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Your search keyword '"Dai, Y."' showing total 38 results
Start Over Author "Dai, Y." Journal the astrophysical journal
38 results on '"Dai, Y."'

1. An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs

Author

Jin, Gaoxiang, Dai, Y Sophia, Pan, Hsi-An, Lin, Lihwai, Li, Cheng, Hsieh, Bau-Ching, Shen, Shiyin, Yuan, Fang-Ting, Feng, Shuai, Cheng, Cheng, Xu, Hai, Huang, Jia-Sheng, and Zhang, Kai

Subjects
Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

The role of active galactic nuclei (AGNs) during galaxy interactions and how they influence the star formation in the system are still under debate. We use a sample of 1156 galaxies in galaxy pairs or mergers (hereafter "pairs") from the MaNGA survey. This pair sample is selected by the velocity offset, projected separation, and morphology, and is further classified into four cases along the merger sequence based on morphological signatures. We then identify a total of 61 (5.5%) AGNs in pairs based on the emission-line diagnostics. No evolution of the AGN fraction is found, either along the merger sequence or compared to isolated galaxies (5.0%). We observe a higher fraction of passive galaxies in galaxy pairs, especially in the pre-merging cases, and associate the higher fraction to their environmental dependence. The isolated AGN and AGNs in pairs show similar distributions in their global stellar mass, star-formation rate (SFR), and central [O iii] surface brightness. AGNs in pairs show radial profiles of increasing specific SFR and declining Dn4000 from center to outskirts, and no significant difference from the isolated AGNs. This is clearly different from star-forming galaxies (SFGs) in our pair sample, which show enhanced central star formation, as reported before. AGNs in pairs have lower Balmer decrements at outer regions, possibly indicating less dust attenuation. Our findings suggest that AGNs are likely follow an inside-out quenching and the merger impact on the star formation in AGNs is less prominent than in SFGs.

Published
2021

2. Spectroscopically Identified Emission Line Galaxy Pairs in the WISP Survey* * Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs 11696, 12283, 12568, 12092, 13352, 13517, and 14178.

Author

Dai, Y Sophia, Malkan, Matthew M, Teplitz, Harry I, Scarlata, Claudia, Alavi, Anahita, Atek, Hakim, Bagley, Micaela, Baronchelli, Ivano, Battisti, Andrew, Bunker, Andrew J, Hathi, Nimish P, Henry, Alaina, Huang, Jiasheng, Jin, Gaoxiang, Li, Zijian, Martin, Crystal, Mehta, Vihang, Phillips, John, Rafelski, Marc, Rutkowski, Michael, Xu, Hai, Xu, Cong K, and Zanella, Anita

Subjects
Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We identify a sample of spectroscopically measured emission line galaxy (ELG) Pairs up to z = 1.6 from the Wide Field Camera 3 (WFC3) Infrared Spectroscopic Parallels (WISP) survey. WISP obtained slitless, near-infrared grism spectroscopy along with direct imaging in the J and H bands by observing in the pure-parallel mode with the WFC3 on board the Hubble Space Telescope. From our search of 419 WISP fields covering an area of ∼0.5 deg2, we find 413 ELG pair systems, mostly H α emitters. We then derive reliable star formation rates (SFRs) based on the attenuation-corrected H α fluxes. Compared to isolated galaxies, we find an average SFR enhancement of 40%–65%, which is stronger for major Pairs and Pairs with smaller velocity separations (Δ v < 300 km s−1). Based on the stacked spectra from various subsamples, we study the trends of emission line ratios in pairs, and find a general consistency with enhanced lower ionization lines. We study the pair fraction among ELGs, and find a marginally significant increase with redshift f ∝ (1 + z) α , where the power-law index α = 0.58 ± 0.17 from z ∼ 0.2 to ∼1.6. The fraction of active galactic nuclei is found to be the same in the ELG Pairs as compared to the isolated ELGs.

