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1. JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334

Author: Tahani, Mehrnoosh, Bastien, Pierre, Furuya, Ray S., Pattle, Kate, Johnstone, Doug, Arzoumanian, Doris, Doi, Yasuo, Hasegawa, Tetsuo, Inutsuka, Shu-ichiro, Coudé, Simon, Fissel, Laura, Chen, Michael Chun-Yuan, Poidevin, Frédérick, Sadavoy, Sarah, Friesen, Rachel, Koch, Patrick M., Di Francesco, James, Moriarty-Schieven, Gerald H., Chen, Zhiwei, Chung, Eun Jung, Eswaraiah, Chakali, Fanciullo, Lapo, Gledhill, Tim, Gouellec, Valentin J. M. Le, Hoang, Thiem, Hwang, Jihye, Kang, Ji-hyun, Kim, Kyoung Hee, Kirchschlager, Florian, Kwon, Woojin, Lee, Chang Won, Liu, Hong-Li, Onaka, Takashi, Rawlings, Mark G., Soam, Archana, Tamura, Motohide, Tang, Xindi, Tomisaka, Kohji, Whitworth, Anthony P., Kwon, Jungmi, Hoang, Thuong D., Redman, Matt, Berry, David, Ching, Tao-Chung, Wang, Jia-Wei, Lai, Shih-Ping, Qiu, Keping, Ward-Thompson, Derek, Houde, Martin, Byun, Do-Young, Chen, Huei-Ru Vivien, Chen, Wen Ping, Cho, Jungyeon, Choi, Minho, Choi, Yunhee, Chrysostomou, Antonio, Diep, Pham Ngoc, Duan, Hao-Yuan, Fiege, Jason, Franzmann, Erica, Friberg, Per, Fuller, Gary, Graves, Sarah F., Greaves, Jane S., Griffin, Matt J., Gu, Qilao, Han, Ilseung, Hatchell, Jennifer, Hayashi, Saeko S., Hull, Charles L. H., Inoue, Tsuyoshi, Iwasaki, Kazunari, Jeong, Il-Gyo, Kanamori, Yoshihiro, Kang, Miju, Kang, Sung-ju, Kataoka, Akimasa, Kawabata, Koji S., Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo Hee, Kim, Kee-Tae, Kim, Mi-Ryang, Kim, Shinyoung, Kirk, Jason M., Kobayashi, Masato I. N., Konyves, Vera, Kusune, Takayoshi, Lacaille, Kevin, Law, Chi-Yan, Lee, Chin-Fei, Lee, Hyeseung, Lee, Jeong-Eun, Lee, Sang-Sung, Lee, Yong-Hee, Li, Dalei, Li, Di, Li, Hua-bai, Liu, Junhao, Liu, Sheng-Yuan, Liu, Tie, de Looze, Ilse, Lyo, A-Ran, Mairs, Steve, Matsumura, Masafumi, Matthews, Brenda C., Nagata, Tetsuya, Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Park, Geumsook, Parsons, Harriet, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Rao, Ramprasad, Retter, Brendan, Richer, John, Rigby, Andrew, Saito, Hiro, Savini, Giorgio, Scaife, Anna M. M., Seta, Masumichi, Shimajiri, Yoshito, Shinnaga, Hiroko, Tang, Ya-Wen, Tsukamoto, Yusuke, Viti, Serena, Wang, Hongchi, Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Yun, Hyeong-Sik, Zenko, Tetsuya, Zhang, Chuan-Peng, Zhang, Guoyin, Zhang, Yapeng, Zhou, Jianjun, Zhu, Lei, André, Philippe, Dowell, C. Darren, Eyres, Stewart P. S., Falle, Sam, van Loo, Sven, and Robitaille, Jean-François
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We study the HII regions associated with the NGC 6334 molecular cloud observed in the sub-millimeter and taken as part of the B-fields In STar-forming Region Observations (BISTRO) Survey. In particular, we investigate the polarization patterns and magnetic field morphologies associated with these HII regions. Through polarization pattern and pressure calculation analyses, several of these bubbles indicate that the gas and magnetic field lines have been pushed away from the bubble, toward an almost tangential (to the bubble) magnetic field morphology. In the densest part of NGC 6334, where the magnetic field morphology is similar to an hourglass, the polarization observations do not exhibit observable impact from HII regions. We detect two nested radial polarization patterns in a bubble to the south of NGC 6334 that correspond to the previously observed bipolar structure in this bubble. Finally, using the results of this study, we present steps (incorporating computer vision; circular Hough Transform) that can be used in future studies to identify bubbles that have physically impacted magnetic field lines., Comment: Accepted for publication in Astrophysical Journal (ApJ)
Published: 2022
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2. Quantifying Variability of YSOs in the Mid-IR Over Six Years with NEOWISE

Author: Park, Wooseok, Lee, Jeong-Eun, Peña, Carlos Contreras, Johnstone, Doug, Herczeg, Gregory, Lee, Sieun, Lee, Seonjae, Bhardwaj, Anupam, and Moriarty-Schieven, Gerald H.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Variability in young stellar objects (YSOs) can be caused by various time-dependent phenomena associated with star formation, including accretion rates, geometric changes in the circumstellar disks, stochastic hydromagnetic interactions between stellar surfaces and inner disk edges, reconnections within the stellar magnetosphere, and hot/cold spots on stellar surfaces. We uncover and characterize $\sim$1700 variables from a sample of $\sim$5400 YSOs in nearby low-mass star-forming regions using mid-IR light curves obtained from the 6.5-years NEOWISE All Sky Survey. The mid-IR variability traces a wide range of dynamical, physical, and geometrical phenomenon. We classify six types of YSO mid-IR variability based on their light curves: secular variability ($Linear, Curved, Periodic$) and stochastic variability ($Burst, Drop, Irregular$). YSOs in earlier evolutionary stages have higher fractions of variables and higher amplitudes for the variability, with the recurrence timescale of FUor-type outbursts (defined here as $\Delta$W1 or $\Delta$W2 $>1$ mag followed by inspection of candidates) of $\sim$1000 years in the early embedded protostellar phase. Known eruptive young stars and subluminous objects show fractions of variables similar to the fraction ($\sim55\%$) found in typical protostars, suggesting that these two distinct types are not distinct in variability over the 6.5-year timescale. Along with brightness variability, we also find a diverse range of secular color variations, which can be attributed to a competitive interplay between the variable accretion luminosity of the central source and the variable extinction by material associated with the accretion process., Comment: Accepted for publication in ApJ
Published: 2021
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3. The JCMT Transient Survey: Four Year Summary of Monitoring the Submillimeter Variability of Protostars

Author: Lee, Yong-Hee, Johnstone, Doug, Lee, Jeong-Eun, Herczeg, Gregory, Mairs, Steve, Contreras-Peña, Carlos, Hatchell, Jennifer, Naylor, Tim, Bell, Graham S., Bourke, Tyler L., Broughton, Colton, Francis, Logan, Gupta, Aashish, Harsono, Daniel, Liu, Sheng-Yuan, Park, Geumsook, Plovie, Spencer, Moriarty-Schieven, Gerald H., Scholz, Aleks, Sharma, Tanvi, Teixeira, Paula Stella, Wang, Yao-Te, Aikawa, Yuri, Bower, Geoffrey C., Chen, Huei-Ru Vivien, Bae, Jaehan, Baek, Giseon, Chapman, Scott, Chen, Wen Ping, Du, Fujun, Dutta, Somnath, Forbrich, Jan, Guo, Zhen, Inutsuka, Shu-ichiro, Kang, Miju, Kirk, Helen, Kuan, Yi-Jehng, Kwon, Woojin, Lai, Shih-Ping, Lalchand, Bhavana, Lane, James M. M., Lee, Chin-Fei, Liu, Tie, Morata, Oscar, Pearson, Samuel, Pon, Andy, Sahu, Dipen, Shang, Hsien, Stamatellos, Dimitris, Tang, Shih-Yun, Xu, Ziyan, and Yoo, Hyunju
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: We present the four-year survey results of monthly submillimeter monitoring of eight nearby ($< 500 $pc) star-forming regions by the JCMT Transient Survey. We apply the Lomb-Scargle Periodogram technique to search for and characterize variability on 295 submillimeter peaks brighter than 0.14 Jy beam$^{-1}$, including 22 disk sources (Class II), 83 protostars (Class 0/I), and 190 starless sources. We uncover 18 secular variables, all of them protostars. No single-epoch burst or drop events and no inherently stochastic sources are observed. We classify the secular variables by their timescales into three groups: Periodic, Curved, and Linear. For the Curved and Periodic cases, the detectable fractional amplitude, with respect to mean peak brightness, is $\sim4$ % for sources brighter than $\sim$ 0.5 Jy beam$^{-1}$. Limiting our sample to only these bright sources, the observed variable fraction is 37 % (16 out of 43). Considering source evolution, we find a similar fraction of bright variables for both Class 0 and Class I. Using an empirically motivated conversion from submillimeter variability to variation in mass accretion rate, six sources (7 % of our full sample) are predicted to have years-long accretion events during which the excess mass accreted reaches more than 40 % above the total quiescently accreted mass: two previously known eruptive Class I sources, V1647 Ori and EC 53 (V371 Ser), and four Class 0 sources, HOPS 356, HOPS 373, HOPS 383, and West 40. Considering the full protostellar ensemble, the importance of episodic accretion on few years timescale is negligible, only a few percent of the assembled mass. However, given that this accretion is dominated by events of order the observing time-window, it remains uncertain as to whether the importance of episodic events will continue to rise with decades-long monitoring., Comment: Accepted for publication in the Astrophysical Journal
Published: 2021
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4. The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333

Author: Doi, Yasuo, Hasegawa, Tetsuo, Furuya, Ray S., Coudé, Simon, Hull, Charles L. H., Arzoumanian, Doris, Bastien, Pierre, Chen, Michael Chun-Yuan, di Francesco, James, Friesen, Rachel, Houde, Martin, Inutsuka, Shu-ichiro, Mairs, Steve, Matsumura, Masafumi, Onaka, Takashi, Sadavoy, Sarah, Shimajiri, Yoshito, Tahani, Mehrnoosh, Tomisaka, Kohji, Eswaraiah, Chakali, Koch, Patrick M., Pattle, Kate, Lee, Chang Won, Tamura, Motohide, Berry, David, Ching, Tao-Chung, Hwang, Jihye, Kwon, Woojin, Soam, Archana, Wang, Jia-Wei, Lai, Shih-Ping, Qiu, Keping, Ward-Thompson, Derek, Byun, Do-Young, Chen, Huei-Ru V., Chen, Wen Ping, Chen, Zhiwei, Cho, Jungyeon, Choi, Minho, Choi, Yunhee, Chrysostomou, Antonio, Chung, Eun Jung, Diep, Pham Ngoc, Duan, Hao-Yuan, Fanciullo, Lapo, Fiege, Jason, Franzmann, Erica, Friberg, Per, Fuller, Gary, Gledhill, Tim, Graves, Sarah F., Greaves, Jane S., Griffin, Matt J., Gu, Qilao, Han, Ilseung, Hatchell, Jennifer, Hayashi, Saeko S., Hoang, Thiem, Inoue, Tsuyoshi, Iwasaki, Kazunari, Jeong, Il-Gyo, Johnstone, Doug, Kanamori, Yoshihiro, Kang, Ji-hyun, Kang, Miju, Kang, Sung-Ju, Kataoka, Akimasa, Kawabata, Koji S., Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo, Kim, Kee-Tae, Kim, Kyoung Hee, Kim, Mi-Ryang, Kim, Shinyoung, Kirk, Jason M., Kobayashi, Masato I. N., Konyves, Vera, Kusune, Takayoshi, Kwon, Jungmi, Lacaille, Kevin, Law, Chi-Yan, Lee, Chin-Fei, Lee, Hyeseung, Lee, Jeong-Eun, Lee, Sang-Sung, Lee, Yong-Hee, Li, Dalei, Li, Di, Li, Hua-Bai, Liu, Hong-Li, Liu, Junhao, Liu, Sheng-Yuan, Liu, Tie, de Looze, Ilse, Lyo, A-Ran, Matthews, Brenda C., Moriarty-Schieven, Gerald H., Nagata, Tetsuya, Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Park, Geumsook, Parsons, Harriet, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Rao, Ramprasad, Rawlings, Mark G., Retter, Brendan, Richer, John, Rigby, Andrew, Saito, Hiro, Savini, Giorgio, Scaife, Anna M. M., Seta, Masumichi, Shinnaga, Hiroko, Tang, Ya-Wen, Tsukamoto, Yusuke, Viti, Serena, Wang, Hongchi, Whitworth, Anthony P., Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Yun, Hyeong-Sik, Zenko, Tetsuya, Zhang, Chuan-Peng, Zhang, Guoyin, Zhang, Yapeng, Zhou, Jianjun, Zhu, Lei, André, Philippe, Dowell, C. Darren, Eyres, Stewart P. S., Falle, Sam, van Loo, Sven, and Robitaille, Jean-François
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present new observations of the active star-formation region NGC 1333 in the Perseus molecular cloud complex from the James Clerk Maxwell Telescope B-Fields In Star-forming Region Observations (BISTRO) survey with the POL-2 instrument. The BISTRO data cover the entire NGC 1333 complex (~1.5 pc x 2 pc) at 0.02 pc resolution and spatially resolve the polarized emission from individual filamentary structures for the first time. The inferred magnetic field structure is complex as a whole, with each individual filament aligned at different position angles relative to the local field orientation. We combine the BISTRO data with low- and high- resolution data derived from Planck and interferometers to study the multiscale magnetic field structure in this region. The magnetic field morphology drastically changes below a scale of ~1 pc and remains continuous from the scales of filaments (~0.1 pc) to that of protostellar envelopes (~0.005 pc or ~1000 au). Finally, we construct simple models in which we assume that the magnetic field is always perpendicular to the long axis of the filaments. We demonstrate that the observed variation of the relative orientation between the filament axes and the magnetic field angles are well reproduced by this model, taking into account the projection effects of the magnetic field and filaments relative to the plane of the sky. These projection effects may explain the apparent complexity of the magnetic field structure observed at the resolution of BISTRO data toward the filament network., Comment: 33 pages, 21 figures, accepted for publication in ApJ
Published: 2020
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5. The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region

Author: Coudé, Simon, Bastien, Pierre, Houde, Martin, Sadavoy, Sarah, Friesen, Rachel, Di Francesco, James, Johnstone, Doug, Mairs, Steve, Hasegawa, Tetsuo, Kwon, Woojin, Lai, Shih-Ping, Qiu, Keping, Ward-Thompson, Derek, Berry, David, Chen, Michael Chun-Yuan, Fiege, Jason, Franzmann, Erica, Hatchell, Jennifer, Lacaille, Kevin, Matthews, Brenda C., Moriarty-Schieven, Gerald H., Pon, Andy, André, Philippe, Arzoumanian, Doris, Aso, Yusuke, Byun, Do-Young, Chakali, Eswaraiah, Chen, Huei-Ru, Chen, Wen Ping, Ching, Tao-Chung, Cho, Jungyeon, Choi, Minho, Chrysostomou, Antonio, Chung, Eun Jung, Doi, Yasuo, Drabek-Maunder, Emily, Dowell, C. Darren, Eyres, Stewart P. S., Falle, Sam, Friberg, Per, Fuller, Gary, Furuya, Ray S., Gledhill, Tim, Graves, Sarah F., Greaves, Jane S., Griffin, Matt J., Gu, Qilao, Hayashi, Saeko S., Hoang, Thiem, Holland, Wayne, Inoue, Tsuyoshi, Inutsuka, Shu-ichiro, Iwasaki, Kazunari, Jeong, Il-Gyo, Kanamori, Yoshihiro, Kataoka, Akimasa, Kang, Ji-hyun, Kang, Miju, Kang, Sung-ju, Kawabata, Koji S., Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo, Kim, Kee-Tae, Kim, Kyoung Hee, Kim, Mi-Ryang, Kim, Shinyoung, Kirk, Jason M., Kobayashi, Masato I. N., Koch, Patrick M., Kwon, Jungmi, Lee, Jeong-Eun, Lee, Chang Won, Lee, Sang-Sung, Li, Dalei, Li, Di, Li, Hua-bai, Liu, Hong-Li, Liu, Junhao, Liu, Sheng-Yuan, Liu, Tie, van Loo, Sven, Lyo, A-Ran, Matsumura, Masafumi, Nagata, Tetsuya, Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Onaka, Takashi, Parsons, Harriet, Pattle, Kate, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Rao, Ramprasad, Rawlings, Mark G., Retter, Brendan, Richer, John, Rigby, Andrew, Robitaille, Jean-François, Saito, Hiro, Savini, Giorgio, Scaife, Anna M. M., Seta, Masumichi, Shinnaga, Hiroko, Soam, Archana, Tamura, Motohide, Tang, Ya-Wen, Tomisaka, Kohji, Tsukamoto, Yusuke, Wang, Hongchi, Wang, Jia-Wei, Whitworth, Anthony P., Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Zenko, Tetsuya, Zhang, Chuan-Peng, Zhang, Guoyin, Zhou, Jianjun, and Zhu, Lei
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the POL-2 850 $\mu$m linear polarization map of the Barnard 1 clump in the Perseus molecular cloud complex from the B-fields In STar-forming Region Observations (BISTRO) survey at the James Clerk Maxwell Telescope. We find a trend of decreasing polarization fraction as a function of total intensity, which we link to depolarization effects towards higher density regions of the cloud. We then use the polarization data at 850 $\mu$m to infer the plane-of-sky orientation of the large-scale magnetic field in Barnard 1. This magnetic field runs North-South across most of the cloud, with the exception of B1-c where it turns more East-West. From the dispersion of polarization angles, we calculate a turbulence correlation length of $5.0 \pm 2.5$ arcsec ($1500$ au), and a turbulent-to-total magnetic energy ratio of $0.5 \pm 0.3$ inside the cloud. We combine this turbulent-to-total magnetic energy ratio with observations of NH$_3$ molecular lines from the Green Bank Ammonia Survey (GAS) to estimate the strength of the plane-of-sky component of the magnetic field through the Davis-Chandrasekhar-Fermi method. With a plane-of-sky amplitude of $120 \pm 60$ $\mu$G and a criticality criterion $\lambda_c = 3.0 \pm 1.5$, we find that Barnard 1 is a supercritical molecular cloud with a magnetic field nearly dominated by its turbulent component., Comment: 22 pages, 7 figures, accepted in the Astrophysical Journal
Published: 2019
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6. The JCMT BISTRO Survey: The Magnetic Field In The Starless Core $\rho$ Ophiuchus C

