Search Results - "Knudsen, Kirsten"

Accurate dust temperature determination in a z = 7.13 galaxy by Bakx, Tom J L C, Sommovigo, Laura, Carniani, Stefano, Ferrara, Andrea, Akins, Hollis B, Fujimoto, Seiji, Hagimoto, Masato, Knudsen, Kirsten K, Pallottini, Andrea, Tamura, Yoichi, Watson, Darach

“…ABSTRACT We report ALMA Band 9 continuum observations of the normal, dusty star-forming galaxy A1689-zD1 at z = 7.13, resulting in a ∼4.6 σ detection at 702…”
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Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O iii] 88 μm, [C ii] 158 μm, and dust continuum with ALMA by Hashimoto, Takuya, Inoue, Akio K, Mawatari, Ken, Tamura, Yoichi, Matsuo, Hiroshi, Furusawa, Hisanori, Harikane, Yuichi, Shibuya, Takatoshi, Knudsen, Kirsten K, Kohno, Kotaro, Ono, Yoshiaki, Zackrisson, Erik, Okamoto, Takashi, Kashikawa, Nobunari, Oesch, Pascal A, Ouchi, Masami, Ota, Kazuaki, Shimizu, Ikkoh, Taniguchi, Yoshiaki, Umehata, Hideki, Watson, Darach

“…Abstract We present new ALMA observations and physical properties of a Lyman break galaxy at z = 7.15. Our target, B14-65666, has a bright ultra-violet (UV)…”
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linestacker: a spectral line stacking tool for interferometric data by Jolly, Jean-Baptiste, Knudsen, Kirsten K, Stanley, Flora

“…ABSTRACT linestacker is a new open access and open source tool for stacking of spectral lines in interferometric data. linestacker is an ensemble of casa…”
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ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13 by Akins, Hollis B., Fujimoto, Seiji, Finlator, Kristian, Watson, Darach, Knudsen, Kirsten K., Richard, Johan, C. Bakx, Tom J. L., Hashimoto, Takuya, Inoue, Akio K., Matsuo, Hiroshi, Michałowski, Michał J., Tamura, Yoichi

“…Abstract We present spatially resolved morphological properties of [C II ] 158 μ m, [O III ] 88 μ m, dust, and rest-frame ultraviolet (UV) continuum emission…”
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A TOTAL MOLECULAR GAS MASS CENSUS IN Z ∼ 2-3 STAR-FORMING GALAXIES: LOW-J CO EXCITATION PROBES OF GALAXIES' EVOLUTIONARY STATES by Sharon, Chelsea E., Riechers, Dominik A., Hodge, Jacqueline, Carilli, Chris L., Walter, Fabian, Weiß, Axel, Knudsen, Kirsten K., Wagg, Jeff

“…ABSTRACT We present CO(1-0) observations obtained at the Karl G. Jansky Very Large Array for 14 galaxies with existing CO(3-2) measurements, including 11…”
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Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies by Manning, Sinclaire M., Casey, Caitlin M., Zavala, Jorge A., Magdis, Georgios E., Drew, Patrick M., Champagne, Jaclyn B., Aravena, Manuel, Béthermin, Matthieu, Clements, David L., Finkelstein, Steven L., Fujimoto, Seiji, Hayward, Christopher C., Hodge, Jacqueline A., Ilbert, Olivier, Kartaltepe, Jeyhan S., Knudsen, Kirsten K., Koekemoer, Anton M., Man, Allison W. S., Sanders, David B., Sheth, Kartik, Spilker, Justin S., Staguhn, Johannes, Talia, Margherita, Treister, Ezequiel, Yun, Min S.

“…Abstract The 2 mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was designed to detect high-redshift ( z ≳ 4), massive, dusty star-forming…”
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A merger in the dusty, z = 7.5 galaxy A1689-zD1? by Knudsen, Kirsten K., Watson, Darach, Frayer, David, Christensen, Lise, Gallazzi, Anna, Michałowski, Michał J., Richard, Johan, Zavala, Jesús

“…Abstract The gravitationally lensed galaxy A1689-zD1 is one of the most distant spectroscopically confirmed sources (z = 7.5). It is the earliest known galaxy…”
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INFRARED SPECTRAL ENERGY DISTRIBUTION DECOMPOSITION OF WISE-SELECTED, HYPERLUMINOUS HOT DUST-OBSCURED GALAXIES by Fan(范璐璐), Lulu, Han(韩云坤), Yunkun, Nikutta, Robert, Drouart, Guillaume, Knudsen, Kirsten K.