Published
2021

3. The Mass–Metallicity Relation at z ∼ 1–2 and Its Dependence on the Star Formation Rate

Author

Henry, Alaina, Rafelski, Marc, Sunnquist, Ben, Pirzkal, Norbert, Pacifici, Camilla, Atek, Hakim, Bagley, Micaela, Baronchelli, Ivano, Barro, Guillermo, Bunker, Andrew J, Colbert, James, Dai, Y Sophia, Elmegreen, Bruce G, Elmegreen, Debra Meloy, Finkelstein, Steven, Kocevski, Dale, Koekemoer, Anton, Malkan, Matthew, Martin, Crystal L, Mehta, Vihang, Pahl, Anthony, Papovich, Casey, Rutkowski, Michael, Almeida, Jorge Sánchez, Scarlata, Claudia, Snyder, Gregory, and Teplitz, Harry

Subjects
Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We present a new measurement of the gas-phase mass-metallicity relation (MZR) and its dependence on star formation rates (SFRs) at 1.3 < z < 2.3. Our sample comprises 1056 galaxies with a mean redshift of z = 1.9, identified from the Hubble Space Telescope Wide Field Camera 3 (WFC3) grism spectroscopy in the Cosmic Assembly Near-infrared Deep Extragalactic Survey and the WFC3 Infrared Spectroscopic Parallel Survey. This sample is four times larger than previous metallicity surveys at z ~ 2 and reaches an order of magnitude lower in stellar mass (108 M o?). Using stacked spectra, we find that the MZR evolves by 0.3 dex relative to z ~ 0.1. Additionally, we identify a subset of 49 galaxies with high signal-to-noise (S/N) spectra and redshifts between 1.3 < z < 1.5, where Ha emission is observed along with [O iii] and [O ii]. With accurate measurements of SFR in these objects, we confirm the existence of a mass-metallicity-SFR (M-Z-SFR) relation at high redshifts. These galaxies show systematic differences from the local M-Z-SFR relation, which vary depending on the adopted measurement of the local relation. However, it remains difficult to ascertain whether these differences could be due to redshift evolution, as the local M-Z-SFR relation is poorly constrained at the masses and SFRs of our sample. Lastly, we reproduced our sample selection in the IllustrisTNG hydrodynamical simulation, demonstrating that our line flux limit lowers the normalization of the simulated MZR by 0.2 dex. We show that the M-Z-SFR relation in IllustrisTNG has an SFR dependence that is too steep by a factor of around 3.

Published
2021

7. A High Space Density of Luminous Lyα Emitters at z ∼ 6.5

Author

Bagley, Micaela B, Scarlata, Claudia, Henry, Alaina, Rafelski, Marc, Malkan, Matthew, Teplitz, Harry, Dai, Y Sophia, Baronchelli, Ivano, Colbert, James, Rutkowski, Michael, Mehta, Vihang, Dressler, Alan, McCarthy, Patrick, Bunker, Andrew, Atek, Hakim, Garel, Thibault, Martin, Crystal L, Hathi, Nimish, and Siana, Brian

Subjects
cosmology: observations, galaxies: high-redshift, astro-ph.CO, astro-ph.GA, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We present the results of a systematic search for Lyα emitters (LAEs) at 6 ≲ z ≲ 7.6 using the HST WFC3 Infrared Spectroscopic Parallel (WISP) Survey. Our total volume over this redshift range is ∼8 × 105 Mpc3, comparable to many of the narrowband surveys despite their larger area coverage. We find two LAEs at z = 6.38 and 6.44 with line luminosities of LLyα ∼ 4.7 × 1043 erg s-1, putting them among the brightest LAEs discovered at these redshifts. Taking advantage of the broad spectral coverage of WISP, we are able to rule out almost all lower-redshift contaminants. The WISP LAEs have a high number density of 7.7 × 10-6 Mpc-3. We argue that the LAEs reside in megaparsec-scale ionized bubbles that allow the Lyα photons to redshift out of resonance before encountering the neutral intergalactic medium. We discuss possible ionizing sources and conclude that the observed LAEs alone are not sufficient to ionize the bubbles.

