +1 more sourceStatistics of associations among IR galaxies [PDF]
In the course of expanding the search of Kleinmann et. al. (1988) for distant, infrared-luminous objects, the authors noticed (as is often remarked) that a large number of infrared-selected galaxies have close neighbors or show merger characteristics (e ...Gallimore, Jack F., Keel, William C.core +1 more sourceEnvironmental Dependence of Local Luminous Infrared Galaxies
, 2010 We study the environmental dependence of local luminous infrared galaxies
(LIRGs) and ultraluminous infrared galaxies (ULIRGs) found in the Sloan Digital
Sky Survey (SDSS) data.Abazajian, Allam, Baldwin, Balogh, Bitsakis, Blanton, Blanton, Brinchmann, Bruzual, C. Park, Capak, Cardelli, Carlberg, Chary, Chen, Choi, Colless, Cooper, D. Elbaz, Dasyra, Elbaz, Falco, Farrah, Feruglio, Gallazzi, Genzel, Gilli, Goto, Gómez, H. M. Lee, H. S. Hwang, Hill, Hill, Hopkins, Hwang, Hwang, Hwang, Ideue, J. C. Lee, Jeong, Kauffmann, Kauffmann, Kennicutt, Kennicutt, Kewley, Kewley, Kim, Koulouridis, Le Floc’h, Le Floc’h, Lee, Lewis, Li, Lotz, M. G. Lee, Magnelli, Marcillac, Murakami, Murphy, Neugebauer, Noeske, Noeske, Owers, Park, Park, Park, Park, Park, Patel, Sanders, Shi, Shi, Slinglend, Soifer, Stoughton, Sutherland, Tanaka, Tran, Tremonti, Veilleux, Veilleux, Veilleux, W.-S. Jeong, Wang, Wang, Wang, Wegner, Wegner, York, Yuan, Zauderer +90 morecore +1 more sourceSMILES Initial Data Release: Unveiling the Obscured Universe with MIRI Multiband Imaging
The Astrophysical JournalThe James Webb Space Telescope is revolutionizing our view of the Universe through unprecedented sensitivity and resolution in the infrared, with some of the largest gains realized at its longest wavelengths.Stacey Alberts, Jianwei Lyu, Irene Shivaei, George H. Rieke, Pablo G. Pérez-González, Nina Bonaventura, Yongda Zhu, Jakob M. Helton, Zhiyuan Ji, Jane Morrison, Brant E. Robertson, Meredith A. Stone, Yang Sun, Christina C. Williams, Christopher N. A. Willmer +14 moredoaj +1 more sourceEXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM AHERSCHEL/PACS STUDY OF THE GOALS SAMPLE [PDF]
, 2013 T. Díaz-Santos, L. Armus, V. Charmandaris, Sabrina Stierwalt, Edward J. Murphy, S. Haan, Hanae Inami, Sangeeta Malhotra, R. Meijerink, G. J. Stacey, Andreea Petric, A. Evans, Sylvain Veilleux, P. van der Werf, S. Lord, N. Lu, Justin Howell, P. N. Appleton, J. M. Mazzarella, J. A. Surace, C. K. Xu, B. Schulz, D. B. Sanders, Carrie Bridge, B. Chan, D. T. Frayer, K. Iwasawa, J. Melbourne, E. Sturm +28 moreopenalex +1 more sourceThe Average Physical Properties and Star Formation Histories of the
UV-Brightest Star-Forming Galaxies at z~3.7
, 2011 [Abridged] We investigate the average physical properties and star formation
histories of the most UV-luminous star-forming galaxies at z~3.7. Our results
are derived from analyses of the average spectral energy distributions (SEDs),
constructed from ...Adelberger, Anthony H. Gonzalez, Arjun Dey, Asantha Cooray, Ashby, Bouwens, Bouwens, Bouwens, Bouwens, Brown, Buell T. Jannuzi, Calzetti, Conroy, Daddi, Daddi, Daniel Stern, Dekel, Desai, Eilat Glikman, Erb, Ferguson, Fuyan Bian, Giavalisco, Jannuzi, Kajisawa, Kolatt, Kyoung-Soo Lee, Lee, Lee, Leitherer, Madau, Marchesini, Marchesini, Mark Brodwin, Martini, Meurer, Michael C. Cooper, Michael J. I. Brown, Naveen Reddy, Noeske, Ouchi, Pannella, Papovich, Quadri, Reddy, Reddy, Reddy, Sawicki, Shapley, Shapley, Shapley, Stark, Steidel, Vanzella, Xiaohui Fan +54 morecore +1 more sourceFormation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies
The Astrophysical JournalWe present an analysis of rest-frame optical and far-infrared continuum emission in three luminous submillimeter galaxies (SMGs) at 3.0 ≲ z ≲ 4.5.Ryota Ikeda, Daisuke Iono, Ken-ichi Tadaki, Maximilien Franco, Min S. Yun, Jorge A. Zavala, Yoichi Tamura, Takafumi Tsukui, Christina C. Williams, Bunyo Hatsukade, Minju M. Lee, Tomonari Michiyama, Ikki Mitsuhashi, Kouichiro Nakanishi, Caitlin M. Casey, Soh Ikarashi, Kianhong Lee, Yuichi Matsuda, Toshiki Saito, Andrea Silva, Hideki Umehata, Hidenobu Yajima +21 moredoaj +1 more sourceA COMPARISON OF THE MORPHOLOGICAL PROPERTIES BETWEEN LOCAL ANDz∼ 1 INFRARED LUMINOUS GALAXIES: ARE LOCAL AND HIGH-z(U)LIRGS DIFFERENT? [PDF]
, 2014 Chao-Ling Hung, D. B. Sanders, Caitlin M. Casey, Michael Koss, Kirsten L. Larson, Nicholas Lee, Yanxia Li, Kelly Lockhart, Hsin-Yi Shih, Joshua E. Barnes, Jeyhan S. Kartaltepe, Howard A. Smith +11 moreopenalex +1 more sourceQuantification of the Age Dependence of Mid-infrared Star Formation Rate Indicators
The Astrophysical JournalWe combine James Webb Space Telescope images of the nearby galaxy NGC 5194 in the hydrogen recombination line Pa α (1.8756 μ m) from the Cycle 1 program JWST-FEAST with 21 μ m dust continuum images from the Cycle 2 Treasury program JWGT to quantify the ...Daniela Calzetti, Robert C. Kennicutt, Angela Adamo, Karin Sandstrom, Daniel A. Dale, Bruce Elmegreen, John S. Gallagher, Benjamin Gregg, Varun Bajaj, Torsten Böker, Giacomo Bortolini, Martha Boyer, Matteo Correnti, Ilse De Looze, Bruce T. Draine, Ana Duarte-Cabral, Helena Faustino Vieira, Kathryn Grasha, L. K. Hunt, Kelsey E. Johnson, Ralf S. Klessen, Mark R. Krumholz, Thomas S.-Y. Lai, Drew Lapeer, Sean T. Linden, Matteo Messa, Göran Östlin, Alex Pedrini, Mònica Relaño, Elena Sabbi, Eva Schinnerer, Evan Skillman, Linda J. Smith, Monica Tosi, Fabian Walter, Tony D. Weinbeck +35 moredoaj +1 more source