Author: Liu, Junhao, Qiu, Keping, Berry, David, Di Francesco, James, Bastien, Pierre, Koch, Patrick M., Furuya, Ray S., Kim, Kee-Tae, Coudé, Simon, Lee, Chang Won, Soam, Archana, Eswaraiah, Chakali, Li, Di, Hwang, Jihye, Lyo, A-Ran, Pattle, Kate, Hasegawa, Tetsuo, Kwon, Woojin, Lai, Shih-Ping, Ward-Thompson, Derek, Ching, Tao-Chung, Chen, Zhiwei, Gu, Qilao, Li, Dalei, Li, Hua-bai, Liu, Hong-Li, Qian, Lei, Wang, Hongchi, Yuan, Jinghua, Zhang, Chuan-Peng, Zhang, Guoyin, Zhang, Ya-Peng, Zhou, Jianjun, Zhu, Lei, André, Philippe, Arzoumanian, Doris, Aso, Yusuke, Byun, Do-Young, Chen, Michael Chun-Yuan, Chen, Huei-Ru Vivien, Chen, Wen Ping, Cho, Jungyeon, Choi, Minho, Chrysostomou, Antonio, Chung, Eun Jung, Doi, Yasuo, Drabek-Maunder, Emily, Dowell, C. Darren, Eyres, Stewart P. S., Falle, Sam, Fanciullo, Lapo, Fiege, Jason, Franzmann, Erica, Friberg, Per, Friesen, Rachel K., Fuller, Gary, Gledhill, Tim, Graves, Sarah F., Greaves, Jane S., Griffin, Matt J., Han, Ilseung, Hatchell, Jennifer, Hayashi, Saeko S., Hoang, Thiem, Holland, Wayne, Houde, Martin, Inoue, Tsuyoshi, Inutsuka, Shu-ichiro, Iwasaki, Kazunari, Jeong, Il-Gyo, Johnstone, Doug, Kanamori, Yoshihiro, Kang, Ji-hyun, Kang, Miju, Kang, Sung-ju, Kataoka, Akimasa, Kawabata, Koji S., Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo, Kim, Kyoung Hee, Kim, Mi-Ryang, Kim, Shinyoung, Kirk, Jason M., Kobayashi, Masato I. N., Kusune, Takayoshi, Kwon, Jungmi, Lacaille, Kevin M., Lee, Chin-Fei, Lee, Jeong-Eun, Lee, Hyeseung, Lee, Sang-Sung, Liu, Sheng-Yuan, Liu, Tie, van Loo, Sven, Mairs, Steve, Matsumura, Masafumi, Matthews, Brenda C., Moriarty-Schieven, Gerald H., Nagata, Tetsuya, Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Onaka, Takashi, Parker, Josh, Parsons, Harriet, Pascale, Enzo, Peretto, Nicolas, Pon, Andy, Pyo, Tae-Soo, Rao, Ramprasad, Rawlings, Mark G., Retter, Brendan, Richer, John, Rigby, Andrew, Robitaille, Jean-François, Sadavoy, Sarah, Saito, Hiro, Savini, Giorgio, Scaife, Anna M. M., Seta, Masumichi, Shinnaga, Hiroko, Tamura, Motohide, Tang, Ya-Wen, Tomisaka, Kohji, Tsukamoto, Yusuke, Wang, Jia-Wei, Whitworth, Anthony P., Yen, Hsi-Wei, Yoo, Hyunju, and Zenko, Tetsuya
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: We report 850~$\mu$m dust polarization observations of a low-mass ($\sim$12 $M_{\odot}$) starless core in the $\rho$ Ophiuchus cloud, Ophiuchus C, made with the POL-2 instrument on the James Clerk Maxwell Telescope (JCMT) as part of the JCMT B-fields In STar-forming Region Observations (BISTRO) survey. We detect an ordered magnetic field projected on the plane of sky in the starless core. The magnetic field across the $\sim$0.1~pc core shows a predominant northeast-southwest orientation centering between $\sim$40$^\circ$ to $\sim$100$^\circ$, indicating that the field in the core is well aligned with the magnetic field in lower-density regions of the cloud probed by near-infrared observations and also the cloud-scale magnetic field traced by Planck observations. The polarization percentage ($P$) decreases with an increasing total intensity ($I$) with a power-law index of $-$1.03 $\pm$ 0.05. We estimate the plane-of-sky field strength ($B_{\mathrm{pos}}$) using modified Davis-Chandrasekhar-Fermi (DCF) methods based on structure function (SF), auto-correlation (ACF), and unsharp masking (UM) analyses. We find that the estimates from the SF, ACF, and UM methods yield strengths of 103 $\pm$ 46 $\mu$G, 136 $\pm$ 69 $\mu$G, and 213 $\pm$ 115 $\mu$G, respectively. Our calculations suggest that the Ophiuchus C core is near magnetically critical or slightly magnetically supercritical (i.e. unstable to collapse). The total magnetic energy calculated from the SF method is comparable to the turbulent energy in Ophiuchus C, while the ACF method and the UM method only set upper limits for the total magnetic energy because of large uncertainties., Comment: 22 pages, 12 figures
Published: 2019
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7. JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146

Author: Wang, Jia-Wei, Lai, Shih-Ping, Eswaraiah, Chakali, Pattle, Kate, Di Francesco, James, Johnstone, Doug, Koch, Patrick M., Liu, Tie, Tamura, Motohide, Furuya, Ray S., Onaka, Takashi, Ward-Thompson, Derek, Soam, Archana, Kim, Kee-Tae, Lee, Chang Won, Lee, Chin-Fei, Mairs, Steve, Arzoumanian, Doris, Kim, Gwanjeong, Hoang, Thiem, Hwang, Jihye, Liu, Sheng-Yuan, Berry, David, Bastien, Pierre, Hasegawa, Tetsuo, Kwon, Woojin, Qiu, Keping, André, Philippe, Aso, Yusuke, Byun, Do-Young, Chen, Huei-Ru, Chen, Michael C., Chen, Wen Ping, Ching, Tao-Chung, Cho, Jungyeon, Choi, Minho, Chrysostomou, Antonio, Chung, Eun Jung, Coudé, Simon, Doi, Yasuo, Dowell, C. Darren, Drabek-Maunder, Emily, Duan, Hao-Yuan, Eyres, Stewart P. S., Falle, Sam, Fanciullo, Lapo, Fiege, Jason, Franzmann, Erica, Friberg, Per, Friesen, Rachel K., Fuller, Gary, Gledhill, Tim, Graves, Sarah F., Greaves, Jane S., Griffin, Matt J., Gu, Qilao, Han, Ilseung, Hatchell, Jennifer, Hayashi, Saeko S., Holland, Wayne, Houde, Martin, Inoue, Tsuyoshi, Inutsuka, Shu-ichiro, Iwasaki, Kazunari, Jeong, Il-Gyo, Kanamori, Yoshihiro, Kang, Ji-hyun, Kang, Miju, Kang, Sung-ju, Kataoka, Akimasa, Kawabata, Koji S., Kemper, Francisca, Kim, Jongsoo, Kim, Kyoung Hee, Kim, Mi-Ryang, Kim, Shinyoung, Kirk, Jason M., Kobayashi, Masato I. N., Konyves, Vera, Kwon, Jungmi, Lacaille, Kevin M., Lee, Hyeseung, Lee, Jeong-Eun, Lee, Sang-Sung, Lee, Yong-Hee, Li, Dalei, Li, Di, Li, Hua-bai, Liu, Hong-Li, Liu, Junhao, Lyo, A-Ran, Matsumura, Masafumi, Matthews, Brenda C., Moriarty-Schieven, Gerald H., Nagata, Tetsuya, Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Park, Geumsook, Parsons, Harriet, Pascale, Enzo, Peretto, Nicolas, Pon, Andy, Pyo, Tae-Soo, Qian, Lei, Rao, Ramprasad, Rawlings, Mark G., Retter, Brendan, Richer, John, Rigby, Andrew, Robitaille, Jean-François, Sadavoy, Sarah, Saito, Hiro, Savini, Giorgio, Scaife, Anna M. M., Seta, Masumichi, Shinnaga, Hiroko, Tang, Ya-Wen, Tomisaka, Kohji, Tsukamoto, Yusuke, van Loo, Sven, Wang, Hongchi, Whitworth, Anthony P., Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Yun, Hyeong-Sik, Zenko, Tetsuya, Zhang, Chuan-Peng, Zhang, Guoyin, Zhang, Ya-Peng, Zhou, Jianjun, and Zhu
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the 850 $\mu$m polarization observations toward the IC5146 filamentary cloud taken using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and its associated polarimeter (POL-2), mounted on the James Clerk Maxwell Telescope (JCMT), as part of the B-fields In STar forming Regions Observations (BISTRO). This work is aimed at revealing the magnetic field morphology within a core-scale ($\lesssim 1.0$ pc) hub-filament structure (HFS) located at the end of a parsec-scale filament. To investigate whether or not the observed polarization traces the magnetic field in the HFS, we analyze the dependence between the observed polarization fraction and total intensity using a Bayesian approach with the polarization fraction described by the Rice likelihood function, which can correctly describe the probability density function (PDF) of the observed polarization fraction for low signal-to-noise ratio (SNR) data. We find a power-law dependence between the polarization fraction and total intensity with an index of 0.56 in $A_V\sim$ 20--300 mag regions, suggesting that the dust grains in these dense regions can still be aligned with magnetic fields in the IC5146 regions. Our polarization maps reveal a curved magnetic field, possibly dragged by the contraction along the parsec-scale filament. We further obtain a magnetic field strength of 0.5$\pm$0.2 mG toward the central hub using the Davis-Chandrasekhar-Fermi method, corresponding to a mass-to-flux criticality of $\sim$ $1.3\pm0.4$ and an Alfv\'{e}nic Mach number of $<$0.6. These results suggest that gravity and magnetic field is currently of comparable importance in the HFS, and turbulence is less important., Comment: 24 pages, 15 figures, accepted for publication in ApJ
Published: 2018
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8. Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements

Author: Soam, Archana, Pattle, Kate, Ward-Thompson, Derek, Lee, Chang Won, Sadavoy, Sarah, Koch, Patrick M., Kim, Gwanjeong, Kwon, Jungmi, Kwon, Woojin, Arzoumanian, Doris, Berry, David, Hoang, Thiem, Tamura, Motohide, Lee, Sang-Sung, Liu, Tie, Kim, Kee-Tae, Johnstone, Doug, Nakamura, Fumitaka, Lyo, A-Ran, Onaka, Takashi, Kim, Jongsoo, Furuya, Ray S., Hasegawa, Tetsuo, Lai, Shih-Ping, Bastien, Pierre, Chung, Eun Jung, Kim, Shinyoung, Parsons, Harriet, Rawlings, Mark, Mairs, Steve, Graves, Sarah F., Robitaille, J. -F., Liu, Hong-Li, Whitworth, Anthony P., Eswaraiah, Chakali, Rao, Ramprasad, Yoo, Hyunju, Houde, Martin, Kang, Ji-hyun, Doi, Yasuo, Choi, Minho, Kang, Miju, Coude, Simon, Li, Hua-bai, Matsumura, Masafumi, Matthews, Brenda C., Pon, Andy, Di Francesco, James, Hayashi, Saeko S., Kawabata, Koji S., Inutsuka, Shu-ichiro, Qiu, Keping, Franzmann, Erica, Friberg, Per, Greaves, Jane S., Kirk, Jason M., Li, Di, Shinnaga, Hiroko, van Loo, Sven, Aso, Yusuke, Byun, Do-Young, Chen, Huei-Ru, Chen, Mike C. -Y., Chen, Wen Ping, Ching, Tao-Chung, Cho, Jungyeon, Chrysostomou, Antonio, Drabek-Maunder, Emily, Eyres, Stewart P. S., Fiege, Jason, Friesen, Rachel K., Fuller, Gary, Gledhill, Tim, Griffin, Matt J., Gu, Qilao, Hatchell, Jennifer, Holland, Wayne, Inoue, Tsuyoshi, Iwasaki, Kazunari, Jeong, Il-Gyo, Kang, Sung-ju, Kemper, Francisca, Kim, Kyoung Hee, Kim, Mi-Ryang, Lacaille, Kevin M., Lee, Jeong-Eun, Li, Dalei, Liu, Junhao, Liu, Sheng-Yuan, Moriarty-Schieven, Gerald H., Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Retter, Brendan, Richer, John, Rigby, Andrew, Savini, Giorgio, Scaife, Anna M. M., Tang, Ya-Wen, Tomisaka, Kohji, Wang, Hongchi, Wang, Jia-Wei, Yen, Hsi-Wei, Yuan, Jinghua, Zhang, Chuan-Peng, Zhang, Guoyin, Zhou, Jianjun, Zhu, Lei, Andre, Philippe, Dowell, C. Darren, Falle, Sam, Tsukamoto, Yusuke, Kanamori, Yoshihiro, Kataoka, Akimasa, Kobayashi, Masato I. N., Nagata, Tetsuya, Saito, Hiro, Seta, Masumichi, Hwang, Jihye, Han, Ilseung, Lee, Hyeseung, and Zenko, Tetsuya
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the results of dust emission polarization measurements of Ophiuchus-B (Oph-B) carried out using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) camera with its associated polarimeter (POL-2) on the James Clerk Maxwell Telescope (JCMT) in Hawaii. This work is part of the B-fields In Star-forming Region Observations (BISTRO) survey initiated to understand the role of magnetic fields in star formation for nearby star-forming molecular clouds. We present a first look at the geometry and strength of magnetic fields in Oph-B. The field geometry is traced over $\sim$0.2 pc, with clear detection of both of the sub-clumps of Oph-B. The field pattern appears significantly disordered in sub-clump Oph-B1. The field geometry in Oph-B2 is more ordered, with a tendency to be along the major axis of the clump, parallel to the filamentary structure within which it lies. The degree of polarization decreases systematically towards the dense core material in the two sub-clumps. The field lines in the lower density material along the periphery are smoothly joined to the large scale magnetic fields probed by NIR polarization observations. We estimated a magnetic field strength of 630$\pm$410 $\mu$G in the Oph-B2 sub-clump using a Davis-Chandeasekhar-Fermi analysis. With this magnetic field strength, we find a mass-to-flux ratio $\lambda$= 1.6$\pm$1.1, which suggests that the Oph-B2 clump is slightly magnetically supercritical., Comment: 17 pages, 10 figures, Accepted for publication in ApJ
Published: 2018
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9. A First Look at BISTRO Observations of The $\rho$ Oph-A core

Author: Kwon, Jungmi, Doi, Yasuo, Tamura, Motohide, Matsumura, Masafumi, Pattle, Kate, Berry, David, Sadavoy, Sarah, Matthews, Brenda C., Ward-Thompson, Derek, Hasegawa, Tetsuo, Furuya, Ray S., Pon, Andy, Di Francesco, James, Arzoumanian, Doris, Hayashi, Saeko S., Kawabata, Koji S., Onaka, Takashi, Choi, Minho, Kang, Miju, Hoang, Thiem, Lee, Chang Won, Lee, Sang-Sung, Liu, Hong-Li, Liu, Tie, Inutsuka, Shu-Ichiro, Eswaraiah, Chakali, Bastien, Pierre, Kwon, Woojin, Lai, Shih-Ping, Qiu, Keping, Coude, Simon, Franzmann, Erica, Friberg, Per, Graves, Sarah F., Greaves, Jane S., Houde, Martin, Johnstone, Doug, Kirk, Jason M., Koch, Patrick M., Li, Di, Parsons, Harriet, Rao, Ramprasad, Rawlings, Mark, Shinnaga, Hiroko, Van Loo, Sven, Aso, Yusuke, Byun, Do-Young, Chen, Huei-Ru, Chen, Mike C. -Y., Chen, Wen Ping, Ching, Tao-Chung, Cho, Jungyeon, Chrysostomou, Antonio, Chung, Eun Jung, Drabek-Maunder, Emily, Eyres, Stewart P. S., Fiege, Jason, Friesen, Rachel K., Fuller, Gary, Gledhill, Tim, Griffin, Matt J., Gu, Qilao, Hatchell, Jennifer, Holland, Wayne, Inoue, Tsuyoshi, Iwasaki, Kazunari, Jeong, Il-Gyo, Kang, Ji-Hyun, Kang, Sung-Ju, Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo, Kim, Kee-Tae, Kim, Kyoung Hee, Kim, Mi-Ryang, Kim, Shinyoung, Lacaille, Kevin M., Lee, Jeong-Eun, Li, Dalei, Li, Hua-Bai, Liu, Junhao, Liu, Sheng-Yuan, Lyo, A-Ran, Mairs, Steve, Moriarty-Schieven, Gerald H., Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Retter, Brendan, Richer, John, Rigby, Andrew, Robitaille, Jean-Franois, Savini, Giorgio, Scaife, Anna M. M., Soam, Archana, Tang, Ya-Wen, Tomisaka, Kohji, Wang, Hongchi, Wang, Jia-Wei, Whitworth, Anthony P., Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Zhang, Chuan-Peng, Zhang, Guoyin, Zhou, Jianjun, Zhu, Lei, Andre, Philippe, Dowell, C. Darren, Falle, Sam, Tsukamoto, Yusuke, Nakagawa, Takao, Kanamori, Yoshihiro, Kataoka, Akimasa, Kobayashi, Masato I. N., Nagata, Tetsuya, Saito, Hiro, Seta, Masumichi, and Zenko, Tetsuya
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present 850 $\mu$m imaging polarimetry data of the $\rho$ Oph-A core taken with the Submillimeter Common-User Bolometer Array-2 (SCUBA-2) and its polarimeter (POL-2), as part of our ongoing survey project, BISTRO (B-fields In STar forming RegiOns). The polarization vectors are used to identify the orientation of the magnetic field projected on the plane of the sky at a resolution of 0.01 pc. We identify 10 subregions with distinct polarization fractions and angles in the 0.2 pc $\rho$ Oph A core; some of them can be part of a coherent magnetic field structure in the $\rho$ Oph region. The results are consistent with previous observations of the brightest regions of $\rho$ Oph-A, where the degrees of polarization are at a level of a few percents, but our data reveal for the first time the magnetic field structures in the fainter regions surrounding the core where the degree of polarization is much higher ($> 5 \%$). A comparison with previous near-infrared polarimetric data shows that there are several magnetic field components which are consistent at near-infrared and submillimeter wavelengths. Using the Davis-Chandrasekhar-Fermi method, we also derive magnetic field strengths in several sub-core regions, which range from approximately 0.2 to 5 mG. We also find a correlation between the magnetic field orientations projected on the sky with the core centroid velocity components., Comment: 22 pages, 11 figures, accepted for publication in ApJ
Published: 2018
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10. SONS: The JCMT legacy survey of debris discs in the submillimetre

Author: Holland, Wayne S., Matthews, Brenda C., Kennedy, Grant M., Greaves, Jane S., Wyatt, Mark C., Booth, Mark, Bastien, Pierre, Bryden, Geoff, Butner, Harold, Chen, Christine H., Chrysostomou, Antonio, Davies, Claire L., Dent, William R. F., Di Francesco, James, Duchene, Gaspard, Gibb, Andy G., Friberg, Per, Ivison, Rob J., Jenness, Tim, Kavelaars, JJ, Lawler, Samantha, Lestrade, Jean-Francois, Marshall, Jonathan P., Moro-Martin, Amaya, Panic, Olja, Phillips, Neil, Serjeant, Stephen, Schieven, Gerald H., Sibthorpe, Bruce, Vican, Laura, Ward-Thompson, Derek, van der Werf, Paul, White, Glenn J., Wilner, David, and Zuckerman, Ben
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Debris discs are evidence of the ongoing destructive collisions between planetesimals, and their presence around stars also suggests that planets exist in these systems. In this paper, we present submillimetre images of the thermal emission from debris discs that formed the SCUBA-2 Observations of Nearby Stars (SONS) survey, one of seven legacy surveys undertaken on the James Clerk Maxwell telescope between 2012 and 2015. The overall results of the survey are presented in the form of 850 microns (and 450 microns, where possible) images and fluxes for the observed fields. Excess thermal emission, over that expected from the stellar photosphere, is detected around 49 stars out of the 100 observed fields. The discs are characterised in terms of their flux density, size (radial distribution of the dust) and derived dust properties from their spectral energy distributions. The results show discs over a range of sizes, typically 1-10 times the diameter of the Edgeworth-Kuiper Belt in our Solar System. The mass of a disc, for particles up to a few millimetres in size, is uniquely obtainable with submillimetre observations and this quantity is presented as a function of the host stars' age, showing a tentative decline in mass with age. Having doubled the number of imaged discs at submillimetre wavelengths from ground-based, single dish telescope observations, one of the key legacy products from the SONS survey is to provide a comprehensive target list to observe at high angular resolution using submillimetre/millimetre interferometers (e.g., ALMA, SMA)., Comment: 61 pages, 51 figures
Published: 2017
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11. First results from BISTRO -- a SCUBA-2 polarimeter survey of the Gould Belt