Published
2017

8. HerMES: SPECTRAL ENERGY DISTRIBUTIONS OF SUBMILLIMETER GALAXIES AT z > 4**Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

Author

Huang, J-S, Rigopoulou, D, Magdis, G, Rowan-Robinson, M, Dai, Y, Bock, JJ, Burgarella, D, Chapman, S, Clements, DL, Cooray, A, Farrah, D, Glenn, J, Oliver, S, Smith, AJ, Wang, L, Page, M, Riechers, D, Roseboom, I, Symeonidis, M, Fazio, GG, Yun, M, Webb, TMA, and Efstathiou, A

Subjects
cosmology: observations, galaxies: evolution, galaxies: formation, infrared: galaxies, astro-ph.GA, astro-ph.CO, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We present a study of the infrared properties for a sample of seven spectroscopically confirmed submillimeter galaxies (SMGs) at z > 4.0. By combining ground-based near-infrared, Spitzer IRAC and MIPS, Herschel SPIRE, and ground-based submillimeter/millimeter photometry, we construct their spectral energy distributions (SEDs) and a composite model to fit the SEDs. The model includes a stellar emission component at λrest < 3.5 μm, a hot dust component peaking at λrest ∼ 5 μm, and cold dust component which becomes significant for λrest > 50 μm. Six objects in the sample are detected at 250 and 350 μm. The dust temperatures for the sources in this sample are in the range of 40-80 K, and their LFIR ∼ 1013 L⊙ qualifies them as hyper-luminous infrared galaxies. The mean FIR-radio index for this sample is around 〈q〉 = 2.2 indicating no radio excess in their radio emission. Most sources in the sample have 24 μm detections corresponding to a rest-frame 4.5 μm luminosity of Log10(L4.5/L ⊙) = 11 ∼ 11.5. Their L4.5/LFIR ratios are very similar to those of starburst-dominated SMGs at z ∼ 2. The L CO-LFIR relation for this sample is consistent with that determined for local ULIRGs and SMGs at z ∼ 2. We conclude that SMGs at z > 4 are hotter and more luminous in the FIR but otherwise very similar to those at z ∼ 2. None of these sources show any sign of the strong QSO phase being triggered. © 2014. The American Astronomical Society. All rights reserved.

Published
2014

9. UV-bright Star-forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 ≤ z ≤ 1

Author

Martin, Alec, primary, Guo, Yicheng, additional, Wang, Xin, additional, Koekemoer, Anton M., additional, Rafelski, Marc, additional, Teplitz, Harry I., additional, Windhorst, Rogier A., additional, Alavi, Anahita, additional, Grogin, Norman A., additional, Prichard, Laura, additional, Sunnquist, Ben, additional, Ceverino, Daniel, additional, Chartab, Nima, additional, Conselice, Christopher J., additional, Dai, Y. Sophia, additional, Dekel, Avishai, additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Hathi, Nimish P., additional, Hayes, Matthew J., additional, Jansen, Rolf A., additional, Ji, Zhiyuan, additional, Koo, David C., additional, Lucas, Ray A., additional, Mandelker, Nir, additional, Mehta, Vihang, additional, Mobasher, Bahram, additional, Nedkova, Kalina V., additional, Primack, Joel, additional, Ravindranath, Swara, additional, Robertson, Brant E., additional, Rutkowski, Michael J., additional, Sattari, Zahra, additional, Soto, Emmaris, additional, and Yung, L. Y. Aaron, additional

Published
2023
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10. Deep H i Mapping of Stephan’s Quintet and Its Neighborhood

Author

Cheng, Cheng, primary, Xu, Cong Kevin, additional, Appleton, P. N., additional, Duc, P.-A., additional, Tang, N.-Y., additional, Dai, Y.-S., additional, Huang, J.-S., additional, Lisenfeld, U., additional, Renaud, F., additional, He, Chuan, additional, and Feng, Hai-Cheng, additional

Published
2023
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11. A Spatially Resolved Analysis of Star Formation Burstiness by Comparing UV and Hα in Galaxies at z ∼ 1 with UVCANDELS

