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1. 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

2. Discovery of a Giant Lya Emitter Near the Reionization Epoch

Author

Ouchi, Masami, Ono, Yoshiaki, Egami, Eiichi, Saito, Tomoki, Oguri, Masamune, McCarthy, Patrick J., Farrah, Duncan, Kashikawa, Nobunari, Momcheva, Ivelina, Shimasaku, Kazuhiro, Nakanishi, Kouichiro, Furusawa, Hisanori, Akiyama, Masayuki, Dunlop, James S., Mortier, Angela M. J., Okamura, Sadanori, Hayashi, Masao, Cirasuolo, Michele, Dressler, Alan, Iye, Masanori, Jarvis, Matt. J., Kodama, Tadayuki, Martin, Crystal L., McLure, Ross J., Ohta, Kouji, Yamada, Toru, and Yoshida, Michitoshi

Subjects
Astrophysics
Abstract

We report the discovery of a giant Lya emitter (LAE) with a Spitzer/IRAC counterpart near the reionization epoch at z=6.595. The giant LAE is found from the extensive 1 deg^2 Subaru narrow-band survey for z=6.6 LAEs in the Subaru/XMM-Newton Deep Survey (SXDS) field, and subsequently identified by deep spectroscopy of Keck/DEIMOS and Magellan/IMACS. Among our 207 LAE candidates, this LAE is not only the brightest narrow-band object with L(Lya) = 3.9+/-0.2 x 10^43 erg/s in our survey volume of 10^6 Mpc^3, but also a spatially extended Lya nebula with the largest isophotal area whose major axis is at least ~3''. This object is more likely to be a large Lya nebula with a size of >~17 kpc than to be a strongly-lensed galaxy by a foreground object. Our Keck spectrum with medium-high spectral and spatial resolutions suggests that the velocity width is v(FWHM)=251+/-21 km/s, and that the line-center velocity changes by ~60 km/s in a 10-kpc range. The stellar mass and star-formation rate are estimated to be 0.9-5.0 x 10^10 Mo and >34 Mo/yr, respectively, from the combination of deep optical to infrared images of Subaru, UKIDSS-Ultra Deep Survey, and Spitzer/IRAC. Although the nature of this object is not yet clearly understood, this could be an important object for studying cooling clouds accreting onto a massive halo, or forming-massive galaxies with significant outflows contributing to cosmic reionization and metal enrichment of inter-galactic medium., Comment: 13 pages, 9 figures, 2 tables. ApJ, in press

Published
2008
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3. The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- VI. 350 micron mapping of submillimetre galaxies

Author

Coppin, Kristen, Halpern, Mark, Scott, Douglas, Borys, Colin, Dunlop, James, Dunne, Loretta, Ivison, Rob, Wagg, Jeff, Aretxaga, Itziar, Battistelli, Elia, Benson, Andrew, Blain, Andrew, Chapman, Scott, Clements, Dave, Dye, Simon, Farrah, Duncan, Hughes, David, Jenness, Tim, van Kampen, Eelco, Lacey, Cedric, Mortier, Angela, Pope, Alexandra, Priddey, Robert, Serjeant, Stephen, Smail, Ian, Stevens, Jason, and Vaccari, Mattia

Subjects
Astrophysics
Abstract

A follow-up survey using the Submillimetre High-Angular Resolution Camera (SHARC-II) at 350 microns has been carried out to map the regions around several 850 micron-selected sources from the Submillimetre HAlf Degree Extragalactic Survey (SHADES). These observations probe the infrared luminosities and hence star-formation rates in the largest existing, most robust sample of submillimetre galaxies (SMGs). We measure 350 micron flux densities for 24 850 micron sources, seven of which are detected at >2.5-sigma within a 10 arcsec search radius of the 850 micron positions. When results from the literature are included the total number of 350 micron flux density constraints of SHADES SMGs is 31, with 15 detections. We fit a modified blackbody to the far-infrared (FIR) photometry of each SMG, and confirm that typical SMGs are dust-rich (Mdust~9x10^8 Msun), luminous (Lfir~2x10^12 Lsun), star-forming galaxies with intrinsic dust temperatures of ~35 K and star-formation rates of ~400 Msun/yr. We have measured the temperature distribution of SMGs and find that the underlying distribution is slightly broader than implied by the error bars, and that most SMGs are at 28 K with a few hotter. We also place new constraints on the 350 micron source counts, N350(>25mJy)~200-500 deg^-2., Comment: Accepted for publication in MNRAS Dec 04 2007: 15 pages; 8 figures. Details: correction of typo in 2 source coordinates in Table 2, minor wording changes, added reference, minor change to Fig. 6