Author: Ward-Thompson, Derek, Pattle, Kate, Bastien, Pierre, Furuya, Ray S., Kwon, Woojin, Lai, Shih-Ping, Qiu, Keping, Berry, David, Choi, Minho, Coudé, Simon, Di Francesco, James, Hoang, Thiem, Franzmann, Erica, Friberg, Per, Graves, Sarah F., Greaves, Jane S., Houde, Martin, Johnstone, Doug, Kirk, Jason M., Koch, Patrick M., Kwon, Jungmi, Lee, Chang Won, Li, Di, Matthews, Brenda C., Mottram, Joseph C., Parsons, Harriet, Pon, Andy, Rao, Ramprasad, Rawlings, Mark, Shinnaga, Hiroko, Sadavoy, Sarah, van Loo, Sven, Aso, Yusuke, Byun, Do-Young, Chakali, Eswariah, Chen, Huei-Ru, Chen, Mike C. -Y., Chen, Wen Ping, Ching, Tao-Chung, Cho, Jungyeon, Chrysostomou, Antonio, Chung, Eun Jung, Doi, Yasuo, Drabek-Maunder, Emily, Eyres, Stewart P. S., Fiege, Jason, Friesen, Rachel K., Fuller, Gary, Gledhill, Tim, Griffin, Matt J., Gu, Qilao, Hasegawa, Tetsuo, Hatchell, Jennifer, Hayashi, Saeko S., Holland, Wayne, Inoue, Tsuyoshi, Inutsuka, Shu-ichiro, Iwasaki, Kazunari, Jeong, Il-Gyo, Kang, Ji-hyun, Kang, Miju, Kang, Sung-ju, Kawabata, Koji S., Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo, Kim, Kee-Tae, Kim, Kyoung Hee, Kim, Mi-Ryang, Kim, Shinyoung, Lacaille, Kevin M., Lee, Jeong-Eun, Lee, Sang-Sung, Li, Dalei, Li, Hua-bai, Liu, Hong-Li, Liu, Junhao, Liu, Sheng-Yuan, Liu, Tie, Lyo, A-Ran, Mairs, Steve, Matsumura, Masafumi, Moriarty-Schieven, Gerald H., Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Onaka, Takashi, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Retter, Brendan, Richer, John, Rigby, Andrew, Robitaille, Jean-François, Savini, Giorgio, Scaife, Anna M. M., Soam, Archana, Tamura, Motohide, Tang, Ya-Wen, Tomisaka, Kohji, Wang, Hongchi, Wang, Jia-Wei, Whitworth, Anthony P., Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Zhang, Chuan-Peng, Zhang, Guoyin, Zhou, Jianjun, Zhu, Lei, André, Philippe, Dowell, C. Darren, Falle, Sam, and Tsukamoto, Yusuke
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the first results from the B-fields In STar-forming Region Observations (BISTRO) survey, using the Sub-millimetre Common-User Bolometer Array 2 (SCUBA-2) camera, with its associated polarimeter (POL-2), on the James Clerk Maxwell Telescope (JCMT) in Hawaii. We discuss the survey's aims and objectives. We describe the rationale behind the survey, and the questions which the survey will aim to answer. The most important of these is the role of magnetic fields in the star formation process on the scale of individual filaments and cores in dense regions. We describe the data acquisition and reduction processes for POL-2, demonstrating both repeatability and consistency with previous data. We present a first-look analysis of the first results from the BISTRO survey in the OMC 1 region. We see that the magnetic field lies approximately perpendicular to the famous 'integral filament' in the densest regions of that filament. Furthermore, we see an 'hour-glass' magnetic field morphology extending beyond the densest region of the integral filament into the less-dense surrounding material, and discuss possible causes for this. We also discuss the more complex morphology seen along the Orion Bar region. We examine the morphology of the field along the lower-density north-eastern filament. We find consistency with previous theoretical models that predict magnetic fields lying parallel to low-density, non-self-gravitating filaments, and perpendicular to higher-density, self-gravitating filaments., Comment: 12 pages, 8 figures, accepted for publication in ApJ
Published: 2017
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12. V2494 Cyg: A unique FU Ori type object in the Cygnus OB7 complex

Author: Magakian, Tigran Yu., Nikogossian, Elena H., Movsessian, Tigran, Moiseev, Alexei, Aspin, Colin, Davis, Chris J., Pyo, Tae-Soo, Khanzadyan, Tigran, Froebrich, Dirk, Smith, Michael D., Moriarty-Schieven, Gerald H., and Beck, Tracy L.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: A photometric and spectral study of the variable star V2494 Cyg in the L 1003 dark cloud is presented. The brightness of the star, formerly known as HH 381 IRS, increased by 2.5 mag in R (probably in the 1980s) and since then has remained nearly constant. Since the brightness increase, V2494 Cyg has illuminated a bipolar cometary nebula. The stellar spectrum has several features typical of the FU Ori type, plus it exhibits very strong Halpha and forbidden emission lines with high-velocity components. These emission lines originate in the HH jet near the star. The kinematic age of the jet is consistent with it forming at the time of the outburst leading to the luminosity increase. V2494 Cyg also produces a rather extended outflow; it is the first known FUor with both an observed outburst and a parsec-sized HH flow. The nebula, illuminated by V2494 Cyg, possesses similar morphological and spectral characteristics to Hubble's Variable Nebula (R Monocerotis/NGC 2261)., Comment: 12 pages, 5 figures. To be published in MNRAS
Published: 2013
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13. The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Author: Cooray, Asantha, Eales, Steve, Chapman, Scott, Clements, David L., Dore, Olivier, Farrah, Duncan, Jarvis, Matt J., Kaplinghat, Manoj, Negrello, Mattia, Melchiorri, Alessandro, Peiris, Hiranya, Pope, Alexandra, Santos, Mario G., Serjeant, Stephen, Thompson, Mark, White, Glenn, Amblard, Alexandre, Banerji, Manda, Corasaniti, Pier-Stefano, Das, Sudeep, de_Bernardis, Francesco, de_Zotti, Gianfranco, Giannantonio, Tommaso, Gonzalez, Joaquin Gonzalez-Nuevo, Khostovan, Ali Ahmad, Mitchell-Wynne, Ketron, Serra, Paolo, Song, Yong-Seon, Vieira, Joaquin, Wang, Lingyu, Zemcov, Michael, Abdalla, Filipe, Afonso, Jose, Aghanim, Nabila, Andreani, Paola, Aretxaga, Itziar, Auld, Robbie, Baes, Maarten, Baker, Andrew, Barkats, Denis, Barreiro, R. Belen, Bartolo, Nicola, Barton, Elizabeth, Barway, Sudhanshu, Battistelli, Elia Stefano, Baugh, Carlton, Beelen, Alexander, Benabed, Karim, Blain, Andrew, Bland-Hawthorn, Joss, Bock, James~J., Bond, J. Richard, Borrill, Julian, Borys, Colin, Boselli, Alessandro, Bouchet, Francois R., Bridge, Carrie, Brighenti, Fabrizio, Buat, Veronique, Buote, David, Burgarella, Denis, Bussmann, Robert, Calabrese, Erminia, Cantalupo, Christopher, Carlberg, Raymond, Carvalho, Carla Sofia, Casey, Caitlin, Cava, Antonio, Cepa, Jordi, Chapin, Edward, Chary, Ranga Ram, Chen, Xuelei, Colafrancesco, Sergio, Cole, Shaun, Coles, Peter, Conley, Alexander, Conversi, Luca, Cooke, Jeff, Crawford, Steven, Cress, Catherine, da Cunha, Elisabete, Dalton, Gavin, Danese, Luigi, Dannerbauer, Helmut, Davies, Jonathan, de Bernardis, Paolo, de Putter, Roland, Devlin, Mark, Diego, Jose M., Dole, Herve, Douspis, Marian, Dunkley, Joanna, Dunlop, James, Dunne, Loretta, Dunner, Rolando, Dye, Simon, Efstathiou, George, Egami, Eiichi, Fang, Taotao, Ferrero, Patrizia, Franceschini, Alberto, Frazer, Christopher C., Frayer, David, Frenk, Carlos, Ganga, Ken, Gavazzi, Raphael, Glenn, Jason, Gong, Yan, Gonzalez-Solares, Eduardo, Griffin, Matt, Guo, Qi, Gurwell, Mark, Hajian, Amir, Halpern, Mark, Hanson, Duncan, Hardcastle, Martin, Hatziminaoglou, Evanthia, Heavens, Alan, Heinis, Sebastien, Herranz, Diego, Hilton, Matt, Ho, Shirley, Holwerda, Benne W., Hopwood, Rosalind, Horner, Jonathan, Huffenberger, Kevin, Hughes, David H., Hughes, John P., Ibar, Edo, Ivison, Rob, Jackson, Neal, Jaffe, Andrew, Jenness, Timothy, Joncas, Gilles, Joudaki, Shahab, Kaviraj, Sugata, Kim, Sam, King, Lindsay, Kisner, Theodore, Knapen, Johan, Kniazev, Alexei, Komatsu, Eiichiro, Koopmans, Leon, Kuo, Chao-Lin, Lacey, Cedric, Lahav, Ofer, Lasenby, Anthony N., Lawrence, Andy, Lee, Myung Gyoon, Leeuw, Lerothodi L., Levenson, Louis R., Lewis, Geraint, Loaring, Nicola, Lopez-Caniego, Marcos, Maddox, Steve, Marriage, Tobias, Marsden, Gaelen, Martinez-Gonzalez, Enrique, Masi, Silvia, Matarrese, Sabino, Mathews, William G., Matsuura, Shuji, McMahon, Richard, Mellier, Yannick, Menanteau, Felipe, Michalowski, Michal~J., Millea, Marius, Mobasher, Bahram, Mohanty, Subhanjoy, Montier, Ludovic, Moodley, Kavilan, Moriarty-Schieven, Gerald H., Mortier, Angela, Munshi, Dipak, Murphy, Eric, Nandra, Kirpal, Natoli, Paolo, Nguyen, Hien, Oliver, Seb, Omont, Alain, Page, Lyman, Page, Mathew, Paladini, Roberta, Pandolfi, Stefania, Pascale, Enzo, Patanchon, Guillaume, Peacock, John, Pearson, Chris, Perez-Fournon, Ismael, Perez-Gonz, Pablo G., Piacentini, Francesco, Pierpaoli, Elena, Pohlen, Michael, Pointecouteau, Etienne, Polenta, Gianluca, Rawlings, Jason, Reese, Erik~D., Rigby, Emma, Rodighiero, Giulia, Romero-Colmenero, Encarni, Roseboom, Isaac, Rowan-Robinson, Michael, Sanchez-Portal, Miguel, Schmidt, Fabian, Schneider, Michael, Schulz, Bernhard, Scott, Douglas, Sedgwick, Chris, Sehgal, Neelima, Seymour, Nick, Sherwin, Blake~D., Short, Jo, Shupe, David, Sievers, Jonathan, Skibba, Ramin, Smidt, Joseph, Smith, Anthony, Smith, Daniel J. B., Smith, Matthew W. L., Spergel, David, Staggs, Suzanne, Stevens, Jason, Switzer, Eric, Takagi, Toshinobu, Takeuchi, Tsutomu, Temi, Pasquale, Trichas, Markos, Trigilio, Corrado, Tugwell, Katherine, Umana, Grazia, Vacca, William, Vaccari, Mattia, Vaisanen, Petri, Valtchanov, Ivan, van der Heyden, Kurt, van der Werf, Paul P., van_Kampen, Eelco, van_Waerbeke, Ludovic, Vegetti, Simona, Veneziani, Marcella, Verde, Licia, Verma, Aprajita, Vielva, Patricio, Viero, Marco P., Vilaro, Baltasar Vila, Wardlow, Julie, Wilson, Grant, Wright, Edward L., Xu, C. Kevin, and Yun, Min S.
Subjects: Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract: A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwave background experiments. The Herschel-SPIRE Legacy Survey (HSLS), will lead to imaging data over 4000 sq. degrees at 250, 350, and 500 micron. Major Goals of HSLS are: (a) produce a catalog of 2.5 to 3 million galaxies down to 26, 27 and 33 mJy (50% completeness; 5 sigma confusion noise) at 250, 350 and 500 micron, respectively, in the southern hemisphere (3000 sq. degrees) and in an equatorial strip (1000 sq. degrees), areas which have extensive multi-wavelength coverage and are easily accessible from ALMA. Two thirds of the of the sources are expected to be at z > 1, one third at z > 2 and about a 1000 at z > 5. (b) Remove point source confusion in secondary anisotropy studies with Planck and ground-based CMB data. (c) Find at least 1200 strongly lensed bright sub-mm sources leading to a 2% test of general relativity. (d) Identify 200 proto-cluster regions at z of 2 and perform an unbiased study of the environmental dependence of star formation. (e) Perform an unbiased survey for star formation and dust at high Galactic latitude and make a census of debris disks and dust around AGB stars and white dwarfs., Comment: White paper supplement to the proposal submitted by the HSLS science team to ESA for Herschel open-time programs
Published: 2010

14. The Local Environment of the FUor-like Objects AR 6A and 6B

Author: Moriarty-Schieven, Gerald H., Aspin, Colin, and Davis, Gary R.
Subjects: Astrophysics
Abstract: We present new 12CO J=3-2 and HCN J=3-2 molecular line maps of the region surrounding the young star AR 6 using the 15 metre James Clerk Maxwell Telescope. AR 6 was previously found to be a double source with both components exhibiting several characteristics of FU Orionis (FUor) eruptive variable stars. Our data indicates that AR 6, like FU Orionis itself, does not possess a CO outflow and likewise, does not show evidence for large amounts of molecular g as in its circumstellar environment. We conclude that from the near-IR to the sub-mm, AR 6 is similar to FU Orionis in several respects. We interpret the lack of significant dust and molecular gas in the circumstellar environment of AR 6, together with the large near-IR thermal excess, as evidence that the sources have exhausted their natal envelopes, that they have at least small hot circumstellar disks, and that they are more evolved than Class I protostars. This, in itself, suggests that, since FUor eruptions have also been observed in stars with large dust mass envelopes (e.g. V346 Nor) and with CO outflows (e.g. L1551 IRS5), FUor events probably occur at many different stages in the early, formative phase of a star's life, and lends support to the idea that FUor outbursts are repetitive like their shorter-lived relatives occurring in EXor eruptive variables. Finally, we show that, being part of the 'Spokes' young stellar cluster, AR 6 is unlike many FUors which typically are located in more sparsely populated regions., Comment: Accepted for publication in The Astronomical Journal (October 2008)
Published: 2008
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15. Multi-Generational Star Formation in L1551

Author: Moriarty-Schieven, Gerald H., Johnstone, Doug, Bally, John, and Jenness, Tim
Subjects: Astrophysics
Abstract: The L1551 molecular cloud contains two small clusters of Class 0 and I protostars, as well as a halo of more evolved Class II and III YSOs, indicating a current and at least one past burst of star formation. We present here new, sensitive maps of 850 and 450 um dust emission covering most of the L1551 cloud, new CO J=2-1 data of the molecular cloud, and a new, deep, optical image of [SII] emission. No new Class 0/I YSOs were detected. Compact sub-millimetre emitters are concentrated in two sub-clusters: IRS5 and L1551NE, and the HL~Tauri group. Both stellar groups show significant extended emission and outflow/jet activity. A jet, terminating at HH 265 and with a very weak associated molecular outflow, may originate from LkHa 358, or from a binary companion to another member of the HL Tauri group. Several Herbig Haro objects associated with IRS5/NE were clearly detected in the sub-mm, as were faint ridges of emission tracing outflow cavity walls. We confirm a large-scale molecular outflow originating from NE parallel to that from IRS5, and suggest that the "hollow shell" morphology is more likely due to two interacting outflows. We confirm the presence of a prestellar core (L1551-MC) of mass 2-3 Mo north-west of IRS5. The next generation cluster may be forming in this core. The L1551 cloud appears cometary in morphology, and appears to be illuminated and eroded from the direction of Orion, perhaps explaining the multiple episodes of star formation in this cloud. The full paper (including figures) can be downloaded at http://www.jach.hawaii.edu/~gms/l1551/l1551-apj641.pdf, or viewed at http://www.jach.hawaii.edu/~gms/l1551/., Comment: Accepted for publication in The Astrophysical Journal, April 2006 (vol. 641). 27 pages, 17 figures
Published: 2005
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16. A Sub-millimeterwave 'Flare' from GG Tau?

Author: Moriarty-Schieven, Gerald H. and Butner, Harold M.
Subjects: Astrophysics
Abstract: We have monitored the millimeter and submillimeter emission from the young stellar object GG Tau, a T Tauri binary system surrounded by a massive circumbinary disk. We find that between 1992 and 1994, the flux has increased significantly at 800, 1100, and 1300 microns, resulting in a steepening of the observed spectral energy distribution at those wavelengths. Such an increase appears consistent with a modest increase in disk luminosity (a factor of two). The increase in the effective disk temperature might arise from a slight change in the disk heating processes. Alternatively, the flux increase may reflect a sudden change in the underlying dust optical properties., Comment: 15 pages, AASTex v.4.0 format, four postscript figures, four tables, to appear in The Astrophysical Journal
Published: 1996
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17. JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334