Author

Mehta, Vihang, primary, Teplitz, Harry I., additional, Scarlata, Claudia, additional, Wang, Xin, additional, Alavi, Anahita, additional, Colbert, James, additional, Rafelski, Marc, additional, Grogin, Norman, additional, Koekemoer, Anton, additional, Prichard, Laura, additional, Windhorst, Rogier, additional, Barber, Justin M., additional, Conselice, Christopher J., additional, Dai, Y. Sophia, additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Guo, Yicheng, additional, Hathi, Nimish, additional, Haro, Pablo Arrabal, additional, Hayes, Matthew, additional, Iyer, Kartheik G., additional, Jansen, Rolf A., additional, Ji, Zhiyuan, additional, Kurczynski, Peter, additional, Kuschel, Maxwell, additional, Lucas, Ray A., additional, Mantha, Kameswara, additional, O’Connell, Robert W., additional, Ravindranath, Swara, additional, Robertson, Brant E., additional, Rutkowski, Michael, additional, Siana, Brian, additional, and Yung, L. Y. Aaron, additional

Published
2023
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12. Fraction of Clumpy Star-forming Galaxies at 0.5 ≤ z ≤ 3 in UVCANDELS: Dependence on Stellar Mass and Environment

Author

Sattari, Zahra, primary, Mobasher, Bahram, additional, Chartab, Nima, additional, Kelson, Daniel D., additional, Teplitz, Harry I., additional, Rafelski, Marc, additional, Grogin, Norman A., additional, Koekemoer, Anton M., additional, Wang, Xin, additional, Windhorst, Rogier A., additional, Alavi, Anahita, additional, Prichard, Laura, additional, Sunnquist, Ben, additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Hathi, Nimish P., additional, Hayes, Matthew J., additional, Ji, Zhiyuan, additional, Mehta, Vihang, additional, Robertson, Brant E., additional, Scarlata, Claudia, additional, Yung, L. Y. Aaron, additional, Conselice, Christopher J., additional, Dai, Y. Sophia, additional, Guo, Yicheng, additional, Lucas, Ray A., additional, Martin, Alec, additional, and Ravindranath, Swara, additional

Published
2023
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13. Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups

Author

Kuschel, Maxwell, primary, Scarlata, Claudia, additional, Mehta, Vihang, additional, Teplitz, Harry I., additional, Rafelski, Marc, additional, Wang, Xin, additional, Sunnquist, Ben, additional, Prichard, Laura, additional, Grogin, Norman, additional, Koekemoer, Anton, additional, Windhorst, Rogier, additional, Rutkowski, Michael, additional, Alavi, Anahita, additional, Chartab, Nima, additional, Conselice, Christopher J., additional, Dai, Y. Sophia, additional, Gawiser, Eric, additional, Giavalisco, Mauro, additional, Haro, Pablo Arrabal, additional, Hathi, Nimish, additional, Jansen, Rolf A., additional, Ji, Zhiyuan, additional, Lucas, Ray A., additional, Mantha, Kameswara, additional, Mobasher, Bahram, additional, O’Connell, Robert W., additional, Robertson, Brant, additional, Sattari, Zahra, additional, Yung, L. Y. Aaron, additional, Davé, Romeel, additional, DeMello, Duilia, additional, Dickinson, Mark, additional, Ferguson, Henry, additional, Finkelstein, Steven L., additional, Hayes, Matt, additional, Howell, Justin, additional, Kaviraj, Sugata, additional, Mackenty, John W., additional, and Siana, Brian, additional

Published
2023
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15. The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