Published
2007
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4. The SCUBA HAlf Degree Extragalactic Survey (SHADES) - IV: Radio-mm-FIR photometric redshifts

Author

Aretxaga, Itziar, Hughes, David H., Coppin, Kristen, Mortier, Angela M. J., Wagg, Jeff, Dunlop, James S., Chapin, Edward L., Eales, Stephen A., Gaztanaga, Enrique, Halpern, Mark, Ivison, Rob J., van Kampen, Eelco, Scott, Douglas, Serjeant, Stephen, Smail, Ian, Babbedge, Thomas, Benson, Andrew J., Chapman, Scott, Clements, David L., Dunne, Loretta, Dye, Simon, Farrah, Duncan, Jarvis, Matthew J., Mann, Robert G., Pope, Alexandra, Priddey, Robert, Rawlings, Steve, Seigar, Marc, Silva, Laura, Simpson, Chris, and Vaccari, Mattia

Subjects
Astrophysics
Abstract

We present the redshift distribution of the SHADES galaxy population based on the rest-frame radio-mm-FIR colours of 120 robustly detected 850um sources in the Lockman Hole East (LH) and Subaru XMM-Newton Deep Field (SXDF). The redshift distribution derived from the full SED information is shown to be narrower than that determined from the radio-submm spectral index, as more photometric bands contribute to a higher redshift accuracy. The redshift distribution of sources derived from at least two photometric bands peaks at z ~ 2.4 and has a near-Gaussian distribution, with 50 per cent (interquartile range) of sources at z=1.8-3.1. We find a statistically-significant difference between the measured redshift distributions in the two fields; the SXDF peaking at a slightly lower redshift (median z ~ 2.2) than the LH (median z ~ 2.7), which we attribute to the noise-properties of the radio observations. We demonstrate however that there could also be field-to-field variations that are consistent with the measured differences in the redshift distributions, and hence, that the incomplete area observed by SHADES with SCUBA, despite being the largest sub-mm survey to date, may still be too small to fully characterize the bright sub-mm galaxy population. Finally we present a brief comparison with the predicted, or assumed, redshift distributions of sub-mm galaxy formation and evolution models, and we derive the contribution of these SHADES sources and the general sub-mm galaxy population to the star formation-rate density at different epochs., Comment: MNRAS, accepted (22 pages, 9 figures, 5 tables). Revised version, minor modifications and 2 extra figures

Published
2007
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5. 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

6. A pilot study for the SCUBA-2 'All-Sky' survey

Author

Mackenzie, Todd, Braglia, Filiberto G., Gibb, Andy G., Scott, Douglas, Jenness, Tim, Serjeant, Stephen, Thompson, Mark A., Berry, David, Brunt, Christopher M., Chapin, Edward L., Chrysostomou, Antonio C., Clements, Dave, Coppin, Kristen, Economou, Frossie, Evans, A., Friberg, Per, Greaves, Jane, Hill, T., Holland, Wayne S., Ivison, R.J., Knapen, Johan H., Jackson, Neal, Joncas, Gilles, Morgan, Larry, Mortier, Angela M. J., Pearson, Chris P., Pestalozzi, Michele R., Pope, Alexandra, Richer, John, Urquhart, J.S., Vaccari, Mattia, Weferling, Bernd, White, Glenn J., Zhu, Ming, Mackenzie, Todd, Braglia, Filiberto G., Gibb, Andy G., Scott, Douglas, Jenness, Tim, Serjeant, Stephen, Thompson, Mark A., Berry, David, Brunt, Christopher M., Chapin, Edward L., Chrysostomou, Antonio C., Clements, Dave, Coppin, Kristen, Economou, Frossie, Evans, A., Friberg, Per, Greaves, Jane, Hill, T., Holland, Wayne S., Ivison, R.J., Knapen, Johan H., Jackson, Neal, Joncas, Gilles, Morgan, Larry, Mortier, Angela M. J., Pearson, Chris P., Pestalozzi, Michele R., Pope, Alexandra, Richer, John, Urquhart, J.S., Vaccari, Mattia, Weferling, Bernd, White, Glenn J., and Zhu, Ming