Author: Tahani, Mehrnoosh, Bastien, Pierre, Furuya, Ray S., Pattle, Kate, Johnstone, Doug, Arzoumanian, Doris, Doi, Yasuo, Hasegawa, Tetsuo, Inutsuka, Shu-Ichiro, Coudé, Simon, Fissel, Laura, Chen, Michael Chun-Yuan, Poidevin, Frédérick, Sadavoy, Sarah, Friesen, Rachel, Koch, Patrick M., Di Francesco, James, Moriarty-Schieven, Gerald H., Chen, Zhiwei, Chung, Eun Jung, Eswaraiah, Chakali, Fanciullo, Lapo, Gledhill, Tim, Le Gouellec, Valentin J. M., Hoang, Thiem, Hwang, Jihye, Kang, Ji-Hyun, Kim, Kyoung Hee, Kirchschlager, Florian, Kwon, Woojin, Lee, Chang Won, Liu, Hong-Li, Onaka, Takashi, Rawlings, Mark G., Soam, Archana, Tamura, Motohide, Tang, Xindi, Tomisaka, Kohji, Whitworth, Anthony P., Kwon, Jungmi, Hoang, Thuong D., Redman, Matt, Berry, David, Ching, Tao-Chung, Wang, Jia-Wei, Lai, Shih-Ping, Qiu, Keping, Ward-Thompson, Derek, Houde, Martin, Byun, Do-Young, Chen, Huei-Ru Vivien, Chen, Wen Ping, Cho, Jungyeon, Choi, Minho, Choi, Yunhee, Chrysostomou, Antonio, Diep, Pham Ngoc, Duan, Hao-Yuan, Fiege, Jason, Franzmann, Erica, Friberg, Per, Fuller, Gary, Graves, Sarah F., Greaves, Jane S., Griffin, Matt J., Gu, Qilao, Han, Ilseung, Hatchell, Jennifer, Hayashi, Saeko S., Hull, Charles L. H., Inoue, Tsuyoshi, Iwasaki, Kazunari, Jeong, Il-Gyo, Kanamori, Yoshihiro, Kang, Miju, Kang, Sung-Ju, Kataoka, Akimasa, Kawabata, Koji S., Kemper, Francisca, Kim, Gwanjeong, Kim, Jongsoo, Kim, Kee-Tae, Kim, Mi-Ryang, Kim, Shinyoung, Kirk, Jason M., Kobayashi, Masato I. N., Konyves, Vera, Kusune, Takayoshi, Lacaille, Kevin, Law, Chi-Yan, Lee, Chin-Fei, Lee, Hyeseung, Lee, Jeong-Eun, Lee, Sang-Sung, Lee, Yong-Hee, Li, Dalei, Li, Di, Li, Hua-Bai, Liu, Junhao, Liu, Sheng-Yuan, Liu, Tie, De Looze, Ilse, Lyo, A-Ran, Mairs, Steve, Matsumura, Masafumi, Matthews, Brenda C., Nagata, Tetsuya, Nakamura, Fumitaka, Nakanishi, Hiroyuki, Ohashi, Nagayoshi, Park, Geumsook, Parsons, Harriet, Peretto, Nicolas, Pyo, Tae-Soo, Qian, Lei, Rao, Ramprasad, Retter, Brendan, Richer, John, Rigby, Andrew, Saito, Hiro, Savini, Giorgio, Scaife, Anna M. M., Seta, Masumichi, Shimajiri, Yoshito, Shinnaga, Hiroko, Tang, Ya-Wen, Tsukamoto, Yusuke, Viti, Serena, Wang, Hongchi, Yen, Hsi-Wei, Yoo, Hyunju, Yuan, Jinghua, Yun, Hyeong-Sik, Zenko, Tetsuya, Zhang, Chuan-Peng, Zhang, Guoyin, Zhang, Yapeng, Zhou, Jianjun, Zhu, Lei, André, Philippe, Dowell, C. Darren, Eyres, Stewart P. S., Falle, Sam, Van Loo, Sven, Robitaille, Jean-François, Tahani, Mehrnoosh [0000-0001-8749-1436], Bastien, Pierre [0000-0002-0794-3859], Furuya, Ray S. [0000-0003-0646-8782], Pattle, Kate [0000-0002-8557-3582], Johnstone, Doug [0000-0002-6773-459X], Arzoumanian, Doris [0000-0002-1959-7201], Doi, Yasuo [0000-0001-8746-6548], Hasegawa, Tetsuo [0000-0003-1853-0184], Inutsuka, Shu-ichiro [0000-0003-4366-6518], Coudé, Simon [0000-0002-0859-0805], Fissel, Laura [0000-0002-0859-0805], Chen, Michael Chun-Yuan [0000-0003-4242-973X], Poidevin, Frédérick [0000-0002-5391-5568], Sadavoy, Sarah [0000-0001-7474-6874], Friesen, Rachel [0000-0001-7594-8128], Koch, Patrick M. [0000-0003-2777-5861], Di Francesco, James [0000-0002-9289-2450], Moriarty-Schieven, Gerald H. [0000-0002-0393-7822], Chen, Zhiwei [0000-0003-0849-0692], Chung, Eun Jung [0000-0003-0014-1527], Eswaraiah, Chakali [0000-0003-4761-6139], Fanciullo, Lapo [0000-0001-9930-9240], Gledhill, Tim [0000-0002-2859-4600], Le Gouellec, Valentin J. M. [0000-0002-5714-799X], Hoang, Thiem [0000-0003-2017-0982], Hwang, Jihye [0000-0001-7866-2686], Kang, Ji-hyun [0000-0001-7379-6263], Kim, Kyoung Hee [0000-0001-9597-7196], Kirchschlager, Florian [0000-0002-3036-0184], Kwon, Woojin [0000-0003-4022-4132], Lee, Chang Won [0000-0002-3179-6334], Liu, Hong-Li [0000-0003-3343-9645], Onaka, Takashi [0000-0002-8234-6747], Rawlings, Mark G. [0000-0002-6529-202X], Soam, Archana [0000-0002-6386-2906], Tamura, Motohide [0000-0002-6510-0681], Tang, Xindi [0000-0002-4154-4309], Tomisaka, Kohji [0000-0003-2726-0892], Kwon, Jungmi [0000-0003-2815-7774], Hoang, Thuong D. [0000-0002-3437-5228], Redman, Matt [0000-0002-1021-9343], Berry, David [0000-0001-6524-2447], Ching, Tao-Chung [0000-0001-8516-2532], Wang, Jia-Wei [0000-0002-6668-974X], Lai, Shih-Ping [0000-0001-5522-486X], Qiu, Keping [0000-0002-5093-5088], Ward-Thompson, Derek [0000-0003-1140-2761], Houde, Martin [0000-0003-4420-8674], Byun, Do-Young [0000-0003-1157-4109], Chen, Huei-Ru Vivien [0000-0002-9774-1846], Chen, Wen Ping [0000-0003-0262-272X], Cho, Jungyeon [0000-0003-1725-4376], Chrysostomou, Antonio [0000-0002-9583-8644], Diep, Pham Ngoc [0000-0002-2808-0888], Duan, Hao-Yuan [0000-0002-7022-4742], Franzmann, Erica [0000-0003-2142-0357], Friberg, Per [0000-0002-8010-8454], Fuller, Gary [0000-0001-8509-1818], Graves, Sarah F. [0000-0001-9361-5781], Greaves, Jane S. [0000-0002-3133-413X], Gu, Qilao [0000-0002-2826-1902], Hatchell, Jennifer [0000-0002-4870-2760], Hayashi, Saeko S. [0000-0001-5026-490X], Hull, Charles L. H. [0000-0002-8975-7573], Inoue, Tsuyoshi [0000-0002-7935-8771], Jeong, Il-Gyo [0000-0002-5492-6832], Kang, Miju [0000-0002-5016-050X], Kang, Sung-ju [0000-0002-5004-7216], Kataoka, Akimasa [0000-0003-4562-4119], Kawabata, Koji S. [0000-0001-6099-9539], Kemper, Francisca [0000-0003-2743-8240], Kim, Gwanjeong [0000-0003-2011-8172], Kim, Jongsoo [0000-0002-1229-0426], Kim, Kee-Tae [0000-0003-2412-7092], Kim, Mi-Ryang [0000-0002-1408-7747], Kim, Shinyoung [0000-0001-9333-5608], Kirk, Jason M. [0000-0002-4552-7477], Kobayashi, Masato I. N. [0000-0003-3990-1204], Konyves, Vera [0000-0002-3746-1498], Lacaille, Kevin [0000-0001-9870-5663], Law, Chi-Yan [0000-0003-1964-970X], Lee, Chin-Fei [0000-0002-3024-5864], Lee, Jeong-Eun [0000-0003-3119-2087], Lee, Sang-Sung [0000-0002-6269-594X], Lee, Yong-Hee [0000-0001-6047-701X], Li, Di [0000-0003-3010-7661], Li, Hua-bai [0000-0003-2641-9240], Liu, Junhao [0000-0002-4774-2998], Liu, Sheng-Yuan [0000-0003-4603-7119], Liu, Tie [0000-0002-5286-2564], Lyo, A-Ran [0000-0002-9907-8427], Mairs, Steve [0000-0002-6956-0730], Matsumura, Masafumi [0000-0002-6906-0103], Matthews, Brenda C. [0000-0003-3017-9577], Nagata, Tetsuya [0000-0001-9264-9015], Nakamura, Fumitaka [0000-0001-5431-2294], Ohashi, Nagayoshi [0000-0003-0998-5064], Park, Geumsook [0000-0001-8467-3736], Parsons, Harriet [0000-0002-6327-3423], Pyo, Tae-Soo [0000-0002-3273-0804], Qian, Lei [0000-0003-0597-0957], Rao, Ramprasad [0000-0002-1407-7944], Richer, John [0000-0002-9693-6860], Rigby, Andrew [0000-0002-3351-2200], Savini, Giorgio [0000-0003-4449-9416], Scaife, Anna M. M. [0000-0002-5364-2301], Shinnaga, Hiroko [0000-0001-9407-6775], Tang, Ya-Wen [0000-0002-0675-276X], Tsukamoto, Yusuke [0000-0001-6738-676X], Viti, Serena [0000-0001-8504-8844], Wang, Hongchi [0000-0003-0746-7968], Yen, Hsi-Wei [0000-0003-1412-893X], Yoo, Hyunju [0000-0002-8578-1728], Yuan, Jinghua [0000-0001-8060-3538], Yun, Hyeong-Sik [0000-0001-6842-1555], Zhang, Chuan-Peng [0000-0002-4428-3183], Zhang, Yapeng [0000-0002-5102-2096], Zhou, Jianjun [0000-0003-0356-818X], André, Philippe [0000-0002-3413-2293], Eyres, Stewart P. S. [0000-0002-6663-7675], Falle, Sam [0000-0002-9829-0426], van Loo, Sven [0000-0003-4746-8500], Robitaille, Jean-François [0000-0001-5079-8573], Apollo - University of Cambridge Repository, Furuya, Ray S [0000-0003-0646-8782], Koch, Patrick M [0000-0003-2777-5861], Moriarty-Schieven, Gerald H [0000-0002-0393-7822], Le Gouellec, Valentin JM [0000-0002-5714-799X], Rawlings, Mark G [0000-0002-6529-202X], Hoang, Thuong D [0000-0002-3437-5228], Graves, Sarah F [0000-0001-9361-5781], Greaves, Jane S [0000-0002-3133-413X], Hayashi, Saeko S [0000-0001-5026-490X], Hull, Charles LH [0000-0002-8975-7573], Kawabata, Koji S [0000-0001-6099-9539], Kirk, Jason M [0000-0002-4552-7477], Kobayashi, Masato IN [0000-0003-3990-1204], Matthews, Brenda C [0000-0003-3017-9577], Scaife, Anna MM [0000-0002-5364-2301], and Eyres, Stewart PS [0000-0002-6663-7675]
Subjects: 5101 Astronomical Sciences, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Interstellar Matter and the Local Universe, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, 51 Physical Sciences
Abstract: We study the HII regions associated with the NGC 6334 molecular cloud observed in the sub-millimeter and taken as part of the B-fields In STar-forming Region Observations (BISTRO) Survey. In particular, we investigate the polarization patterns and magnetic field morphologies associated with these HII regions. Through polarization pattern and pressure calculation analyses, several of these bubbles indicate that the gas and magnetic field lines have been pushed away from the bubble, toward an almost tangential (to the bubble) magnetic field morphology. In the densest part of NGC 6334, where the magnetic field morphology is similar to an hourglass, the polarization observations do not exhibit observable impact from HII regions. We detect two nested radial polarization patterns in a bubble to the south of NGC 6334 that correspond to the previously observed bipolar structure in this bubble. Finally, using the results of this study, we present steps (incorporating computer vision; circular Hough Transform) that can be used in future studies to identify bubbles that have physically impacted magnetic field lines., Comment: Accepted for publication in Astrophysical Journal (ApJ)
Published: 2023

18. Quantifying Variability of Young Stellar Objects in the Mid-infrared Over 6 Years with the Near-Earth Object Wide-field Infrared Survey Explorer

Author: Park, Wooseok, primary, Lee, Jeong-Eun, additional, Contreras Peña, Carlos, additional, Johnstone, Doug, additional, Herczeg, Gregory, additional, Lee, Sieun, additional, Lee, Seonjae, additional, Bhardwaj, Anupam, additional, and Moriarty-Schieven, Gerald H., additional
Published: 2021
Full Text: View/download PDF

19. The JCMT Transient Survey: Four-year Summary of Monitoring the Submillimeter Variability of Protostars

Author: Lee, Yong-Hee, primary, Johnstone, Doug, additional, Lee, Jeong-Eun, additional, Herczeg, Gregory, additional, Mairs, Steve, additional, Contreras-Peña, Carlos, additional, Hatchell, Jennifer, additional, Naylor, Tim, additional, Bell, Graham S., additional, Bourke, Tyler L., additional, Broughton, Colton, additional, Francis, Logan, additional, Gupta, Aashish, additional, Harsono, Daniel, additional, Liu, Sheng-Yuan, additional, Park, Geumsook, additional, Plovie, Spencer, additional, Moriarty-Schieven, Gerald H., additional, Scholz, Aleks, additional, Sharma, Tanvi, additional, Stella Teixeira, Paula, additional, Wang, Yao-Te, additional, Aikawa, Yuri, additional, Bower, Geoffrey C., additional, Vivien Chen, Huei-Ru, additional, Bae, Jaehan, additional, Baek, Giseon, additional, Chapman, Scott, additional, Ping Chen, Wen, additional, Du, Fujun, additional, Dutta, Somnath, additional, Forbrich, Jan, additional, Guo, Zhen, additional, Inutsuka, Shu-ichiro, additional, Kang, Miju, additional, Kirk, Helen, additional, Kuan, Yi-Jehng, additional, Kwon, Woojin, additional, Lai, Shih-Ping, additional, Lalchand, Bhavana, additional, Lane, James M. M., additional, Lee, Chin-Fei, additional, Liu, Tie, additional, Morata, Oscar, additional, Pearson, Samuel, additional, Pon, Andy, additional, Sahu, Dipen, additional, Shang, Hsien, additional, Stamatellos, Dimitris, additional, Tang, Shih-Yun, additional, Xu, Ziyan, additional, Yoo, Hyunju, additional, and Rawlings, Jonathan M. C., additional
Published: 2021
Full Text: View/download PDF

20. Erratum: “The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333” (2020, ApJ, 899, 28)

Author: Doi, Yasuo, primary, Hasegawa, Tetsuo, additional, Furuya, Ray S., additional, Coudé, Simon, additional, Hull, Charles L. H., additional, Arzoumanian, Doris, additional, Bastien, Pierre, additional, Chen, Michael Chun-Yuan, additional, Di Francesco, James, additional, Friesen, Rachel, additional, Houde, Martin, additional, Inutsuka, Shu-ichiro, additional, Mairs, Steve, additional, Matsumura, Masafumi, additional, Onaka, Takashi, additional, Sadavoy, Sarah, additional, Shimajiri, Yoshito, additional, Tahani, Mehrnoosh, additional, Tomisaka, Kohji, additional, Eswaraiah, Chakali, additional, Koch, Patrick M., additional, Pattle, Kate, additional, Lee, Chang Won, additional, Tamura, Motohide, additional, Berry, David, additional, Ching, Tao-Chung, additional, Hwang, Jihye, additional, Kwon, Woojin, additional, Soam, Archana, additional, Wang, Jia-Wei, additional, Lai, Shih-Ping, additional, Qiu, Keping, additional, Ward-Thompson, Derek, additional, Byun, Do-Young, additional, Chen, Huei-Ru Vivien, additional, Chen, Wen Ping, additional, Chen, Zhiwei, additional, Cho, Jungyeon, additional, Choi, Minho, additional, Choi, Yunhee, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Diep, Pham Ngoc, additional, Duan, Hao-Yuan, additional, Fanciullo, Lapo, additional, Fiege, Jason, additional, Franzmann, Erica, additional, Friberg, Per, additional, Fuller, Gary, additional, Gledhill, Tim, additional, Graves, Sarah F., additional, Greaves, Jane S., additional, Griffin, Matt J., additional, Gu, Qilao, additional, Han, Ilseung, additional, Hatchell, Jennifer, additional, Hayashi, Saeko S., additional, Hoang, Thiem, additional, Inoue, Tsuyoshi, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Johnstone, Doug, additional, Kanamori, Yoshihiro, additional, Kang, Ji-hyun, additional, Kang, Miju, additional, Kang, Sung-ju, additional, Kataoka, Akimasa, additional, Kawabata, Koji S., additional, Kemper, Francisca, additional, Kim, Gwanjeong, additional, Kim, Jongsoo, additional, Kim, Kee-Tae, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Kirk, Jason M., additional, Kobayashi, Masato I. N., additional, Konyves, Vera, additional, Kusune, Takayoshi, additional, Kwon, Jungmi, additional, Lacaille, Kevin, additional, Law, Chi-Yan, additional, Lee, Chin-Fei, additional, Lee, Hyeseung, additional, Lee, Jeong-Eun, additional, Lee, Sang-Sung, additional, Lee, Yong-Hee, additional, Li, Dalei, additional, Li, Di, additional, Li, Hua-bai, additional, Liu, Hong-Li, additional, Liu, Junhao, additional, Liu, Sheng-Yuan, additional, Liu, Tie, additional, Looze, Ilse de, additional, Lyo, A-Ran, additional, Matthews, Brenda C., additional, Moriarty-Schieven, Gerald H., additional, Nagata, Tetsuya, additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Park, Geumsook, additional, Parsons, Harriet, additional, Peretto, Nicolas, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Rao, Ramprasad, additional, Rawlings, Mark G., additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Saito, Hiro, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Seta, Masumichi, additional, Shinnaga, Hiroko, additional, Tang, Ya-Wen, additional, Tsukamoto, Yusuke, additional, Viti, Serena, additional, Wang, Hongchi, additional, Whitworth, Anthony P., additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, Yuan, Jinghua, additional, Yun, Hyeong-Sik, additional, Zenko, Tetsuya, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhang, Yapeng, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, André, Philippe, additional, Dowell, C. Darren, additional, Eyres, Stewart P. S., additional, Falle, Sam, additional, van Loo, Sven, additional, and Robitaille, Jean-François, additional
Published: 2021
Full Text: View/download PDF

21. The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Author: Cooray, Asantha, Eales, Steve, Chapman, Scott, Clements, David L., Dore, Olivier, Farrah, Duncan, Jarvis, Matt J., Kaplinghat, Manoj, Negrello, Mattia, Melchiorri, Alessandro, Peiris, Hiranya, Pope, Alexandra, Santos, Mario G., Serjeant, Stephen, Thompson, Mark, White, Glenn, Amblard, Alexandre, Banerji, Manda, Corasaniti, Pier-Stefano, Das, Sudeep, Bernardis, Francesco, Zotti, Gianfranco, Giannantonio, Tommaso, Gonzalez-Nuevo Gonzalez, Joaquin, Khostovan, Ali Ahmad, Mitchell-Wynne, Ketron, Serra, Paolo, Song, Yong-Seon, Vieira, Joaquin, Wang, Lingyu, Zemcov, Michael, Abdalla, Filipe, Afonso, Jose, Aghanim, Nabila, Andreani, Paola, Aretxaga, Itziar, Auld, Robbie, Baes, Maarten, Baker, Andrew, Barkats, Denis, Belen Barreiro, R., Bartolo, Nicola, Barton, Elizabeth, Barway, Sudhanshu, Stefano Battistelli, Elia, Baugh, Carlton, Beelen, Alexander, Benabed, Karim, Blain, Andrew, Bland-Hawthorn, Joss, Bock, James J., Bond, J. Richard, Borrill, Julian, Borys, Colin, Boselli, Alessandro, Bouchet, Francois R., Bridge, Carrie, Brighenti, Fabrizio, Buat, Veronique, Buote, David, Burgarella, Denis, Bussmann, Robert, Calabrese, Erminia, Cantalupo, Christopher, Carlberg, Raymond, Sofia Carvalho, Carla, Caitlin Casey, Cava, Antonio, Cepa, Jordi, Chapin, Edward, Ram Chary, Ranga, Chen, Xuelei, Colafrancesco, Sergio, Cole, Shaun, Coles, Peter, Conley, Alexander, Conversi, Luca, Cooke, Jeff, Crawford, Steven, Cress, Catherine, Da Cunha, Elisabete, Dalton, Gavin, Danese, Luigi, Dannerbauer, Helmut, Davies, Jonathan, Bernardis, Paolo, Putter, Roland, Devlin, Mark, Diego, Jose M., Dole, Herve, Douspis, Marian, Dunkley, Joanna, Dunlop, James, Dunne, Loretta, Dunner, Rolando, Dye, Simon, Efstathiou, George, Egami, Eiichi, Fang, Taotao, Ferrero, Patrizia, Franceschini, Alberto, Frazer, Christopher C., Frayer, David, Frenk, Carlos, Ganga, Ken, Gavazzi, Raphael, Glenn, Jason, Gong, Yan, Gonzalez-Solares, Eduardo, Griffin, Matt, Guo, Qi, Gurwell, Mark, Hajian, Amir, Halpern, Mark, Hanson, Duncan, Hardcastle, Martin, Hatziminaoglou, Evanthia, Heavens, Alan, Heinis, Sebastien, Herranz, Diego, Hilton, Matt, Ho, Shirley, Holwerda, Benne W., Hopwood, Rosalind, Horner, Jonathan, Huffenberger, Kevin, Hughes, David H., Hughes, John P., Ibar, Edo, Ivison, Rob, Jackson, Neal, Jaffe, Andrew, Jenness, Timothy, Joncas, Gilles, Joudaki, Shahab, Kaviraj, Sugata, Kim, Sam, King, Lindsay, Kisner, Theodore, Knapen, Johan, Kniazev, Alexei, Komatsu, Eiichiro, Koopmans, Leon, Kuo, Chao-Lin, Lacey, Cedric, Lahav, Ofer, Lasenby, Anthony N., Lawrence, Andy, Lee, Myung Gyoon, Leeuw, Lerothodi L., Levenson, Louis R., Lewis, Geraint, Loaring, Nicola, Lopez-Caniego, Marcos, Maddox, Steve, Marriage, Tobias, Marsden, Gaelen, Martinez-Gonzalez, Enrique, Masi, Silvia, Matarrese, Sabino, Mathews, William G., Matsuura, Shuji, Mcmahon, Richard, Mellier, Yannick, Menanteau, Felipe, Michalowski, Michal J., Millea, Marius, Mobasher, Bahram, Mohanty, Subhanjoy, Montier, Ludovic, Moodley, Kavilan, Moriarty-Schieven, Gerald H., Mortier, Angela, Munshi, Dipak, Murphy, Eric, Nandra, Kirpal, Natoli, Paolo, Nguyen, Hien, Oliver, Seb, Omont, Alain, Page, Lyman, Page, Mathew, Paladini, Roberta, Pandolfi, Stefania, Pascale, Enzo, Patanchon, Guillaume, Peacock, John, Pearson, Chris, Perez-Fournon, Ismael, Perez-Gonz, Pablo G., Piacentini, Francesco, Pierpaoli, Elena, Pohlen, Michael, Pointecouteau, Etienne, Polenta, Gianluca, Rawlings, Jason, Reese, Erik D., Rigby, Emma, Rodighiero, Giulia, Romero-Colmenero, Encarni, Roseboom, Isaac, Rowan-Robinson, Michael, Sanchez-Portal, Miguel, Schmidt, Fabian, Schneider, Michael, Schulz, Bernhard, Scott, Douglas, Sedgwick, Chris, Sehgal, Neelima, Seymour, Nick, Sherwin, Blake D., Short, Jo, Shupe, David, Sievers, Jonathan, Skibba, Ramin, Smidt, Joseph, Smith, Anthony, Smith, Daniel J. B., Smith, Matthew W. L., Spergel, David, Staggs, Suzanne, Stevens, Jason, Switzer, Eric, Takagi, Toshinobu, Takeuchi, Tsutomu, Temi, Pasquale, Trichas, Markos, Trigilio, Corrado, Tugwell, Katherine, Umana, Grazia, Vacca, William, Vaccari, Mattia, Vaisanen, Petri, Valtchanov, Ivan, Heyden, Kurt, Werf, Paul P., Kampen, Eelco, Waerbeke, Ludovic, Vegetti, Simona, Veneziani, Marcella, Verde, Licia, Verma, Aprajita, Vielva, Patricio, Viero, Marco P., Vila Vilaro, Baltasar, Wardlow, Julie, Wilson, Grant, Wright, Edward L., Xu, C. Kevin, Yun, Min S., Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS]Physics [physics], Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwave background experiments. The Herschel-SPIRE Legacy Survey (HSLS), will lead to imaging data over 4000 sq. degrees at 250, 350, and 500 micron. Major Goals of HSLS are: (a) produce a catalog of 2.5 to 3 million galaxies down to 26, 27 and 33 mJy (50% completeness; 5 sigma confusion noise) at 250, 350 and 500 micron, respectively, in the southern hemisphere (3000 sq. degrees) and in an equatorial strip (1000 sq. degrees), areas which have extensive multi-wavelength coverage and are easily accessible from ALMA. Two thirds of the of the sources are expected to be at z > 1, one third at z > 2 and about a 1000 at z > 5. (b) Remove point source confusion in secondary anisotropy studies with Planck and ground-based CMB data. (c) Find at least 1200 strongly lensed bright sub-mm sources leading to a 2% test of general relativity. (d) Identify 200 proto-cluster regions at z of 2 and perform an unbiased study of the environmental dependence of star formation. (e) Perform an unbiased survey for star formation and dust at high Galactic latitude and make a census of debris disks and dust around AGB stars and white dwarfs., White paper supplement to the proposal submitted by the HSLS science team to ESA for Herschel open-time programs
Published: 2020