Author

Ching, Tao-Chung, primary, Qiu, Keping, additional, Li, Di, additional, Ren, Zhiyuan, additional, Lai, Shih-Ping, additional, Berry, David, additional, Pattle, Kate, additional, Furuya, Ray, additional, Ward-Thompson, Derek, additional, Johnstone, Doug, additional, Koch, Patrick M., additional, Lee, Chang Won, additional, Hoang, Thiem, additional, Hasegawa, Tetsuo, additional, Kwon, Woojin, additional, Bastien, Pierre, additional, Eswaraiah, Chakali, additional, Wang, Jia-Wei, additional, Kim, Kyoung Hee, additional, Hwang, Jihye, additional, Soam, Archana, additional, Lyo, A-Ran, additional, Liu, Junhao, additional, Le Gouellec, Valentin J. M., additional, Arzoumanian, Doris, additional, Whitworth, Anthony, additional, Francesco, James Di, additional, Poidevin, Frédérick, additional, Liu, Tie, additional, Coudé, Simon, additional, Tahani, Mehrnoosh, additional, Liu, Hong-Li, additional, Onaka, Takashi, additional, Li, Dalei, additional, Tamura, Motohide, additional, Chen, Zhiwei, additional, Tang, Xindi, additional, Kirchschlager, Florian, additional, Bourke, Tyler L., additional, Byun, Do-Young, additional, Chen, Mike, additional, Chen, Huei-Ru Vivien, additional, Chen, Wen Ping, additional, Cho, Jungyeon, additional, Choi, Yunhee, additional, Choi, Youngwoo, additional, Choi, Minho, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Dai, Y. Sophia, additional, Diep, Pham Ngoc, additional, Doi, Yasuo, additional, Duan, Yan, additional, Duan, Hao-Yuan, additional, Eden, David, additional, Fanciullo, Lapo, additional, Fiege, Jason, additional, Fissel, Laura M., additional, Franzmann, Erica, additional, Friberg, Per, additional, Friesen, Rachel, additional, Fuller, Gary, additional, Gledhill, Tim, additional, Graves, Sarah, additional, Greaves, Jane, additional, Griffin, Matt, additional, Gu, Qilao, additional, Han, Ilseung, additional, Hayashi, Saeko, additional, Houde, Martin, additional, Hull, Charles L. H., additional, Inoue, Tsuyoshi, additional, Inutsuka, Shu-ichiro, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Könyves, Vera, additional, Kang, Ji-hyun, additional, Kang, Miju, additional, Karoly, Janik, additional, Kataoka, Akimasa, additional, Kawabata, Koji, additional, Kemper, Francisca, additional, Kim, Jongsoo, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Kim, Hyosung, additional, Kim, Kee-Tae, additional, Kim, Gwanjeong, additional, Kirk, Jason, additional, Kobayashi, Masato I. N., additional, Kusune, Takayoshi, additional, Kwon, Jungmi, additional, Lacaille, Kevin, additional, Law, Chi-Yan, additional, Lee, Sang-Sung, additional, Lee, Hyeseung, additional, Lee, Jeong-Eun, additional, Lee, Chin-Fei, additional, Lee, Yong-Hee, additional, Li, Guangxing, additional, Li, Hua-bai, additional, Lin, Sheng-Jun, additional, Liu, Sheng-Yuan, additional, Lu, Xing, additional, Mairs, Steve, additional, Matsumura, Masafumi, additional, Matthews, Brenda, additional, Moriarty-Schieven, Gerald, additional, Nagata, Tetsuya, additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ngoc, Nguyen Bich, additional, Ohashi, Nagayoshi, additional, Park, Geumsook, additional, Parsons, Harriet, additional, Peretto, Nicolas, additional, Priestley, Felix, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Rao, Ramprasad, additional, Rawlings, Mark, additional, Rawlings, Jonathan, additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Sadavoy, Sarah, additional, Saito, Hiro, additional, Savini, Giorgio, additional, Seta, Masumichi, additional, Shimajiri, Yoshito, additional, Shinnaga, Hiroko, additional, Tang, Ya-Wen, additional, Tomisaka, Kohji, additional, Tram, Le Ngoc, additional, Tsukamoto, Yusuke, additional, Viti, Serena, additional, Wang, Hongchi, additional, Wu, Jintai, additional, Xie, Jinjin, additional, Yang, Meng-Zhe, additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, Yuan, Jinghua, additional, Yun, Hyeong-Sik, additional, Zenko, Tetsuya, additional, Zhang, Chuan-Peng, additional, Zhang, Yapeng, additional, Zhang, Guoyin, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, de Looze, Ilse, additional, André, Philippe, additional, Dowell, C. Darren, additional, Eyres, Stewart, additional, Falle, Sam, additional, Robitaille, Jean-François, additional, and van Loo, Sven, additional

Published
2022
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16. The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2