“…ABSTRACT We utilize a Bayesian approach to fit the observed mid-IR-to-submillimeter/millimeter spectral energy distributions (SEDs) of 22 WISE-selected and…”
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Physical Properties of Hyperluminous, Dust-obscured Quasars at z ∼ 3: Multiwavelength Spectral Energy Distribution Analysis and Cold Gas Content Revealed by ALMA by Sun, Weibin, Fan, Lulu, Han, Yunkun, Knudsen, Kirsten K., Chen, Guangwen, Zhang, Hong-Xin

“…Abstract We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the…”
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The Spectral Energy Distribution of the Hyperluminous, Hot Dust-obscured Galaxy W2246-0526 by Fan, Lulu, Gao, Ying, Knudsen, Kirsten K., Shu, Xinwen

“…Hot dust-obscured galaxies (Hot DOGs) are a luminous, dust-obscured population recently discovered in the WISE All-Sky survey. Multiwavelength follow-up…”
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Metal-enriched Neutral Gas Reservoir around a Strongly Lensed Low-mass Galaxy at z = 4 Identified by JWST/NIRISS and VLT/MUSE by Lin, Xiaojing, Cai, Zheng, Zou, Siwei, Li, Zihao, Chen, Zuyi, Bian, Fuyan, Sun, Fengwu, Shu, Yiping, Wu, Yunjing, Li, Mingyu, Li, Jianan, Fan, Xiaohui, Prochaska, J. Xavier, Schaerer, Daniel, Charlot, Stephane, Espada, Daniel, Dessauges-Zavadsky, Miroslava, Egami, Eiichi, Stark, Daniel, Knudsen, Kirsten K., Bruzual, Gustavo, Chevallard, Jacopo

“…Abstract Direct observations of low-mass, low-metallicity galaxies at z ≳ 4 provide an indispensable opportunity for detailed inspection of the ionization…”
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Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85 by Casey, Caitlin M., Zavala, Jorge A., Aravena, Manuel, Béthermin, Matthieu, Caputi, Karina I., Champagne, Jaclyn B., Clements, David L., Cunha, Elisabete da, Drew, Patrick, Finkelstein, Steven L., Hayward, Christopher C., Kartaltepe, Jeyhan S., Knudsen, Kirsten, Koekemoer, Anton M., Magdis, Georgios E., Man, Allison, Manning, Sinclaire M., Scoville, Nick Z., Sheth, Kartik, Spilker, Justin, Staguhn, Johannes, Talia, Margherita, Taniguchi, Yoshiaki, Toft, Sune, Treister, Ezequiel, Yun, Min

“…We present a physical characterization of MM J100026.36+021527.9 (a.k.a. "Mambo-9"), a dusty star-forming galaxy (DSFG) at z = 5.850 0.001. This is the…”
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ALMA Lensing Cluster Survey: Bright [C ii] 158 μm Lines from a Multiply Imaged Sub-L ⋆ Galaxy at z = 6.0719 by Fujimoto, Seiji, Oguri, Masamune, Brammer, Gabriel, Yoshimura, Yuki, Laporte, Nicolas, González-López, Jorge, Caminha, Gabriel B., Kohno, Kotaro, Zitrin, Adi, Richard, Johan, Ouchi, Masami, Bauer, Franz E., Smail, Ian, Hatsukade, Bunyo, Ono, Yoshiaki, Kokorev, Vasily, Umehata, Hideki, Schaerer, Daniel, Knudsen, Kirsten, Sun, Fengwu, Magdis, Georgios, Valentino, Francesco, Ao, Yiping, Toft, Sune, Dessauges-Zavadsky, Miroslava, Shimasaku, Kazuhiro, Caputi, Karina, Kusakabe, Haruka, Morokuma-Matsui, Kana, Shotaro, Kikuchihara, Egami, Eiichi, Lee, Minju M., Rawle, Timothy, Espada, Daniel

“…Abstract We present bright [C ii ] 158 μ m line detections from a strongly magnified and multiply imaged ( μ ∼ 20–160) sub– L * ( M UV = − 19.75 − 0.44 + 0.55…”
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Gas conditions of a star-formation selected sample in the first billion years by Bakx, Tom J L C, Algera, Hiddo S B, Venemans, Bram, Sommovigo, Laura, Fujimoto, Seiji, Carniani, Stefano, Hagimoto, Masato, Hashimoto, Takuya, Inoue, Akio K, Salak, Dragan, Serjeant, Stephen, Vallini, Livia, Eales, Stephen, Ferrara, Andrea, Fudamoto, Yoshinobu, Imamura, Chihiro, Inoue, Shigeki, Knudsen, Kirsten K, Matsuo, Hiroshi, Sugahara, Yuma, Tamura, Yoichi, Taniguchi, Akio, Yamanaka, Satoshi