22. The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333

Author: Doi, Yasuo, primary, Hasegawa, Tetsuo, additional, Furuya, Ray S., additional, Coudé, Simon, additional, Hull, Charles L. H., additional, Arzoumanian, Doris, additional, Bastien, Pierre, additional, Chen, Michael Chun-Yuan, additional, Di Francesco, James, additional, Friesen, Rachel, additional, Houde, Martin, additional, Inutsuka, Shu-ichiro, additional, Mairs, Steve, additional, Matsumura, Masafumi, additional, Onaka, Takashi, additional, Sadavoy, Sarah, additional, Shimajiri, Yoshito, additional, Tahani, Mehrnoosh, additional, Tomisaka, Kohji, additional, Eswaraiah, Chakali, additional, Koch, Patrick M., additional, Pattle, Kate, additional, Won Lee, Chang, additional, Tamura, Motohide, additional, Berry, David, additional, Ching, Tao-Chung, additional, Hwang, Jihye, additional, Kwon, Woojin, additional, Soam, Archana, additional, Wang, Jia-Wei, additional, Lai, Shih-Ping, additional, Qiu, Keping, additional, Ward-Thompson, Derek, additional, Byun, Do-Young, additional, Chen, Huei-Ru Vivien, additional, Chen, Wen Ping, additional, Chen, Zhiwei, additional, Cho, Jungyeon, additional, Choi, Minho, additional, Choi, Yunhee, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Diep, Pham Ngoc, additional, Duan, Hao-Yuan, additional, Fanciullo, Lapo, additional, Fiege, Jason, additional, Franzmann, Erica, additional, Friberg, Per, additional, Fuller, Gary, additional, Gledhill, Tim, additional, Graves, Sarah F., additional, Greaves, Jane S., additional, Griffin, Matt J., additional, Gu, Qilao, additional, Han, Ilseung, additional, Hatchell, Jennifer, additional, Hayashi, Saeko S., additional, Hoang, Thiem, additional, Inoue, Tsuyoshi, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Johnstone, Doug, additional, Kanamori, Yoshihiro, additional, Kang, Ji-hyun, additional, Kang, Miju, additional, Kang, Sung-ju, additional, Kataoka, Akimasa, additional, Kawabata, Koji S., additional, Kemper, Francisca, additional, Kim, Gwanjeong, additional, Kim, Jongsoo, additional, Kim, Kee-Tae, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Kirk, Jason M., additional, Kobayashi, Masato I. N., additional, Konyves, Vera, additional, Kusune, Takayoshi, additional, Kwon, Jungmi, additional, Lacaille, Kevin, additional, Law, Chi-Yan, additional, Lee, Chin-Fei, additional, Lee, Hyeseung, additional, Lee, Jeong-Eun, additional, Lee, Sang-Sung, additional, Lee, Yong-Hee, additional, Li, Dalei, additional, Li, Di, additional, Li, Hua-bai, additional, Liu, Hong-Li, additional, Liu, Junhao, additional, Liu, Sheng-Yuan, additional, Liu, Tie, additional, de Looze, Ilse, additional, Lyo, A-Ran, additional, Matthews, Brenda C., additional, Moriarty-Schieven, Gerald H., additional, Nagata, Tetsuya, additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Park, Geumsook, additional, Parsons, Harriet, additional, Peretto, Nicolas, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Rao, Ramprasad, additional, Rawlings, Mark G., additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Saito, Hiro, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Seta, Masumichi, additional, Shinnaga, Hiroko, additional, Tang, Ya-Wen, additional, Tsukamoto, Yusuke, additional, Viti, Serena, additional, Wang, Hongchi, additional, Whitworth, Anthony P., additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, Yuan, Jinghua, additional, Yun, Hyeong-Sik, additional, Zenko, Tetsuya, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhang, Yapeng, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, André, Philippe, additional, Dowell, C. Darren, additional, Eyres, Stewart P. S., additional, Falle, Sam, additional, van Loo, Sven, additional, and Robitaille, Jean-François, additional
Published: 2020
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23. The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C

Author: Liu, Junhao, primary, Qiu, Keping, additional, Berry, David, additional, Di Francesco, James, additional, Bastien, Pierre, additional, Koch, Patrick M., additional, Furuya, Ray S., additional, Kim, Kee-Tae, additional, Coudé, Simon, additional, Lee, Chang Won, additional, Soam, Archana, additional, Eswaraiah, Chakali, additional, Li, Di, additional, Hwang, Jihye, additional, Lyo, A-Ran, additional, Pattle, Kate, additional, Hasegawa, Tetsuo, additional, Kwon, Woojin, additional, Lai, Shih-Ping, additional, Ward-Thompson, Derek, additional, Ching, Tao-Chung, additional, Chen, Zhiwei, additional, Gu, Qilao, additional, Li, Dalei, additional, Li, Hua-bai, additional, Liu, Hong-Li, additional, Qian, Lei, additional, Wang, Hongchi, additional, Yuan, Jinghua, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhang, Ya-Peng, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, André, Philippe, additional, Arzoumanian, Doris, additional, Aso, Yusuke, additional, Byun, Do-Young, additional, Chen, Michael Chun-Yuan, additional, Chen, Huei-Ru Vivien, additional, Chen, Wen Ping, additional, Cho, Jungyeon, additional, Choi, Minho, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Doi, Yasuo, additional, Drabek-Maunder, Emily, additional, Dowell, C. Darren, additional, Eyres, Stewart P. S., additional, Falle, Sam, additional, Fanciullo, Lapo, additional, Fiege, Jason, additional, Franzmann, Erica, additional, Friberg, Per, additional, Friesen, Rachel K., additional, Fuller, Gary, additional, Gledhill, Tim, additional, Graves, Sarah F., additional, Greaves, Jane S., additional, Griffin, Matt J., additional, Han, Ilseung, additional, Hatchell, Jennifer, additional, Hayashi, Saeko S., additional, Hoang, Thiem, additional, Holland, Wayne, additional, Houde, Martin, additional, Inoue, Tsuyoshi, additional, Inutsuka, Shu-ichiro, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Johnstone, Doug, additional, Kanamori, Yoshihiro, additional, Kang, Ji-hyun, additional, Kang, Miju, additional, Kang, Sung-ju, additional, Kataoka, Akimasa, additional, Kawabata, Koji S., additional, Kemper, Francisca, additional, Kim, Gwanjeong, additional, Kim, Jongsoo, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Kirk, Jason M., additional, Kobayashi, Masato I. N., additional, Kusune, Takayoshi, additional, Kwon, Jungmi, additional, Lacaille, Kevin M., additional, Lee, Chin-Fei, additional, Lee, Jeong-Eun, additional, Lee, Hyeseung, additional, Lee, Sang-Sung, additional, Liu, Sheng-Yuan, additional, Liu, Tie, additional, van Loo, Sven, additional, Mairs, Steve, additional, Matsumura, Masafumi, additional, Matthews, Brenda C., additional, Moriarty-Schieven, Gerald H., additional, Nagata, Tetsuya, additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Onaka, Takashi, additional, Parker, Josh, additional, Parsons, Harriet, additional, Pascale, Enzo, additional, Peretto, Nicolas, additional, Pon, Andy, additional, Pyo, Tae-Soo, additional, Rao, Ramprasad, additional, Rawlings, Mark G., additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Robitaille, Jean-François, additional, Sadavoy, Sarah, additional, Saito, Hiro, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Seta, Masumichi, additional, Shinnaga, Hiroko, additional, Tamura, Motohide, additional, Tang, Ya-Wen, additional, Tomisaka, Kohji, additional, Tsukamoto, Yusuke, additional, Wang, Jia-Wei, additional, Whitworth, Anthony P., additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, and Zenko, Tetsuya, additional
Published: 2019
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24. JCMT BISTRO Survey: Magnetic Fields within the Hub-filament Structure in IC 5146

Author: Wang, Jia-Wei, primary, Lai, Shih-Ping, additional, Eswaraiah, Chakali, additional, Pattle, Kate, additional, Francesco, James Di, additional, Johnstone, Doug, additional, Koch, Patrick M., additional, Liu, Tie, additional, Tamura, Motohide, additional, Furuya, Ray S., additional, Onaka, Takashi, additional, Ward-Thompson, Derek, additional, Soam, Archana, additional, Kim, Kee-Tae, additional, Lee, Chang Won, additional, Lee, Chin-Fei, additional, Mairs, Steve, additional, Arzoumanian, Doris, additional, Kim, Gwanjeong, additional, Hoang, Thiem, additional, Hwang, Jihye, additional, Liu, Sheng-Yuan, additional, Berry, David, additional, Bastien, Pierre, additional, Hasegawa, Tetsuo, additional, Kwon, Woojin, additional, Qiu, Keping, additional, André, Philippe, additional, Aso, Yusuke, additional, Byun, Do-Young, additional, Chen, Huei-Ru, additional, Chen, Michael C., additional, Chen, Wen Ping, additional, Ching, Tao-Chung, additional, Cho, Jungyeon, additional, Choi, Minho, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Coudé, Simon, additional, Doi, Yasuo, additional, Dowell, C. Darren, additional, Drabek-Maunder, Emily, additional, Duan, Hao-Yuan, additional, Eyres, Stewart P. S., additional, Falle, Sam, additional, Fanciullo, Lapo, additional, Fiege, Jason, additional, Franzmann, Erica, additional, Friberg, Per, additional, Friesen, Rachel K., additional, Fuller, Gary, additional, Gledhill, Tim, additional, Graves, Sarah F., additional, Greaves, Jane S., additional, Griffin, Matt J., additional, Gu, Qilao, additional, Han, Ilseung, additional, Hatchell, Jennifer, additional, Hayashi, Saeko S., additional, Holland, Wayne, additional, Houde, Martin, additional, Inoue, Tsuyoshi, additional, Inutsuka, Shu-ichiro, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Kanamori, Yoshihiro, additional, Kang, Ji-hyun, additional, Kang, Miju, additional, Kang, Sung-ju, additional, Kataoka, Akimasa, additional, Kawabata, Koji S., additional, Kemper, Francisca, additional, Kim, Jongsoo, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Kirk, Jason M., additional, Kobayashi, Masato I. N., additional, Konyves, Vera, additional, Kwon, Jungmi, additional, Lacaille, Kevin M., additional, Lee, Hyeseung, additional, Lee, Jeong-Eun, additional, Lee, Sang-Sung, additional, Lee, Yong-Hee, additional, Li, Dalei, additional, Li, Di, additional, Li, Hua-bai, additional, Liu, Hong-Li, additional, Liu, Junhao, additional, Lyo, A-Ran, additional, Matsumura, Masafumi, additional, Matthews, Brenda C., additional, Moriarty-Schieven, Gerald H., additional, Nagata, Tetsuya, additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Park, Geumsook, additional, Parsons, Harriet, additional, Pascale, Enzo, additional, Peretto, Nicolas, additional, Pon, Andy, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Rao, Ramprasad, additional, Rawlings, Mark G., additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Robitaille, Jean-François, additional, Sadavoy, Sarah, additional, Saito, Hiro, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Seta, Masumichi, additional, Shinnaga, Hiroko, additional, Tang, Ya-Wen, additional, Tomisaka, Kohji, additional, Tsukamoto, Yusuke, additional, Loo, Sven van, additional, Wang, Hongchi, additional, Whitworth, Anthony P., additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, Yuan, Jinghua, additional, Yun, Hyeong-Sik, additional, Zenko, Tetsuya, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhang, Ya-Peng, additional, Zhou, Jianjun, additional, and Zhu, Lei, additional
Published: 2019
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25. The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17

Author: Liu, Tie, Kim, Kee-Tae, Juvela, Mika, Wang, Ke, Tatematsu, Ken’ichi, Francesco, James Di, Liu, Sheng-Yuan, Wu, Yuefang, Thompson, Mark, Fuller, Gary, Eden, David, Li, Di, Ristorcelli, I., Kang, Sung-ju, Lin, Yuxin, Johnstone, D., He, J. H., Koch, P. M., Sanhueza, Patricio, Qin, Sheng-Li, Zhang, Q., Hirano, N., Goldsmith, Paul F., Evans II, Neal J., White, Glenn J., Choi, Minho, Lee, Chang Won, Toth, L. V., Mairs, Steve, Yi, H.-W., Tang, Mengyao, Soam, Archana, Peretto, N., Samal, Manash R., Fich, Michel, Parsons, Harriet, Yuan, Jinghua, Zhang, Chuan-Peng, Malinen, Johanna, Bendo, George J., Rivera-Ingraham, A., Liu, Hong-Li, Wouterloot, Jan, Li, Pak Shing, Qian, Lei, Rawlings, Jonathan, Rawlings, Mark G., Feng, Siyi, Aikawa, Yuri, Akhter, S., Alina, Dana, Bell, Graham, Bernard, J.-P., Blain, Andrew, Bőgner, Rebeka, Bronfman, L., Byun, D.-Y., Chapman, Scott, Chen, Huei-Ru, Chen, M., Chen, Wen-Ping, Chen, X., Chen, Xuepeng, Chrysostomou, A., Cosentino, Giuliana, Cunningham, M. R., Demyk, K., Drabek-Maunder, Emily, Doi, Yasuo, Eswaraiah, C., Falgarone, Edith, Fehér, O., Fraser, Helen, Friberg, Per, Garay, G., Ge, J. X., Gear, W. K., Greaves, Jane, Guan, X., Harvey-Smith, Lisa, HASEGAWA, Tetsuo, Hatchell, J., He, Yuxin, Henkel, C., Hirota, T., Holland, W., Hughes, A., Jarken, E., Ji, Tae-Geun, Jimenez-Serra, Izaskun, Kang, Miju, Kawabata, Koji S., Kim, Gwanjeong, Kim, Jungha, Kim, Jongsoo, Kim, Shinyoung, Koo, B.-C., Kwon, Woojin, Kuan, Yi-Jehng, Lacaille, K. M., Lai, Shih-Ping, Lee, C. F., Lee, J.-E., Lee, Y.-U., Li, Dalei, Li, Hua-bai, Lo, N., Lopez, John A. P., Lu, Xing, Lyo, A-Ran, Mardones, D., Marston, A., McGehee, P., Meng, F., Montier, L., Montillaud, Julien, Moore, T., Morata, O., Moriarty-Schieven, Gerald H., Ohashi, S., Pak, Soojong, Park, Geumsook, Paladini, R., Pattle, Kate M, Pech, Gerardo, Pelkonen, V.-M., Qiu, K., Ren, Zhi-Yuan, Richer, John, Saito, M., Sakai, Takeshi, Shang, H., Shinnaga, Hiroko, Stamatellos, Dimitris, Tang, Y.-W., Traficante, Alessio, Vastel, Charlotte, Viti, S., Walsh, Andrew, Wang, Bingru, Wang, Hongchi, Wang, Junzhi, Ward-Thompson, Derek, Whitworth, Anthony, Xu, Ye, Yang, J., Yang, Yao-Lun, Yuan, Lixia, Zavagno, A., Zhang, Guoyin, Zhang, H.-W., Zhou, Chenlin, Zhou, Jianjun, Zhu, Lei, Zuo, Pei, Zhang, Chao, Liu, Tie, Kim, Kee-Tae, Juvela, Mika, Wang, Ke, Tatematsu, Ken’ichi, Francesco, James Di, Liu, Sheng-Yuan, Wu, Yuefang, Thompson, Mark, Fuller, Gary, Eden, David, Li, Di, Ristorcelli, I., Kang, Sung-ju, Lin, Yuxin, Johnstone, D., He, J. H., Koch, P. M., Sanhueza, Patricio, Qin, Sheng-Li, Zhang, Q., Hirano, N., Goldsmith, Paul F., Evans II, Neal J., White, Glenn J., Choi, Minho, Lee, Chang Won, Toth, L. V., Mairs, Steve, Yi, H.-W., Tang, Mengyao, Soam, Archana, Peretto, N., Samal, Manash R., Fich, Michel, Parsons, Harriet, Yuan, Jinghua, Zhang, Chuan-Peng, Malinen, Johanna, Bendo, George J., Rivera-Ingraham, A., Liu, Hong-Li, Wouterloot, Jan, Li, Pak Shing, Qian, Lei, Rawlings, Jonathan, Rawlings, Mark G., Feng, Siyi, Aikawa, Yuri, Akhter, S., Alina, Dana, Bell, Graham, Bernard, J.-P., Blain, Andrew, Bőgner, Rebeka, Bronfman, L., Byun, D.-Y., Chapman, Scott, Chen, Huei-Ru, Chen, M., Chen, Wen-Ping, Chen, X., Chen, Xuepeng, Chrysostomou, A., Cosentino, Giuliana, Cunningham, M. R., Demyk, K., Drabek-Maunder, Emily, Doi, Yasuo, Eswaraiah, C., Falgarone, Edith, Fehér, O., Fraser, Helen, Friberg, Per, Garay, G., Ge, J. X., Gear, W. K., Greaves, Jane, Guan, X., Harvey-Smith, Lisa, HASEGAWA, Tetsuo, Hatchell, J., He, Yuxin, Henkel, C., Hirota, T., Holland, W., Hughes, A., Jarken, E., Ji, Tae-Geun, Jimenez-Serra, Izaskun, Kang, Miju, Kawabata, Koji S., Kim, Gwanjeong, Kim, Jungha, Kim, Jongsoo, Kim, Shinyoung, Koo, B.-C., Kwon, Woojin, Kuan, Yi-Jehng, Lacaille, K. M., Lai, Shih-Ping, Lee, C. F., Lee, J.-E., Lee, Y.-U., Li, Dalei, Li, Hua-bai, Lo, N., Lopez, John A. P., Lu, Xing, Lyo, A-Ran, Mardones, D., Marston, A., McGehee, P., Meng, F., Montier, L., Montillaud, Julien, Moore, T., Morata, O., Moriarty-Schieven, Gerald H., Ohashi, S., Pak, Soojong, Park, Geumsook, Paladini, R., Pattle, Kate M, Pech, Gerardo, Pelkonen, V.-M., Qiu, K., Ren, Zhi-Yuan, Richer, John, Saito, M., Sakai, Takeshi, Shang, H., Shinnaga, Hiroko, Stamatellos, Dimitris, Tang, Y.-W., Traficante, Alessio, Vastel, Charlotte, Viti, S., Walsh, Andrew, Wang, Bingru, Wang, Hongchi, Wang, Junzhi, Ward-Thompson, Derek, Whitworth, Anthony, Xu, Ye, Yang, J., Yang, Yao-Lun, Yuan, Lixia, Zavagno, A., Zhang, Guoyin, Zhang, H.-W., Zhou, Chenlin, Zhou, Jianjun, Zhu, Lei, Zuo, Pei, and Zhang, Chao
Abstract: The low dust temperatures (<14 K) of Planck Galactic cold clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. “TOP-SCOPE” is a joint survey program targeting ∼2000 PGCCs in J=1–0 transitions of CO isotopologues and ∼1000 PGCCs in 850 μm continuum emission. The objective of the “TOP-SCOPE” survey and the joint surveys (SMT 10 m, KVN 21 m, and NRO 45 m) is to statistically study the initial conditions occurring during star formation and the evolution of molecular clouds, across a wide range of environments. The observations, data analysis, and example science cases for these surveys are introduced with an exemplar source, PGCC G26.53+0.17 (G26), which is a filamentary infrared dark cloud (IRDC). The total mass, length, and mean line mass (M/L) of the G26 filament are ∼6200 M☉, ∼12 pc, and ∼500 M☉pc−1, respectively. Ten massive clumps, including eight starless ones, are found along the filament. The most massive clump as a whole may still be in global collapse, while its denser part seems to be undergoing expansion owing to outflow feedback. The fragmentation in the G26 filament from cloud scale to clump scale is in agreement with gravitational fragmentation of an isothermal, nonmagnetized, and turbulent supported cylinder. A bimodal behavior in dust emissivity spectral index (β) distribution is found in G26, suggesting grain growth along the filament. The G26 filament may be formed owing to large-scale compression flows evidenced by the temperature and velocity gradients across its natal cloud. Key words: ISM: abundances – ISM: clouds – ISM: kinematics and dynamics – stars: formation – surveys
Published: 2018