Author

Hwang, Jihye, primary, Kim, Jongsoo, additional, Pattle, Kate, additional, Lee, Chang Won, additional, Koch, Patrick M., additional, Johnstone, Doug, additional, Tomisaka, Kohji, additional, Whitworth, Anthony, additional, Furuya, Ray S., additional, Kang, Ji-hyun, additional, Lyo, A-Ran, additional, Chung, Eun Jung, additional, Arzoumanian, Doris, additional, Park, Geumsook, additional, Kwon, Woojin, additional, Kim, Shinyoung, additional, Tamura, Motohide, additional, Kwon, Jungmi, additional, Soam, Archana, additional, Han, Ilseung, additional, Hoang, Thiem, additional, Kim, Kyoung Hee, additional, Onaka, Takashi, additional, Eswaraiah, Chakali, additional, Ward-Thompson, Derek, additional, Liu, Hong-Li, additional, Tang, Xindi, additional, Chen, Wen Ping, additional, Matsumura, Masafumi, additional, Hoang, Thuong Duc, additional, Chen, Zhiwei, additional, Le Gouellec, Valentin J. M., additional, Kirchschlager, Florian, additional, Poidevin, Frédérick, additional, Bastien, Pierre, additional, Qiu, Keping, additional, Hasegawa, Tetsuo, additional, Lai, Shih-Ping, additional, Byun, Do-Young, additional, Cho, Jungyeon, additional, Choi, Minho, additional, Choi, Youngwoo, additional, Choi, Yunhee, additional, Jeong, Il-Gyo, additional, Kang, Miju, additional, Kim, Hyosung, additional, Kim, Kee-Tae, additional, Lee, Jeong-Eun, additional, Lee, Sang-Sung, additional, Lee, Yong-Hee, additional, Lee, Hyeseung, additional, Kim, Mi-Ryang, additional, Yoo, Hyunju, additional, Yun, Hyeong-Sik, additional, Chen, Mike, additional, Francesco, James Di, additional, Fiege, Jason, additional, Fissel, Laura M., additional, Franzmann, Erica, additional, Houde, Martin, additional, Lacaille, Kevin, additional, Matthews, Brenda, additional, Sadavoy, Sarah, additional, Moriarty-Schieven, Gerald, additional, Tahani, Mehrnoosh, additional, Ching, Tao-Chung, additional, Dai, Y. Sophia, additional, Duan, Yan, additional, Gu, Qilao, additional, Law, Chi-Yan, additional, Li, Dalei, additional, Li, Di, additional, Li, Guangxing, additional, Li, Hua-bai, additional, Liu, Tie, additional, Lu, Xing, additional, Qian, Lei, additional, Wang, Hongchi, additional, Wu, Jintai, additional, Xie, Jinjin, additional, Yuan, Jinghua, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhang, Yapeng, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, Berry, David, additional, Friberg, Per, additional, Graves, Sarah, additional, Liu, Junhao, additional, Mairs, Steve, additional, Parsons, Harriet, additional, Rawlings, Mark, additional, Doi, Yasuo, additional, Hayashi, Saeko, additional, Hull, Charles L. H., additional, Inoue, Tsuyoshi, additional, Inutsuka, Shu-ichiro, additional, Iwasaki, Kazunari, additional, Kataoka, Akimasa, additional, Kawabata, Koji, additional, Kim, Gwanjeong, additional, Kobayashi, Masato I. N., additional, Nagata, Tetsuya, additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Pyo, Tae-Soo, additional, Saito, Hiro, additional, Seta, Masumichi, additional, Shimajiri, Yoshito, additional, Shinnaga, Hiroko, additional, Tsukamoto, Yusuke, additional, Zenko, Tetsuya, additional, Chen, Huei-Ru Vivien, additional, Duan, Hao-Yuan, additional, Fanciullo, Lapo, additional, Kemper, Francisca, additional, Lee, Chin-Fei, additional, Lin, Sheng-Jun, additional, Liu, Sheng-Yuan, additional, Ohashi, Nagayoshi, additional, Rao, Ramprasad, additional, Tang, Ya-Wen, additional, Wang, Jia-Wei, additional, Yang, Meng-Zhe, additional, Yen, Hsi-Wei, additional, Bourke, Tyler L., additional, Chrysostomou, Antonio, additional, Debattista, Victor, additional, Eden, David, additional, Eyres, Stewart, additional, Falle, Sam, additional, Fuller, Gary, additional, Gledhill, Tim, additional, Greaves, Jane, additional, Griffin, Matt, additional, Hatchell, Jennifer, additional, Karoly, Janik, additional, Kirk, Jason, additional, Könyves, Vera, additional, Longmore, Steven, additional, van Loo, Sven, additional, Looze, Ilse de, additional, Peretto, Nicolas, additional, Priestley, Felix, additional, Rawlings, Jonathan, additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Savini, Giorgio, additional, Scaife, Anna, additional, Viti, Serena, additional, Diep, Pham Ngoc, additional, Ngoc, Nguyen Bich, additional, Tram, Le Ngoc, additional, André, Philippe, additional, Coudé, Simon, additional, Dowell, C. Darren, additional, Friesen, Rachel, additional, and Robitaille, Jean-Franćois, additional