“…ABSTRACT We present Atacama Large Millimetre/submillimetre Array (ALMA) observations of the [O iii] 88 $\mu {\rm m}$ emission of a sample of thirteen galaxies…”
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The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description by Muxlow, T W B, Thomson, A P, Radcliffe, J F, Wrigley, N H, Beswick, R J, Smail, Ian, McHardy, I M, Garrington, S T, Ivison, R J, Jarvis, M J, Prandoni, I, Bondi, M, Guidetti, D, Argo, M K, Bacon, David, Best, P N, Biggs, A D, Chapman, S C, Coppin, K, Chen, H, Garratt, T K, Garrett, M A, Ibar, E, Kneib, Jean-Paul, Knudsen, Kirsten K, Koopmans, L V E, Morabito, L K, Murphy, E J, Njeri, A, Pearson, Chris, Pérez-Torres, M A, Richards, A M S, Röttgering, H J A, Sargent, M T, Serjeant, Stephen, Simpson, C, Simpson, J M, Swinbank, A M, Varenius, E, Venturi, T

“…ABSTRACT We present an overview and description of the e-MERGE Survey (e-MERLIN Galaxy Evolution Survey) Data Release 1 (DR1), a large program of…”
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ALMA Reveals a Gas-rich, Maximum Starburst in the Hyperluminous, Dust-obscured Quasar W0533-3401 at z ∼ 2.9 by Fan, Lulu, Knudsen, Kirsten K., Han, Yunkun, Tan, Qing-hua

“…We present ALMA observations and multiwavelength spectral energy distribution analysis in a Wide-field Infrared Survey Explorer-selected, hyperluminous…”
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The SCUBA-2 850 μ m Follow-up of WISE -selected, Luminous Dust-obscured Quasars by Fan, Lulu, Jones, Suzy F., Han, Yunkun, Knudsen, Kirsten K.

“…Hot dust-obscured galaxies (Hot DOGs) are a new population recently discovered in the Wide-field Infrared Survey Explorer All-Sky survey. Multiwavelength…”
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A variable active galactic nucleus at z  = 2.06 triply-imaged by the galaxy cluster MACS J0035.4−2015 by Furtak, Lukas J, Mainali, Ramesh, Zitrin, Adi, Plat, Adèle, Fujimoto, Seiji, Donahue, Megan, Nelson, Erica J, Bauer, Franz E, Uematsu, Ryosuke, Caminha, Gabriel B, Andrade-Santos, Felipe, Bradley, Larry D, Caputi, Karina I, Charlot, Stéphane, Chevallard, Jacopo, Coe, Dan, Curtis-Lake, Emma, Espada, Daniel, Frye, Brenda L, Knudsen, Kirsten K, Koekemoer, Anton M, Kohno, Kotaro, Kokorev, Vasily, Laporte, Nicolas, Lee, Minju M, Lemaux, Brian C, Magdis, Georgios E, Sharon, Keren, Stark, Daniel P, Su, Yuanyuan, Suess, Katherine A, Ueda, Yoshihiro, Umehata, Hideki, Vidal-García, Alba, Wu, John F

“…ABSTRACT We report the discovery of a triply imaged active galactic nucleus (AGN), lensed by the galaxy cluster MACS J0035.4−2015 (zd = 0.352). The object is…”
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[C ii] emission in z ∼ 6 strongly lensed, star-forming galaxies by Knudsen, Kirsten K., Richard, Johan, Kneib, Jean-Paul, Jauzac, Mathilde, Clément, Benjamin, Drouart, Guillaume, Egami, Eiichi, Lindroos, Lukas

“…The far-infrared fine-structure line [C ii] at 1900.5 GHz is known to be one of the brightest cooling lines in local galaxies, and therefore it has been…”
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The SCUBA-2 850 μm Follow-up of WISE-selected, Luminous Dust-obscured Quasars by Fan, Lulu, Jones, Suzy F., Han, Yunkun, Knudsen, Kirsten K.

“…Hot dust-obscured galaxies (Hot DOGs) are a new population recently discovered in the Wide-field Infrared Survey Explorer All-Sky survey. Multiwavelength…”
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