26. Magnetic Fields toward Ophiuchus-B Derived from SCUBA-2 Polarization Measurements

Author: Soam, Archana, primary, Pattle, Kate, additional, Ward-Thompson, Derek, additional, Lee, Chang Won, additional, Sadavoy, Sarah, additional, Koch, Patrick M., additional, Kim, Gwanjeong, additional, Kwon, Jungmi, additional, Kwon, Woojin, additional, Arzoumanian, Doris, additional, Berry, David, additional, Hoang, Thiem, additional, Tamura, Motohide, additional, Lee, Sang-Sung, additional, Liu, Tie, additional, Kim, Kee-Tae, additional, Johnstone, Doug, additional, Nakamura, Fumitaka, additional, Lyo, A-Ran, additional, Onaka, Takashi, additional, Kim, Jongsoo, additional, Furuya, Ray S., additional, Hasegawa, Tetsuo, additional, Lai, Shih-Ping, additional, Bastien, Pierre, additional, Chung, Eun Jung, additional, Kim, Shinyoung, additional, Parsons, Harriet, additional, Rawlings, Mark G., additional, Mairs, Steve, additional, Graves, Sarah F., additional, Robitaille, Jean-Franois, additional, Liu, Hong-Li, additional, Whitworth, Anthony P., additional, Eswaraiah, Chakali, additional, Rao, Ramprasad, additional, Yoo, Hyunju, additional, Houde, Martin, additional, Kang, Ji-hyun, additional, Doi, Yasuo, additional, Choi, Minho, additional, Kang, Miju, additional, Coudé, Simon, additional, Li, Hua-bai, additional, Matsumura, Masafumi, additional, Matthews, Brenda C., additional, Pon, Andy, additional, Francesco, James Di, additional, Hayashi, Saeko S., additional, Kawabata, Koji S., additional, Inutsuka, Shu-ichiro, additional, Qiu, Keping, additional, Franzmann, Erica, additional, Friberg, Per, additional, Greaves, Jane S., additional, Kirk, Jason M., additional, Li, Di, additional, Shinnaga, Hiroko, additional, Loo, Sven van, additional, Aso, Yusuke, additional, Byun, Do-Young, additional, Chen, Huei-Ru, additional, Chen, Mike C.-Y., additional, Chen, Wen Ping, additional, Ching, Tao-Chung, additional, Cho, Jungyeon, additional, Chrysostomou, Antonio, additional, Drabek-Maunder, Emily, additional, Eyres, Stewart P. S., additional, Fiege, Jason, additional, Friesen, Rachel K., additional, Fuller, Gary, additional, Gledhill, Tim, additional, Griffin, Matt J., additional, Gu, Qilao, additional, Hatchell, Jennifer, additional, Holland, Wayne, additional, Inoue, Tsuyoshi, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Kang, Sung-ju, additional, Kemper, Francisca, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Lacaille, Kevin M., additional, Lee, Jeong-Eun, additional, Li, Dalei, additional, Liu, Junhao, additional, Liu, Sheng-Yuan, additional, Moriarty-Schieven, Gerald H., additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Peretto, Nicolas, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Tang, Ya-Wen, additional, Tomisaka, Kohji, additional, Wang, Hongchi, additional, Wang, Jia-Wei, additional, Yen, Hsi-Wei, additional, Yuan, Jinghua, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, André, Philippe, additional, Dowell, C. Darren, additional, Falle, Sam, additional, Tsukamoto, Yusuke, additional, Kanamori, Yoshihiro, additional, Kataoka, Akimasa, additional, Kobayashi, Masato I. N., additional, Nagata, Tetsuya, additional, Saito, Hiro, additional, Seta, Masumichi, additional, Hwang, Jihye, additional, Han, Ilseung, additional, Lee, Hyeseung, additional, and Zenko, Tetsuya, additional
Published: 2018
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27. A First Look at BISTRO Observations of the ρ Oph-A core

Author: Kwon, Jungmi, primary, Doi, Yasuo, additional, Tamura, Motohide, additional, Matsumura, Masafumi, additional, Pattle, Kate, additional, Berry, David, additional, Sadavoy, Sarah, additional, Matthews, Brenda C., additional, Ward-Thompson, Derek, additional, Hasegawa, Tetsuo, additional, Furuya, Ray S., additional, Pon, Andy, additional, Francesco, James Di, additional, Arzoumanian, Doris, additional, Hayashi, Saeko S., additional, Kawabata, Koji S., additional, Onaka, Takashi, additional, Choi, Minho, additional, Kang, Miju, additional, Hoang, Thiem, additional, Lee, Chang Won, additional, Lee, Sang-Sung, additional, Liu, Hong-Li, additional, Liu, Tie, additional, Inutsuka, Shu-ichiro, additional, Eswaraiah, Chakali, additional, Bastien, Pierre, additional, Kwon, Woojin, additional, Lai, Shih-Ping, additional, Qiu, Keping, additional, Coudé, Simon, additional, Franzmann, Erica, additional, Friberg, Per, additional, Graves, Sarah F., additional, Greaves, Jane S., additional, Houde, Martin, additional, Johnstone, Doug, additional, Kirk, Jason M., additional, Koch, Patrick M., additional, Li, Di, additional, Parsons, Harriet, additional, Rao, Ramprasad, additional, Rawlings, Mark G., additional, Shinnaga, Hiroko, additional, Loo, Sven van, additional, Aso, Yusuke, additional, Byun, Do-Young, additional, Chen, Huei-Ru, additional, Chen, Mike C.-Y., additional, Chen, Wen Ping, additional, Ching, Tao-Chung, additional, Cho, Jungyeon, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Drabek-Maunder, Emily, additional, Eyres, Stewart P. S., additional, Fiege, Jason, additional, Friesen, Rachel K., additional, Fuller, Gary, additional, Gledhill, Tim, additional, Griffin, Matt J., additional, Gu, Qilao, additional, Hatchell, Jennifer, additional, Holland, Wayne, additional, Inoue, Tsuyoshi, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Kang, Ji-hyun, additional, Kang, Sung-ju, additional, Kemper, Francisca, additional, Kim, Gwanjeong, additional, Kim, Jongsoo, additional, Kim, Kee-Tae, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Lacaille, Kevin M., additional, Lee, Jeong-Eun, additional, Li, Dalei, additional, Li, Hua-bai, additional, Liu, Junhao, additional, Liu, Sheng-Yuan, additional, Lyo, A-Ran, additional, Mairs, Steve, additional, Moriarty-Schieven, Gerald H., additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Peretto, Nicolas, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Robitaille, Jean-Franois, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Soam, Archana, additional, Tang, Ya-Wen, additional, Tomisaka, Kohji, additional, Wang, Hongchi, additional, Wang, Jia-Wei, additional, Whitworth, Anthony P., additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, Yuan, Jinghua, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, André, Philippe, additional, Dowell, C. Darren, additional, Falle, Sam, additional, Tsukamoto, Yusuke, additional, Nakagawa, Takao, additional, Kanamori, Yoshihiro, additional, Kataoka, Akimasa, additional, Kobayashi, Masato I. N., additional, Nagata, Tetsuya, additional, Saito, Hiro, additional, Seta, Masumichi, additional, and Zenko, Tetsuya, additional
Published: 2018
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28. The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17

Author: Liu, Tie, primary, Kim, Kee-Tae, additional, Juvela, Mika, additional, Wang, Ke, additional, Tatematsu, Ken’ichi, additional, Francesco, James Di, additional, Liu, Sheng-Yuan, additional, Wu, Yuefang, additional, Thompson, Mark, additional, Fuller, Gary, additional, Eden, David, additional, Li, Di, additional, Ristorcelli, I., additional, Kang, Sung-ju, additional, Lin, Yuxin, additional, Johnstone, D., additional, He, J. H., additional, Koch, P. M., additional, Sanhueza, Patricio, additional, Qin, Sheng-Li, additional, Zhang, Q., additional, Hirano, N., additional, Goldsmith, Paul F., additional, Evans II, Neal J., additional, White, Glenn J., additional, Choi, Minho, additional, Lee, Chang Won, additional, Toth, L. V., additional, Mairs, Steve, additional, Yi, H.-W., additional, Tang, Mengyao, additional, Soam, Archana, additional, Peretto, N., additional, Samal, Manash R., additional, Fich, Michel, additional, Parsons, Harriet, additional, Yuan, Jinghua, additional, Zhang, Chuan-Peng, additional, Malinen, Johanna, additional, Bendo, George J., additional, Rivera-Ingraham, A., additional, Liu, Hong-Li, additional, Wouterloot, Jan, additional, Li, Pak Shing, additional, Qian, Lei, additional, Rawlings, Jonathan, additional, Rawlings, Mark G., additional, Feng, Siyi, additional, Aikawa, Yuri, additional, Akhter, S., additional, Alina, Dana, additional, Bell, Graham, additional, Bernard, J.-P., additional, Blain, Andrew, additional, Bőgner, Rebeka, additional, Bronfman, L., additional, Byun, D.-Y., additional, Chapman, Scott, additional, Chen, Huei-Ru, additional, Chen, M., additional, Chen, Wen-Ping, additional, Chen, X., additional, Chen, Xuepeng, additional, Chrysostomou, A., additional, Cosentino, Giuliana, additional, Cunningham, M. R., additional, Demyk, K., additional, Drabek-Maunder, Emily, additional, Doi, Yasuo, additional, Eswaraiah, C., additional, Falgarone, Edith, additional, Fehér, O., additional, Fraser, Helen, additional, Friberg, Per, additional, Garay, G., additional, Ge, J. X., additional, Gear, W. K., additional, Greaves, Jane, additional, Guan, X., additional, Harvey-Smith, Lisa, additional, HASEGAWA, Tetsuo, additional, Hatchell, J., additional, He, Yuxin, additional, Henkel, C., additional, Hirota, T., additional, Holland, W., additional, Hughes, A., additional, Jarken, E., additional, Ji, Tae-Geun, additional, Jimenez-Serra, Izaskun, additional, Kang, Miju, additional, Kawabata, Koji S., additional, Kim, Gwanjeong, additional, Kim, Jungha, additional, Kim, Jongsoo, additional, Kim, Shinyoung, additional, Koo, B.-C., additional, Kwon, Woojin, additional, Kuan, Yi-Jehng, additional, Lacaille, K. M., additional, Lai, Shih-Ping, additional, Lee, C. F., additional, Lee, J.-E., additional, Lee, Y.-U., additional, Li, Dalei, additional, Li, Hua-bai, additional, Lo, N., additional, Lopez, John A. P., additional, Lu, Xing, additional, Lyo, A-Ran, additional, Mardones, D., additional, Marston, A., additional, McGehee, P., additional, Meng, F., additional, Montier, L., additional, Montillaud, Julien, additional, Moore, T., additional, Morata, O., additional, Moriarty-Schieven, Gerald H., additional, Ohashi, S., additional, Pak, Soojong, additional, Park, Geumsook, additional, Paladini, R., additional, Pattle, Kate M, additional, Pech, Gerardo, additional, Pelkonen, V.-M., additional, Qiu, K., additional, Ren, Zhi-Yuan, additional, Richer, John, additional, Saito, M., additional, Sakai, Takeshi, additional, Shang, H., additional, Shinnaga, Hiroko, additional, Stamatellos, Dimitris, additional, Tang, Y.-W., additional, Traficante, Alessio, additional, Vastel, Charlotte, additional, Viti, S., additional, Walsh, Andrew, additional, Wang, Bingru, additional, Wang, Hongchi, additional, Wang, Junzhi, additional, Ward-Thompson, D., additional, Whitworth, Anthony, additional, Xu, Ye, additional, Yang, J., additional, Yang, Yao-Lun, additional, Yuan, Lixia, additional, Zavagno, A., additional, Zhang, Guoyin, additional, Zhang, H.-W., additional, Zhou, Chenlin, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, Zuo, Pei, additional, and Zhang, Chao, additional
Published: 2018
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29. First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt

Author: Ward-Thompson, Derek, primary, Pattle, Kate, additional, Bastien, Pierre, additional, Furuya, Ray S., additional, Kwon, Woojin, additional, Lai, Shih-Ping, additional, Qiu, Keping, additional, Berry, David, additional, Choi, Minho, additional, Coudé, Simon, additional, Francesco, James Di, additional, Hoang, Thiem, additional, Franzmann, Erica, additional, Friberg, Per, additional, Graves, Sarah F., additional, Greaves, Jane S., additional, Houde, Martin, additional, Johnstone, Doug, additional, Kirk, Jason M., additional, Koch, Patrick M., additional, Kwon, Jungmi, additional, Lee, Chang Won, additional, Li, Di, additional, Matthews, Brenda C., additional, Mottram, Joseph C., additional, Parsons, Harriet, additional, Pon, Andy, additional, Rao, Ramprasad, additional, Rawlings, Mark, additional, Shinnaga, Hiroko, additional, Sadavoy, Sarah, additional, Loo, Sven van, additional, Aso, Yusuke, additional, Byun, Do-Young, additional, Eswaraiah, Chakali, additional, Chen, Huei-Ru, additional, Chen, Mike C.-Y., additional, Chen, Wen Ping, additional, Ching, Tao-Chung, additional, Cho, Jungyeon, additional, Chrysostomou, Antonio, additional, Chung, Eun Jung, additional, Doi, Yasuo, additional, Drabek-Maunder, Emily, additional, Eyres, Stewart P. S., additional, Fiege, Jason, additional, Friesen, Rachel K., additional, Fuller, Gary, additional, Gledhill, Tim, additional, Griffin, Matt J., additional, Gu, Qilao, additional, Hasegawa, Tetsuo, additional, Hatchell, Jennifer, additional, Hayashi, Saeko S., additional, Holland, Wayne, additional, Inoue, Tsuyoshi, additional, Inutsuka, Shu-ichiro, additional, Iwasaki, Kazunari, additional, Jeong, Il-Gyo, additional, Kang, Ji-hyun, additional, Kang, Miju, additional, Kang, Sung-ju, additional, Kawabata, Koji S., additional, Kemper, Francisca, additional, Kim, Gwanjeong, additional, Kim, Jongsoo, additional, Kim, Kee-Tae, additional, Kim, Kyoung Hee, additional, Kim, Mi-Ryang, additional, Kim, Shinyoung, additional, Lacaille, Kevin M., additional, Lee, Jeong-Eun, additional, Lee, Sang-Sung, additional, Li, Dalei, additional, Li, Hua-bai, additional, Liu, Hong-Li, additional, Liu, Junhao, additional, Liu, Sheng-Yuan, additional, Liu, Tie, additional, Lyo, A-Ran, additional, Mairs, Steve, additional, Matsumura, Masafumi, additional, Moriarty-Schieven, Gerald H., additional, Nakamura, Fumitaka, additional, Nakanishi, Hiroyuki, additional, Ohashi, Nagayoshi, additional, Onaka, Takashi, additional, Peretto, Nicolas, additional, Pyo, Tae-Soo, additional, Qian, Lei, additional, Retter, Brendan, additional, Richer, John, additional, Rigby, Andrew, additional, Robitaille, Jean-François, additional, Savini, Giorgio, additional, Scaife, Anna M. M., additional, Soam, Archana, additional, Tamura, Motohide, additional, Tang, Ya-Wen, additional, Tomisaka, Kohji, additional, Wang, Hongchi, additional, Wang, Jia-Wei, additional, Whitworth, Anthony P., additional, Yen, Hsi-Wei, additional, Yoo, Hyunju, additional, Yuan, Jinghua, additional, Zhang, Chuan-Peng, additional, Zhang, Guoyin, additional, Zhou, Jianjun, additional, Zhu, Lei, additional, André, Philippe, additional, Dowell, C. Darren, additional, Falle, Sam, additional, and Tsukamoto, Yusuke, additional
Published: 2017
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30. SONS: The JCMT legacy survey of debris discs in the submillimetre

Author: Holland, Wayne S., primary, Matthews, Brenda C., additional, Kennedy, Grant M., additional, Greaves, Jane S., additional, Wyatt, Mark C., additional, Booth, Mark, additional, Bastien, Pierre, additional, Bryden, Geoff, additional, Butner, Harold, additional, Chen, Christine H., additional, Chrysostomou, Antonio, additional, Davies, Claire L., additional, Dent, William R. F., additional, Di Francesco, James, additional, Duchêne, Gaspard, additional, Gibb, Andy G., additional, Friberg, Per, additional, Ivison, Rob J., additional, Jenness, Tim, additional, Kavelaars, JJ, additional, Lawler, Samantha, additional, Lestrade, Jean-François, additional, Marshall, Jonathan P., additional, Moro-Martin, Amaya, additional, Panić, Olja, additional, Phillips, Neil, additional, Serjeant, Stephen, additional, Schieven, Gerald H., additional, Sibthorpe, Bruce, additional, Vican, Laura, additional, Ward-Thompson, Derek, additional, van der Werf, Paul, additional, White, Glenn J., additional, Wilner, David, additional, and Zuckerman, Ben, additional
Published: 2017
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31. V2494 Cyg: a unique FU Ori type object in the Cygnus OB7 complex

Author: Magakian, Tigran Yu., primary, Nikogossian, Elena H., additional, Movsessian, Tigran, additional, Moiseev, Alexei, additional, Aspin, Colin, additional, Davis, Chris J., additional, Pyo, Tae-Soo, additional, Khanzadyan, Tigran, additional, Froebrich, Dirk, additional, Smith, Michael D., additional, Moriarty-Schieven, Gerald H., additional, and Beck, Tracy L., additional
Published: 2013
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32. CSO BOLOCAM 1.1 mm CONTINUUM MAPPING OF THE BRAID NEBULA STAR FORMATION REGION IN CYGNUS OB7

Author: Aspin, Colin, primary, Beck, Tracy L., additional, Davis, Chris J., additional, Froebrich, Dirk, additional, Khanzadyan, Tigran, additional, Magakian, Tigran Yu., additional, Moriarty-Schieven, Gerald H., additional, Movsessian, Tigran A., additional, Mitchison, Sharon, additional, Nikogossian, Elena G., additional, Pyo, Tae-Soo, additional, and Smith, Michael D., additional
Published: 2011
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33. A WIDE-FIELD NARROWBAND OPTICAL SURVEY OF THE BRAID NEBULA STAR FORMATION REGION IN CYGNUS OB7

Author: Magakian, Tigran Yu., primary, Nikogossian, Elena H., additional, Aspin, Colin, additional, Pyo, Tae-Soo, additional, Khanzadyan, Tigran, additional, Movsessian, Tigran, additional, Smith, Michael D., additional, Mitchison, Sharon, additional, Davis, Chris J., additional, Beck, Tracy L., additional, and Moriarty-Schieven, Gerald H., additional
Published: 2010
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34. THE LOCAL ENVIRONMENT OF THE FU-ORIONIS-LIKE OBJECTS AR 6A AND 6B

Author: Moriarty-Schieven, Gerald H., primary, Aspin, Colin, additional, and Davis, Gary R., additional
Published: 2008
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35. Multigenerational Star Formation in L1551

Author: Moriarty‐Schieven, Gerald H., primary, Johnstone, Doug, additional, Bally, John, additional, and Jenness, Tim, additional
Published: 2006
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36. Physical Properties and Kinetic Structure of a Starless Core in Taurus Molecular Cloud

Author: Shinnaga, Hiroko, primary, Ohashi, Nagayoshi, additional, Lee, Siow‐Wang, additional, and Moriarty‐Schieven, Gerald H., additional
Published: 2004
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37. Submillimeter Continuum Emission in the ρ Ophiuchi Molecular Cloud: Filaments, Arcs, and an Unidentified Far-Infrared Object

Author: Wilson, Christine D., primary, Avery, Lorne W., additional, Fich, Michel, additional, Johnstone, Doug, additional, Joncas, Gilles, additional, Knee, Lewis B. G., additional, Matthews, Henry E., additional, Mitchell, George F., additional, Moriarty-Schieven, Gerald H., additional, and Pudritz, Ralph E., additional
Published: 1999
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38. 6.7 GHz Methanol Masers Associated with [ITAL]IRAS[/ITAL]-Selected Sources

Author: MacLeod, Gordon C., primary, van der Walt, D. Johan, additional, North, Adrian, additional, Gaylard, Michael J., additional, Galt, John A., additional, and Moriarty-Schieven, Gerald H., additional
Published: 1998
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39. A textbook case of bow shock entrainment in a YSO outflow

Author: Davis, Christopher J., primary, Smith, Michael D., additional, and Moriarty-Schieven, Gerald H., additional
Published: 1998
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40. A Submillimeter‐Wave “Flare” from GG Tauri?