Published
2022
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17. Groups and Protocluster Candidates in the CLAUDS and HSC-SSP Joint Deep Surveys

Author

Li, Qingyang, primary, Yang, Xiaohu, additional, Liu, Chengze, additional, Jing, Yipeng, additional, He, Min, additional, Huang, Jia-Sheng, additional, Dai, Y. Sophia, additional, Sawicki, Marcin, additional, Arnouts, Stephane, additional, Gwyn, Stephen, additional, Moutard, Thibaud, additional, Mo, H. J., additional, Wang, Kai, additional, Katsianis, Antonios, additional, Cui, Weiguang, additional, Han, Jiaxin, additional, Chiu, I-Non, additional, Gu, Yizhou, additional, and Xu, Haojie, additional

Published
2022
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19. A Complete 16 μm Selected Galaxy Sample at z ∼ 1: Mid-infrared Spectral Energy Distributions

Author

Huang, J.-S., primary, Dai, Y.-S., additional, Willner, S. P., additional, Faber, S. M., additional, Cheng, C., additional, Xu, H., additional, Yan, H., additional, Wu, S., additional, Shao, X., additional, Hao, C., additional, Xia, X., additional, Rigopoulou, D., additional, Pereira Santaella, M., additional, Magdis, G., additional, Cortzen, I., additional, Fazio, G. G., additional, Assmann, P., additional, Fan, L., additional, Musin, M., additional, Wang, Z., additional, Xu, K. C., additional, He, C., additional, Jin, G., additional, and Esamdin, A., additional

Published
2021
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21. A Large Massive Quiescent Galaxy Sample at z ∼ 1.2

Author

Xu, Hai, primary, Dai, Y. Sophia, additional, Huang, Jia-Sheng, additional, Wang, Zhaoyu, additional, Cheng, Cheng, additional, Shao, Xu, additional, Wu, Shumei, additional, Yang, Xiaohu, additional, Jing, Yipeng, additional, Sawicki, Marcin, additional, and Liu, Feng-Yuan, additional

Published
2020
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23. ALMA $[{\rm{N}}\,{\rm{II}}]$ 205 μm Imaging Spectroscopy of the Lensed Submillimeter Galaxy ID 141 at Redshift 4.24

Author

Cheng, Cheng, primary, Cao, Xiaoyue, additional, Lu, Nanyao, additional, Li, Ran, additional, Yang, Chentao, additional, Rigopoulou, Dimitra, additional, Charmandaris, Vassilis, additional, Gao, Yu, additional, Xu, Cong Kevin, additional, van der Werf, Paul, additional, Diaz Santos, Tanio, additional, Privon, George C., additional, Zhao, Yinghe, additional, Cao, Tianwen, additional, Dai, Y. Sophia, additional, Huang, Jia-Sheng, additional, Sanders, David, additional, Wang, Chunxiang, additional, Wang, Zhong, additional, and Zhu, Lei, additional

Published
2020
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25. SDSS-IV MaNGA: Spatial Evolution of Star Formation Triggered by Galaxy Interactions

Author

Pan, Hsi-An, primary, Lin, Lihwai, additional, Hsieh, Bau-Ching, additional, Barrera-Ballesteros, Jorge K., additional, Sánchez, Sebastián F., additional, Hsu, Chin-Hao, additional, Keenan, Ryan, additional, Tissera, Patricia B., additional, Boquien, Médéric, additional, Dai, Y. Sophia, additional, Knapen, Johan H., additional, Riffel, Rogério, additional, Argudo-Fernández, Maria, additional, Xiao, Ting, additional, and Yuan, Fang-Ting, additional

Published
2019
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27. A High Space Density of Luminous LyαEmitters at $z\sim 6.5$

Author

Bagley, Micaela B., primary, Scarlata, Claudia, additional, Henry, Alaina, additional, Rafelski, Marc, additional, Malkan, Matthew, additional, Teplitz, Harry, additional, Dai, Y. Sophia, additional, Baronchelli, Ivano, additional, Colbert, James, additional, Rutkowski, Michael, additional, Mehta, Vihang, additional, Dressler, Alan, additional, McCarthy, Patrick, additional, Bunker, Andrew, additional, Atek, Hakim, additional, Garel, Thibault, additional, Martin, Crystal L., additional, Hathi, Nimish, additional, and Siana, Brian, additional

Published
2017
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28. ALMA MEASUREMENTS OF CIRCUMSTELLAR MATERIAL IN THE GQ LUP SYSTEM

Author

MacGregor, Meredith A., primary, Wilner, David J., additional, Czekala, Ian, additional, Andrews, Sean M., additional, Dai, Y. Sophia, additional, Herczeg, Gregory J., additional, Kratter, Kaitlin M., additional, Kraus, Adam L., additional, Ricci, Luca, additional, and Testi, Leonardo, additional

Published
2017
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29. THE ROLE OF QUENCHING TIME IN THE EVOLUTION OF THE MASS–SIZE RELATION OF PASSIVE GALAXIES FROM THE WISP SURVEY

Author

Zanella, A., primary, Scarlata, C., additional, Corsini, E. M., additional, Bedregal, A. G., additional, Bontà, E. Dalla, additional, Atek, H., additional, Bunker, A. J., additional, Colbert, J ., additional, Dai, Y. S., additional, Henry, A., additional, Malkan, M., additional, Martin, C., additional, Rafelski, M., additional, Rutkowski, M. J., additional, Siana, B., additional, and Teplitz, H., additional

Published
2016
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30. PREDICTING THE REDSHIFT 2 HαLUMINOSITY FUNCTION USING [O iii] EMISSION LINE GALAXIES

Author

Mehta, Vihang, primary, Scarlata, Claudia, additional, Colbert, James W., additional, Dai, Y. S., additional, Dressler, Alan, additional, Henry, Alaina, additional, Malkan, Matt, additional, Rafelski, Marc, additional, Siana, Brian, additional, Teplitz, Harry I., additional, Bagley, Micaela, additional, Beck, Melanie, additional, Ross, Nathaniel R., additional, Rutkowski, Michael, additional, and Wang, Yun, additional

Published
2015
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33. HerMES: SPECTRAL ENERGY DISTRIBUTIONS OF SUBMILLIMETER GALAXIES ATz> 4

Author

Huang, J.-S., primary, Rigopoulou, D., additional, Magdis, G., additional, Rowan-Robinson, M., additional, Dai, Y., additional, Bock, J. J., additional, Burgarella, D., additional, Chapman, S., additional, Clements, D. L., additional, Cooray, A., additional, Farrah, D., additional, Glenn, J., additional, Oliver, S., additional, Smith, A. J., additional, Wang, L., additional, Page, M., additional, Riechers, D., additional, Roseboom, I., additional, Symeonidis, M., additional, Fazio, G. G., additional, Yun, M., additional, Webb, T. M. A., additional, and Efstathiou, A., additional

Published
2014
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36. A POPULATION OF DUST-RICH QUASARS ATz∼ 1.5

Author

Dai, Y. Sophia, primary, Bergeron, Jacqueline, additional, Elvis, Martin, additional, Omont, Alain, additional, Huang, Jia-Sheng, additional, Bock, Jamie, additional, Cooray, Asantha, additional, Fazio, Giovanni, additional, Hatziminaoglou, Evanthia, additional, Ibar, Edo, additional, Magdis, Georgios E., additional, Oliver, Seb J., additional, Page, Mathew J., additional, Perez-Fournon, Ismael, additional, Rigopoulou, Dimitra, additional, Roseboom, Isaac G., additional, Scott, Douglas, additional, Symeonidis, Myrto, additional, Trichas, Markos, additional, Vieira, Joaquin D., additional, Willmer, Christopher N. A., additional, and Zemcov, Michael, additional

Published
2012
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