Author: Moriarty‐Schieven, Gerald H., primary and Butner, Harold M., additional
Published: 1997
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41. Interferometric Observations of Outflows From Low-Mass Protostars in Taurus

Author: Tamura, Motohide, primary, Ohashi, Nagayoshi, additional, Hirano, Naomi, additional, Itoh, Yoichi, additional, and Moriarty-Schieven, Gerald H., additional
Published: 1996
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42. The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17

Author: Liu, Tie, Kim, Kee-Tae, Juvela, Mika, Wang, Ke, Tatematsu, Ken’ichi, Francesco, James Di, Liu, Sheng-Yuan, Wu, Yuefang, Thompson, Mark, Fuller, Gary, Eden, David, Li, Di, Ristorcelli, I., Kang, Sung-ju, Lin, Yuxin, Johnstone, D., He, J. H., Koch, P. M., Sanhueza, Patricio, Qin, Sheng-Li, Zhang, Q., Hirano, N., Goldsmith, Paul F., Evans II, Neal J., White, Glenn J., Choi, Minho, Lee, Chang Won, Toth, L. V., Mairs, Steve, Yi, H.-W., Tang, Mengyao, Soam, Archana, Peretto, N., Samal, Manash R., Fich, Michel, Parsons, Harriet, Yuan, Jinghua, Zhang, Chuan-Peng, Malinen, Johanna, Bendo, George J., Rivera-Ingraham, A., Liu, Hong-Li, Wouterloot, Jan, Li, Pak Shing, Qian, Lei, Rawlings, Jonathan, Rawlings, Mark G., Feng, Siyi, Aikawa, Yuri, Akhter, S., Alina, Dana, Bell, Graham, Bernard, J.-P., Blain, Andrew, Bőgner, Rebeka, Bronfman, L., Byun, D.-Y., Chapman, Scott, Chen, Huei-Ru, Chen, M., Chen, Wen-Ping, Chen, X., Chen, Xuepeng, Chrysostomou, A., Cosentino, Giuliana, Cunningham, M. R., Demyk, K., Drabek-Maunder, Emily, Doi, Yasuo, Eswaraiah, C., Falgarone, Edith, Fehér, O., Fraser, Helen, Friberg, Per, Garay, G., Ge, J. X., Gear, W. K., Greaves, Jane, Guan, X., Harvey-Smith, Lisa, HASEGAWA, Tetsuo, Hatchell, J., He, Yuxin, Henkel, C., Hirota, T., Holland, W., Hughes, A., Jarken, E., Ji, Tae-Geun, Jimenez-Serra, Izaskun, Kang, Miju, Kawabata, Koji S., Kim, Gwanjeong, Kim, Jungha, Kim, Jongsoo, Kim, Shinyoung, Koo, B.-C., Kwon, Woojin, Kuan, Yi-Jehng, Lacaille, K. M., Lai, Shih-Ping, Lee, C. F., Lee, J.-E., Lee, Y.-U., Li, Dalei, Li, Hua-bai, Lo, N., Lopez, John A. P., Lu, Xing, Lyo, A-Ran, Mardones, D., Marston, A., McGehee, P., Meng, F., Montier, L., Montillaud, Julien, Moore, T., Morata, O., Moriarty-Schieven, Gerald H., Ohashi, S., Pak, Soojong, Park, Geumsook, Paladini, R., Pattle, Kate M, Pech, Gerardo, Pelkonen, V.-M., Qiu, K., Ren, Zhi-Yuan, Richer, John, Saito, M., Sakai, Takeshi, Shang, H., Shinnaga, Hiroko, Stamatellos, Dimitris, Tang, Y.-W., Traficante, Alessio, Vastel, Charlotte, Viti, S., Walsh, Andrew, Wang, Bingru, Wang, Hongchi, Wang, Junzhi, Ward-Thompson, D., Whitworth, Anthony, Xu, Ye, Yang, J., Yang, Yao-Lun, Yuan, Lixia, Zavagno, A., Zhang, Guoyin, Zhang, H.-W., Zhou, Chenlin, Zhou, Jianjun, Zhu, Lei, Zuo, Pei, Zhang, Chao, Liu, Tie, Kim, Kee-Tae, Juvela, Mika, Wang, Ke, Tatematsu, Ken’ichi, Francesco, James Di, Liu, Sheng-Yuan, Wu, Yuefang, Thompson, Mark, Fuller, Gary, Eden, David, Li, Di, Ristorcelli, I., Kang, Sung-ju, Lin, Yuxin, Johnstone, D., He, J. H., Koch, P. M., Sanhueza, Patricio, Qin, Sheng-Li, Zhang, Q., Hirano, N., Goldsmith, Paul F., Evans II, Neal J., White, Glenn J., Choi, Minho, Lee, Chang Won, Toth, L. V., Mairs, Steve, Yi, H.-W., Tang, Mengyao, Soam, Archana, Peretto, N., Samal, Manash R., Fich, Michel, Parsons, Harriet, Yuan, Jinghua, Zhang, Chuan-Peng, Malinen, Johanna, Bendo, George J., Rivera-Ingraham, A., Liu, Hong-Li, Wouterloot, Jan, Li, Pak Shing, Qian, Lei, Rawlings, Jonathan, Rawlings, Mark G., Feng, Siyi, Aikawa, Yuri, Akhter, S., Alina, Dana, Bell, Graham, Bernard, J.-P., Blain, Andrew, Bőgner, Rebeka, Bronfman, L., Byun, D.-Y., Chapman, Scott, Chen, Huei-Ru, Chen, M., Chen, Wen-Ping, Chen, X., Chen, Xuepeng, Chrysostomou, A., Cosentino, Giuliana, Cunningham, M. R., Demyk, K., Drabek-Maunder, Emily, Doi, Yasuo, Eswaraiah, C., Falgarone, Edith, Fehér, O., Fraser, Helen, Friberg, Per, Garay, G., Ge, J. X., Gear, W. K., Greaves, Jane, Guan, X., Harvey-Smith, Lisa, HASEGAWA, Tetsuo, Hatchell, J., He, Yuxin, Henkel, C., Hirota, T., Holland, W., Hughes, A., Jarken, E., Ji, Tae-Geun, Jimenez-Serra, Izaskun, Kang, Miju, Kawabata, Koji S., Kim, Gwanjeong, Kim, Jungha, Kim, Jongsoo, Kim, Shinyoung, Koo, B.-C., Kwon, Woojin, Kuan, Yi-Jehng, Lacaille, K. M., Lai, Shih-Ping, Lee, C. F., Lee, J.-E., Lee, Y.-U., Li, Dalei, Li, Hua-bai, Lo, N., Lopez, John A. P., Lu, Xing, Lyo, A-Ran, Mardones, D., Marston, A., McGehee, P., Meng, F., Montier, L., Montillaud, Julien, Moore, T., Morata, O., Moriarty-Schieven, Gerald H., Ohashi, S., Pak, Soojong, Park, Geumsook, Paladini, R., Pattle, Kate M, Pech, Gerardo, Pelkonen, V.-M., Qiu, K., Ren, Zhi-Yuan, Richer, John, Saito, M., Sakai, Takeshi, Shang, H., Shinnaga, Hiroko, Stamatellos, Dimitris, Tang, Y.-W., Traficante, Alessio, Vastel, Charlotte, Viti, S., Walsh, Andrew, Wang, Bingru, Wang, Hongchi, Wang, Junzhi, Ward-Thompson, D., Whitworth, Anthony, Xu, Ye, Yang, J., Yang, Yao-Lun, Yuan, Lixia, Zavagno, A., Zhang, Guoyin, Zhang, H.-W., Zhou, Chenlin, Zhou, Jianjun, Zhu, Lei, Zuo, Pei, and Zhang, Chao
Abstract: The low dust temperatures (<14 K) of Planck Galactic cold clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. "TOP-SCOPE" is a joint survey program targeting ~2000 PGCCs in J = 1–0 transitions of CO isotopologues and ~1000 PGCCs in 850 μm continuum emission. The objective of the "TOP-SCOPE" survey and the joint surveys (SMT 10 m, KVN 21 m, and NRO 45 m) is to statistically study the initial conditions occurring during star formation and the evolution of molecular clouds, across a wide range of environments. The observations, data analysis, and example science cases for these surveys are introduced with an exemplar source, PGCC G26.53+0.17 (G26), which is a filamentary infrared dark cloud (IRDC). The total mass, length, and mean line mass (M/L) of the G26 filament are ~6200 M ☉, ~12 pc, and ~500 M ☉ pc−1, respectively. Ten massive clumps, including eight starless ones, are found along the filament. The most massive clump as a whole may still be in global collapse, while its denser part seems to be undergoing expansion owing to outflow feedback. The fragmentation in the G26 filament from cloud scale to clump scale is in agreement with gravitational fragmentation of an isothermal, nonmagnetized, and turbulent supported cylinder. A bimodal behavior in dust emissivity spectral index (β) distribution is found in G26, suggesting grain growth along the filament. The G26 filament may be formed owing to large-scale compression flows evidenced by the temperature and velocity gradients across its natal cloud.

43. SONS: The JCMT legacy survey of debris discs in the submillimetre

Author: Holland, Wayne S., Matthews, Brenda C., Kennedy, Grant M., Greaves, Jane S., Wyatt, Mark C., Booth, Mark, Bastien, Pierre, Bryden, Geoff, Butner, Harold, Chen, Christine H., Chrysostomou, Antonio, Davies, Claire L., Dent, William R. F., Francesco, James Di, Duchêne, Gaspard, Gibb, Andy G., Friberg, Per, Ivison, Rob J., Jenness, Tim, Lawler, Samantha, Lestrade, Jean-Franois, Marshall, Jonathan P., Moro-Martin, Amaya, Panić, Olja, Phillips, Neil, Serjeant, Stephen, Schieven, Gerald H., Sibthorpe, Bruce, Vican, Laura, Ward-Thompson, Derek, Werf, Paul van der, White, Glenn J., Wilner, David, Zuckerman, Ben, Holland, Wayne S., Matthews, Brenda C., Kennedy, Grant M., Greaves, Jane S., Wyatt, Mark C., Booth, Mark, Bastien, Pierre, Bryden, Geoff, Butner, Harold, Chen, Christine H., Chrysostomou, Antonio, Davies, Claire L., Dent, William R. F., Francesco, James Di, Duchêne, Gaspard, Gibb, Andy G., Friberg, Per, Ivison, Rob J., Jenness, Tim, Lawler, Samantha, Lestrade, Jean-Franois, Marshall, Jonathan P., Moro-Martin, Amaya, Panić, Olja, Phillips, Neil, Serjeant, Stephen, Schieven, Gerald H., Sibthorpe, Bruce, Vican, Laura, Ward-Thompson, Derek, Werf, Paul van der, White, Glenn J., Wilner, David, and Zuckerman, Ben
Abstract: Debris discs are evidence of the ongoing destructive collisions between planetesimals, and their presence around stars also suggests that planets exist in these systems. In this paper, we present submillimetre images of the thermal emission from debris discs that formed the SCUBA-2 Observations of Nearby Stars (SONS) survey, one of seven legacy surveys undertaken on the James Clerk Maxwell telescope between 2012 and 2015. The overall results of the survey are presented in the form of 850 microns (and 450 microns, where possible) images and fluxes for the observed fields. Excess thermal emission, over that expected from the stellar photosphere, is detected around 49 stars out of the 100 observed fields. The discs are characterised in terms of their flux density, size (radial distribution of the dust) and derived dust properties from their spectral energy distributions. The results show discs over a range of sizes, typically 1-10 times the diameter of the Edgeworth-Kuiper Belt in our Solar System. The mass of a disc, for particles up to a few millimetres in size, is uniquely obtainable with submillimetre observations and this quantity is presented as a function of the host stars' age, showing a tentative decline in mass with age. Having doubled the number of imaged discs at submillimetre wavelengths from ground-based, single dish telescope observations, one of the key legacy products from the SONS survey is to provide a comprehensive target list to observe at high angular resolution using submillimetre/millimetre interferometers (e.g., ALMA, SMA).

44. The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Author: Cooray, Asantha, Eales, Steve, Chapman, Scott, Clements, David L., Dore, Olivier, Farrah, Duncan, Jarvis, Matt J., Kaplinghat, Manoj, Negrello, Mattia, Melchiorri, Alessandro, Peiris, Hiranya, Pope, Alexandra, Santos, Mario G., Serjeant, Stephen, Thompson, Mark, White, Glenn, Amblard, Alexandre, Banerji, Manda, Corasaniti, Pier-Stefano, Das, Sudeep, de Bernardis, Francesco, de Zotti, Gianfranco, Giannantonio, Tommaso, Gonzalez-Nuevo Gonzalez, Joaquin, Khostovan, Ali Ahmad, Mitchell-Wynne, Ketron, Serra, Paolo, Song, Yong-Seon, Vieira, Joaquin, Wang, Lingyu, Zemcov, Michael, Abdalla, Filipe, Afonso, Jose, Aghanim, Nabila, Andreani, Paola, Aretxaga, Itziar, Auld, Robbie, Baes, Maarten, Baker, Andrew, Barkats, Denis, Belen Barreiro, R., Bartolo, Nicola, Barton, Elizabeth, Barway, Sudhanshu, Stefano Battistelli, Elia, Baugh, Carlton, Beelen, Alexander, Benabed, Karim, Blain, Andrew, Bland-Hawthorn, Joss, Bock, James~J., Bond, J. Richard, Borrill, Julian, Borys, Colin, Boselli, Alessandro, Bouchet, Francois R., Bridge, Carrie, Brighenti, Fabrizio, Buat, Veronique, Buote, David, Burgarella, Denis, Bussmann, Robert, Calabrese, Erminia, Cantalupo, Christopher, Carlberg, Raymond, Sofia Carvalho, Carla, Casey, Caitlin, Cava, Antonio, Cepa, Jordi, Chapin, Edward, Chary, Ranga Ram, Chen, Xuelei, Colafrancesco, Sergio, Cole, Shaun, Coles, Peter, Conley, Alexander, Conversi, Luca, Cooke, Jeff, Crawford, Steven, Cress, Catherine, da Cunha, Elisabete, Dalton, Gavin, Danese, Luigi, Dannerbauer, Helmut, Davies, Jonathan, de Bernardis, Paolo, de Putter, Roland, Devlin, Mark, Diego, Jose M., Dole, Herve, Douspis, Marian, Dunkley, Joanna, Dunlop, James, Dunne, Loretta, Dunner, Rolando, Dye, Simon, Efstathiou, George, Egami, Eiichi, Fang, Taotao, Ferrero, Patrizia, Franceschini, Alberto, Frazer, Christopher C., Frayer, David, Frenk, Carlos, Ganga, Ken, Gavazzi, Raphael, Glenn, Jason, Gong, Yan, Gonzalez-Solares, Eduardo, Griffin, Matt, Guo, Qi, Gurwell, Mark, Hajian, Amir, Halpern, Mark, Hanson, Duncan, Hardcastle, Martin, Hatziminaoglou, Evanthia, Heavens, Alan, Heinis, Sebastien, Herranz, Diego, Hilton, Matt, Ho, Shirley, Holwerda, Benne W., Hopwood, Rosalind, Horner, Jonathan, Huffenberger, Kevin, Hughes, David H., Hughes, John P., Ibar, Edo, Ivison, Rob, Jackson, Neal, Jaffe, Andrew, Jenness, Timothy, Joncas, Gilles, Joudaki, Shahab, Kaviraj, Sugata, Kim, Sam, King, Lindsay, Kisner, Theodore, Knapen, Johan, Kniazev, Alexei, Komatsu, Eiichiro, Koopmans, Leon, Kuo, Chao-Lin, Lacey, Cedric, Lahav, Ofer, Lasenby, Anthony N., Lawrence, Andy, Lee, Myung Gyoon, Leeuw, Lerothodi L., Levenson, Louis R., Lewis, Geraint, Loaring, Nicola, Lopez-Caniego, Marcos, Maddox, Steve, Marriage, Tobias, Marsden, Gaelen, Martinez-Gonzalez, Enrique, Masi, Silvia, Matarrese, Sabino, Mathews, William G., Matsuura, Shuji, McMahon, Richard, Mellier, Yannick, Menanteau, Felipe, Michalowski, Michal~J., Millea, Marius, Mobasher, Bahram, Mohanty, Subhanjoy, Montier, Ludovic, Moodley, Kavilan, Moriarty-Schieven, Gerald H., Mortier, Angela, Munshi, Dipak, Murphy, Eric, Nandra, Kirpal, Natoli, Paolo, Nguyen, Hien, Oliver, Seb, Omont, Alain, Page, Lyman, Page, Mathew, Paladini, Roberta, Pandolfi, Stefania, Pascale, Enzo, Patanchon, Guillaume, Peacock, John, Pearson, Chris, Perez-Fournon, Ismael, Perez-Gonz, Pablo G., Piacentini, Francesco, Pierpaoli, Elena, Pohlen, Michael, Pointecouteau, Etienne, Polenta, Gianluca, Rawlings, Jason, Reese, Erik~D., Rigby, Emma, Rodighiero, Giulia, Romero-Colmenero, Encarni, Roseboom, Isaac, Rowan-Robinson, Michael, Sanchez-Portal, Miguel, Schmidt, Fabian, Schneider, Michael, Schulz, Bernhard, Scott, Douglas, Sedgwick, Chris, Sehgal, Neelima, Seymour, Nick, Sherwin, Blake~D., Short, Jo, Shupe, David, Sievers, Jonathan, Skibba, Ramin, Smidt, Joseph, Smith, Anthony, Smith, Daniel J. B., Smith, Matthew W. L., Spergel, David, Staggs, Suzanne, Stevens, Jason, Switzer, Eric, Takagi, Toshinobu, Takeuchi, Tsutomu, Temi, Pasquale, Trichas, Markos, Trigilio, Corrado, Tugwell, Katherine, Umana, Grazia, Vacca, William, Vaccari, Mattia, Vaisanen, Petri, Valtchanov, Ivan, van der Heyden, Kurt, van der Werf, Paul P., van Kampen, Eelco, van Waerbeke, Ludovic, Vegetti, Simona, Veneziani, Marcella, Verde, Licia, Verma, Aprajita, Vielva, Patricio, Viero, Marco P., Vila Vilaro, Baltasar, Wardlow, Julie, Wilson, Grant, Wright, Edward L., Xu, C. Kevin, Yun, Min S., Cooray, Asantha, Eales, Steve, Chapman, Scott, Clements, David L., Dore, Olivier, Farrah, Duncan, Jarvis, Matt J., Kaplinghat, Manoj, Negrello, Mattia, Melchiorri, Alessandro, Peiris, Hiranya, Pope, Alexandra, Santos, Mario G., Serjeant, Stephen, Thompson, Mark, White, Glenn, Amblard, Alexandre, Banerji, Manda, Corasaniti, Pier-Stefano, Das, Sudeep, de Bernardis, Francesco, de Zotti, Gianfranco, Giannantonio, Tommaso, Gonzalez-Nuevo Gonzalez, Joaquin, Khostovan, Ali Ahmad, Mitchell-Wynne, Ketron, Serra, Paolo, Song, Yong-Seon, Vieira, Joaquin, Wang, Lingyu, Zemcov, Michael, Abdalla, Filipe, Afonso, Jose, Aghanim, Nabila, Andreani, Paola, Aretxaga, Itziar, Auld, Robbie, Baes, Maarten, Baker, Andrew, Barkats, Denis, Belen Barreiro, R., Bartolo, Nicola, Barton, Elizabeth, Barway, Sudhanshu, Stefano Battistelli, Elia, Baugh, Carlton, Beelen, Alexander, Benabed, Karim, Blain, Andrew, Bland-Hawthorn, Joss, Bock, James~J., Bond, J. Richard, Borrill, Julian, Borys, Colin, Boselli, Alessandro, Bouchet, Francois R., Bridge, Carrie, Brighenti, Fabrizio, Buat, Veronique, Buote, David, Burgarella, Denis, Bussmann, Robert, Calabrese, Erminia, Cantalupo, Christopher, Carlberg, Raymond, Sofia Carvalho, Carla, Casey, Caitlin, Cava, Antonio, Cepa, Jordi, Chapin, Edward, Chary, Ranga Ram, Chen, Xuelei, Colafrancesco, Sergio, Cole, Shaun, Coles, Peter, Conley, Alexander, Conversi, Luca, Cooke, Jeff, Crawford, Steven, Cress, Catherine, da Cunha, Elisabete, Dalton, Gavin, Danese, Luigi, Dannerbauer, Helmut, Davies, Jonathan, de Bernardis, Paolo, de Putter, Roland, Devlin, Mark, Diego, Jose M., Dole, Herve, Douspis, Marian, Dunkley, Joanna, Dunlop, James, Dunne, Loretta, Dunner, Rolando, Dye, Simon, Efstathiou, George, Egami, Eiichi, Fang, Taotao, Ferrero, Patrizia, Franceschini, Alberto, Frazer, Christopher C., Frayer, David, Frenk, Carlos, Ganga, Ken, Gavazzi, Raphael, Glenn, Jason, Gong, Yan, Gonzalez-Solares, Eduardo, Griffin, Matt, Guo, Qi, Gurwell, Mark, Hajian, Amir, Halpern, Mark, Hanson, Duncan, Hardcastle, Martin, Hatziminaoglou, Evanthia, Heavens, Alan, Heinis, Sebastien, Herranz, Diego, Hilton, Matt, Ho, Shirley, Holwerda, Benne W., Hopwood, Rosalind, Horner, Jonathan, Huffenberger, Kevin, Hughes, David H., Hughes, John P., Ibar, Edo, Ivison, Rob, Jackson, Neal, Jaffe, Andrew, Jenness, Timothy, Joncas, Gilles, Joudaki, Shahab, Kaviraj, Sugata, Kim, Sam, King, Lindsay, Kisner, Theodore, Knapen, Johan, Kniazev, Alexei, Komatsu, Eiichiro, Koopmans, Leon, Kuo, Chao-Lin, Lacey, Cedric, Lahav, Ofer, Lasenby, Anthony N., Lawrence, Andy, Lee, Myung Gyoon, Leeuw, Lerothodi L., Levenson, Louis R., Lewis, Geraint, Loaring, Nicola, Lopez-Caniego, Marcos, Maddox, Steve, Marriage, Tobias, Marsden, Gaelen, Martinez-Gonzalez, Enrique, Masi, Silvia, Matarrese, Sabino, Mathews, William G., Matsuura, Shuji, McMahon, Richard, Mellier, Yannick, Menanteau, Felipe, Michalowski, Michal~J., Millea, Marius, Mobasher, Bahram, Mohanty, Subhanjoy, Montier, Ludovic, Moodley, Kavilan, Moriarty-Schieven, Gerald H., Mortier, Angela, Munshi, Dipak, Murphy, Eric, Nandra, Kirpal, Natoli, Paolo, Nguyen, Hien, Oliver, Seb, Omont, Alain, Page, Lyman, Page, Mathew, Paladini, Roberta, Pandolfi, Stefania, Pascale, Enzo, Patanchon, Guillaume, Peacock, John, Pearson, Chris, Perez-Fournon, Ismael, Perez-Gonz, Pablo G., Piacentini, Francesco, Pierpaoli, Elena, Pohlen, Michael, Pointecouteau, Etienne, Polenta, Gianluca, Rawlings, Jason, Reese, Erik~D., Rigby, Emma, Rodighiero, Giulia, Romero-Colmenero, Encarni, Roseboom, Isaac, Rowan-Robinson, Michael, Sanchez-Portal, Miguel, Schmidt, Fabian, Schneider, Michael, Schulz, Bernhard, Scott, Douglas, Sedgwick, Chris, Sehgal, Neelima, Seymour, Nick, Sherwin, Blake~D., Short, Jo, Shupe, David, Sievers, Jonathan, Skibba, Ramin, Smidt, Joseph, Smith, Anthony, Smith, Daniel J. B., Smith, Matthew W. L., Spergel, David, Staggs, Suzanne, Stevens, Jason, Switzer, Eric, Takagi, Toshinobu, Takeuchi, Tsutomu, Temi, Pasquale, Trichas, Markos, Trigilio, Corrado, Tugwell, Katherine, Umana, Grazia, Vacca, William, Vaccari, Mattia, Vaisanen, Petri, Valtchanov, Ivan, van der Heyden, Kurt, van der Werf, Paul P., van Kampen, Eelco, van Waerbeke, Ludovic, Vegetti, Simona, Veneziani, Marcella, Verde, Licia, Verma, Aprajita, Vielva, Patricio, Viero, Marco P., Vila Vilaro, Baltasar, Wardlow, Julie, Wilson, Grant, Wright, Edward L., Xu, C. Kevin, and Yun, Min S.
Abstract: A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwave background experiments. The Herschel-SPIRE Legacy Survey (HSLS), will lead to imaging data over 4000 sq. degrees at 250, 350, and 500 micron. Major Goals of HSLS are: (a) produce a catalog of 2.5 to 3 million galaxies down to 26, 27 and 33 mJy (50% completeness; 5 sigma confusion noise) at 250, 350 and 500 micron, respectively, in the southern hemisphere (3000 sq. degrees) and in an equatorial strip (1000 sq. degrees), areas which have extensive multi-wavelength coverage and are easily accessible from ALMA. Two thirds of the of the sources are expected to be at z > 1, one third at z > 2 and about a 1000 at z > 5. (b) Remove point source confusion in secondary anisotropy studies with Planck and ground-based CMB data. (c) Find at least 1200 strongly lensed bright sub-mm sources leading to a 2% test of general relativity. (d) Identify 200 proto-cluster regions at z of 2 and perform an unbiased study of the environmental dependence of star formation. (e) Perform an unbiased survey for star formation and dust at high Galactic latitude and make a census of debris disks and dust around AGB stars and white dwarfs.

45. The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Author: Cooray, Asantha, Eales, Steve, Chapman, Scott, Clements, David L., Dore, Olivier, Farrah, Duncan, Jarvis, Matt J., Kaplinghat, Manoj, Negrello, Mattia, Melchiorri, Alessandro, Peiris, Hiranya, Pope, Alexandra, Santos, Mario G., Serjeant, Stephen, Thompson, Mark, White, Glenn, Amblard, Alexandre, Banerji, Manda, Corasaniti, Pier-Stefano, Das, Sudeep, de Bernardis, Francesco, de Zotti, Gianfranco, Giannantonio, Tommaso, Gonzalez-Nuevo Gonzalez, Joaquin, Khostovan, Ali Ahmad, Mitchell-Wynne, Ketron, Serra, Paolo, Song, Yong-Seon, Vieira, Joaquin, Wang, Lingyu, Zemcov, Michael, Abdalla, Filipe, Afonso, Jose, Aghanim, Nabila, Andreani, Paola, Aretxaga, Itziar, Auld, Robbie, Baes, Maarten, Baker, Andrew, Barkats, Denis, Belen Barreiro, R., Bartolo, Nicola, Barton, Elizabeth, Barway, Sudhanshu, Stefano Battistelli, Elia, Baugh, Carlton, Beelen, Alexander, Benabed, Karim, Blain, Andrew, Bland-Hawthorn, Joss, Bock, James~J., Bond, J. Richard, Borrill, Julian, Borys, Colin, Boselli, Alessandro, Bouchet, Francois R., Bridge, Carrie, Brighenti, Fabrizio, Buat, Veronique, Buote, David, Burgarella, Denis, Bussmann, Robert, Calabrese, Erminia, Cantalupo, Christopher, Carlberg, Raymond, Sofia Carvalho, Carla, Casey, Caitlin, Cava, Antonio, Cepa, Jordi, Chapin, Edward, Chary, Ranga Ram, Chen, Xuelei, Colafrancesco, Sergio, Cole, Shaun, Coles, Peter, Conley, Alexander, Conversi, Luca, Cooke, Jeff, Crawford, Steven, Cress, Catherine, da Cunha, Elisabete, Dalton, Gavin, Danese, Luigi, Dannerbauer, Helmut, Davies, Jonathan, de Bernardis, Paolo, de Putter, Roland, Devlin, Mark, Diego, Jose M., Dole, Herve, Douspis, Marian, Dunkley, Joanna, Dunlop, James, Dunne, Loretta, Dunner, Rolando, Dye, Simon, Efstathiou, George, Egami, Eiichi, Fang, Taotao, Ferrero, Patrizia, Franceschini, Alberto, Frazer, Christopher C., Frayer, David, Frenk, Carlos, Ganga, Ken, Gavazzi, Raphael, Glenn, Jason, Gong, Yan, Gonzalez-Solares, Eduardo, Griffin, Matt, Guo, Qi, Gurwell, Mark, Hajian, Amir, Halpern, Mark, Hanson, Duncan, Hardcastle, Martin, Hatziminaoglou, Evanthia, Heavens, Alan, Heinis, Sebastien, Herranz, Diego, Hilton, Matt, Ho, Shirley, Holwerda, Benne W., Hopwood, Rosalind, Horner, Jonathan, Huffenberger, Kevin, Hughes, David H., Hughes, John P., Ibar, Edo, Ivison, Rob, Jackson, Neal, Jaffe, Andrew, Jenness, Timothy, Joncas, Gilles, Joudaki, Shahab, Kaviraj, Sugata, Kim, Sam, King, Lindsay, Kisner, Theodore, Knapen, Johan, Kniazev, Alexei, Komatsu, Eiichiro, Koopmans, Leon, Kuo, Chao-Lin, Lacey, Cedric, Lahav, Ofer, Lasenby, Anthony N., Lawrence, Andy, Lee, Myung Gyoon, Leeuw, Lerothodi L., Levenson, Louis R., Lewis, Geraint, Loaring, Nicola, Lopez-Caniego, Marcos, Maddox, Steve, Marriage, Tobias, Marsden, Gaelen, Martinez-Gonzalez, Enrique, Masi, Silvia, Matarrese, Sabino, Mathews, William G., Matsuura, Shuji, McMahon, Richard, Mellier, Yannick, Menanteau, Felipe, Michalowski, Michal~J., Millea, Marius, Mobasher, Bahram, Mohanty, Subhanjoy, Montier, Ludovic, Moodley, Kavilan, Moriarty-Schieven, Gerald H., Mortier, Angela, Munshi, Dipak, Murphy, Eric, Nandra, Kirpal, Natoli, Paolo, Nguyen, Hien, Oliver, Seb, Omont, Alain, Page, Lyman, Page, Mathew, Paladini, Roberta, Pandolfi, Stefania, Pascale, Enzo, Patanchon, Guillaume, Peacock, John, Pearson, Chris, Perez-Fournon, Ismael, Perez-Gonz, Pablo G., Piacentini, Francesco, Pierpaoli, Elena, Pohlen, Michael, Pointecouteau, Etienne, Polenta, Gianluca, Rawlings, Jason, Reese, Erik~D., Rigby, Emma, Rodighiero, Giulia, Romero-Colmenero, Encarni, Roseboom, Isaac, Rowan-Robinson, Michael, Sanchez-Portal, Miguel, Schmidt, Fabian, Schneider, Michael, Schulz, Bernhard, Scott, Douglas, Sedgwick, Chris, Sehgal, Neelima, Seymour, Nick, Sherwin, Blake~D., Short, Jo, Shupe, David, Sievers, Jonathan, Skibba, Ramin, Smidt, Joseph, Smith, Anthony, Smith, Daniel J. B., Smith, Matthew W. L., Spergel, David, Staggs, Suzanne, Stevens, Jason, Switzer, Eric, Takagi, Toshinobu, Takeuchi, Tsutomu, Temi, Pasquale, Trichas, Markos, Trigilio, Corrado, Tugwell, Katherine, Umana, Grazia, Vacca, William, Vaccari, Mattia, Vaisanen, Petri, Valtchanov, Ivan, van der Heyden, Kurt, van der Werf, Paul P., van Kampen, Eelco, van Waerbeke, Ludovic, Vegetti, Simona, Veneziani, Marcella, Verde, Licia, Verma, Aprajita, Vielva, Patricio, Viero, Marco P., Vila Vilaro, Baltasar, Wardlow, Julie, Wilson, Grant, Wright, Edward L., Xu, C. Kevin, Yun, Min S., Cooray, Asantha, Eales, Steve, Chapman, Scott, Clements, David L., Dore, Olivier, Farrah, Duncan, Jarvis, Matt J., Kaplinghat, Manoj, Negrello, Mattia, Melchiorri, Alessandro, Peiris, Hiranya, Pope, Alexandra, Santos, Mario G., Serjeant, Stephen, Thompson, Mark, White, Glenn, Amblard, Alexandre, Banerji, Manda, Corasaniti, Pier-Stefano, Das, Sudeep, de Bernardis, Francesco, de Zotti, Gianfranco, Giannantonio, Tommaso, Gonzalez-Nuevo Gonzalez, Joaquin, Khostovan, Ali Ahmad, Mitchell-Wynne, Ketron, Serra, Paolo, Song, Yong-Seon, Vieira, Joaquin, Wang, Lingyu, Zemcov, Michael, Abdalla, Filipe, Afonso, Jose, Aghanim, Nabila, Andreani, Paola, Aretxaga, Itziar, Auld, Robbie, Baes, Maarten, Baker, Andrew, Barkats, Denis, Belen Barreiro, R., Bartolo, Nicola, Barton, Elizabeth, Barway, Sudhanshu, Stefano Battistelli, Elia, Baugh, Carlton, Beelen, Alexander, Benabed, Karim, Blain, Andrew, Bland-Hawthorn, Joss, Bock, James~J., Bond, J. Richard, Borrill, Julian, Borys, Colin, Boselli, Alessandro, Bouchet, Francois R., Bridge, Carrie, Brighenti, Fabrizio, Buat, Veronique, Buote, David, Burgarella, Denis, Bussmann, Robert, Calabrese, Erminia, Cantalupo, Christopher, Carlberg, Raymond, Sofia Carvalho, Carla, Casey, Caitlin, Cava, Antonio, Cepa, Jordi, Chapin, Edward, Chary, Ranga Ram, Chen, Xuelei, Colafrancesco, Sergio, Cole, Shaun, Coles, Peter, Conley, Alexander, Conversi, Luca, Cooke, Jeff, Crawford, Steven, Cress, Catherine, da Cunha, Elisabete, Dalton, Gavin, Danese, Luigi, Dannerbauer, Helmut, Davies, Jonathan, de Bernardis, Paolo, de Putter, Roland, Devlin, Mark, Diego, Jose M., Dole, Herve, Douspis, Marian, Dunkley, Joanna, Dunlop, James, Dunne, Loretta, Dunner, Rolando, Dye, Simon, Efstathiou, George, Egami, Eiichi, Fang, Taotao, Ferrero, Patrizia, Franceschini, Alberto, Frazer, Christopher C., Frayer, David, Frenk, Carlos, Ganga, Ken, Gavazzi, Raphael, Glenn, Jason, Gong, Yan, Gonzalez-Solares, Eduardo, Griffin, Matt, Guo, Qi, Gurwell, Mark, Hajian, Amir, Halpern, Mark, Hanson, Duncan, Hardcastle, Martin, Hatziminaoglou, Evanthia, Heavens, Alan, Heinis, Sebastien, Herranz, Diego, Hilton, Matt, Ho, Shirley, Holwerda, Benne W., Hopwood, Rosalind, Horner, Jonathan, Huffenberger, Kevin, Hughes, David H., Hughes, John P., Ibar, Edo, Ivison, Rob, Jackson, Neal, Jaffe, Andrew, Jenness, Timothy, Joncas, Gilles, Joudaki, Shahab, Kaviraj, Sugata, Kim, Sam, King, Lindsay, Kisner, Theodore, Knapen, Johan, Kniazev, Alexei, Komatsu, Eiichiro, Koopmans, Leon, Kuo, Chao-Lin, Lacey, Cedric, Lahav, Ofer, Lasenby, Anthony N., Lawrence, Andy, Lee, Myung Gyoon, Leeuw, Lerothodi L., Levenson, Louis R., Lewis, Geraint, Loaring, Nicola, Lopez-Caniego, Marcos, Maddox, Steve, Marriage, Tobias, Marsden, Gaelen, Martinez-Gonzalez, Enrique, Masi, Silvia, Matarrese, Sabino, Mathews, William G., Matsuura, Shuji, McMahon, Richard, Mellier, Yannick, Menanteau, Felipe, Michalowski, Michal~J., Millea, Marius, Mobasher, Bahram, Mohanty, Subhanjoy, Montier, Ludovic, Moodley, Kavilan, Moriarty-Schieven, Gerald H., Mortier, Angela, Munshi, Dipak, Murphy, Eric, Nandra, Kirpal, Natoli, Paolo, Nguyen, Hien, Oliver, Seb, Omont, Alain, Page, Lyman, Page, Mathew, Paladini, Roberta, Pandolfi, Stefania, Pascale, Enzo, Patanchon, Guillaume, Peacock, John, Pearson, Chris, Perez-Fournon, Ismael, Perez-Gonz, Pablo G., Piacentini, Francesco, Pierpaoli, Elena, Pohlen, Michael, Pointecouteau, Etienne, Polenta, Gianluca, Rawlings, Jason, Reese, Erik~D., Rigby, Emma, Rodighiero, Giulia, Romero-Colmenero, Encarni, Roseboom, Isaac, Rowan-Robinson, Michael, Sanchez-Portal, Miguel, Schmidt, Fabian, Schneider, Michael, Schulz, Bernhard, Scott, Douglas, Sedgwick, Chris, Sehgal, Neelima, Seymour, Nick, Sherwin, Blake~D., Short, Jo, Shupe, David, Sievers, Jonathan, Skibba, Ramin, Smidt, Joseph, Smith, Anthony, Smith, Daniel J. B., Smith, Matthew W. L., Spergel, David, Staggs, Suzanne, Stevens, Jason, Switzer, Eric, Takagi, Toshinobu, Takeuchi, Tsutomu, Temi, Pasquale, Trichas, Markos, Trigilio, Corrado, Tugwell, Katherine, Umana, Grazia, Vacca, William, Vaccari, Mattia, Vaisanen, Petri, Valtchanov, Ivan, van der Heyden, Kurt, van der Werf, Paul P., van Kampen, Eelco, van Waerbeke, Ludovic, Vegetti, Simona, Veneziani, Marcella, Verde, Licia, Verma, Aprajita, Vielva, Patricio, Viero, Marco P., Vila Vilaro, Baltasar, Wardlow, Julie, Wilson, Grant, Wright, Edward L., Xu, C. Kevin, and Yun, Min S.
Abstract: A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwave background experiments. The Herschel-SPIRE Legacy Survey (HSLS), will lead to imaging data over 4000 sq. degrees at 250, 350, and 500 micron. Major Goals of HSLS are: (a) produce a catalog of 2.5 to 3 million galaxies down to 26, 27 and 33 mJy (50% completeness; 5 sigma confusion noise) at 250, 350 and 500 micron, respectively, in the southern hemisphere (3000 sq. degrees) and in an equatorial strip (1000 sq. degrees), areas which have extensive multi-wavelength coverage and are easily accessible from ALMA. Two thirds of the of the sources are expected to be at z > 1, one third at z > 2 and about a 1000 at z > 5. (b) Remove point source confusion in secondary anisotropy studies with Planck and ground-based CMB data. (c) Find at least 1200 strongly lensed bright sub-mm sources leading to a 2% test of general relativity. (d) Identify 200 proto-cluster regions at z of 2 and perform an unbiased study of the environmental dependence of star formation. (e) Perform an unbiased survey for star formation and dust at high Galactic latitude and make a census of debris disks and dust around AGB stars and white dwarfs.

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