Published
2011

7. The SCUBA half degree extragalactic survey - IV. Radio-mm-FIR photometric redshifts

Author

Aretxaga, Itziar, Hughes, David H., Coppin, Kirsten, Mortier, Angela M. J., Wagg, Jeff, Dunlop, James S., Chapin, Edward L., Eales, Stephen A., Gaztanaga, Enrique, Halpern, Mark, Ivison, R.J., van Kampen, Eelco, Scott, Douglas, Serjeant, Stephen, Smail, Ian, Babbedge, Tom, Benson, Andrew J., Chapman, Scott, Clements, David L., Dunne, Loretta, Dye, Simon, Farrah, Duncan, Jarvis, Matt J., Mann, Robert G., Pope, Alexandra, Priddey, Robert, Rawlings, Steve, Seigar, Marc, Silva, Laura, Simpson, Chris, Vaccari, Mattia, Aretxaga, Itziar, Hughes, David H., Coppin, Kirsten, Mortier, Angela M. J., Wagg, Jeff, Dunlop, James S., Chapin, Edward L., Eales, Stephen A., Gaztanaga, Enrique, Halpern, Mark, Ivison, R.J., van Kampen, Eelco, Scott, Douglas, Serjeant, Stephen, Smail, Ian, Babbedge, Tom, Benson, Andrew J., Chapman, Scott, Clements, David L., Dunne, Loretta, Dye, Simon, Farrah, Duncan, Jarvis, Matt J., Mann, Robert G., Pope, Alexandra, Priddey, Robert, Rawlings, Steve, Seigar, Marc, Silva, Laura, Simpson, Chris, and Vaccari, Mattia

Abstract

We present the redshift distribution of the Submillimetre Common-User Bolometer Array (SCUBA) Half Degree Survey (SHADES) galaxy population based on the rest-frame radio mm-far-infrared(FIR) colours of 120 robustly detected 850 mu m sources in the Lockman Hole East (LH) and Subaru XMM-Newton Deep Field (SXDF). The redshift distribution derived from the full spectral energy distribution (SED) information is shown to be narrower than that determined from the radio-sub-mm spectral index, as more photometric bands contribute to a higher redshift accuracy. The redshift distribution of sources derived from at least two photometric bands peaks at z approximate to 2.4 and has a near-Gaussian distribution, with 50 per cent (interquartile range) of sources at z = 1.8-3.1. We find a statistically significant difference between the measured redshift distributions in the two fields; the SXDF peaking at a slightly lower redshift (median z approximate to 2.2) than the LH (median z approximate to 2.7), which we attribute to the noise properties of the radio observations. We demonstrate, however, that there could also be field-to-field variations that are consistent with the measured differences in the redshift distributions and, hence, that the incomplete area observed by SHADES with SCUBA, despite being the largest sub-mm survey to date, may still be too small to fully characterize the bright sub-mm galaxy population. Finally, we present a brief comparison with the predicted, or assumed, redshift distributions of sub-mm galaxy formation and evolution models, and we derive the contribution of these SHADES sources and the general sub-mm galaxy population to the star formation rate density at different epochs.

Published
2007

8. The SCUBA HAlf degree extragalactic survey (SHADES) - V. Submillimetre properties of near-infrared-selected galaxies in the Subaru/XMM-Newton deep field

Author

Takagi, Toshinobu, Mortier, Angela M. J., Shimasaku, K., Coppin, Kirsten, Pope, A., Ivison, R.J., Hanami, Hitoshi, Serjeant, Stephen, Clements, David L., Priddey, Robert, Dunlop, James S., Takata, T., Aretxaga, Itziar, Chapman, S.C., Eales, Stephen A., Farrah, Duncan, Granato, G.L., Halpern, Mark, Hughes, D.H., van Kampen, Eelco, Scott, D., Sekiguchi, K., Smail, Ian, Vaccari, Mattia, Takagi, Toshinobu, Mortier, Angela M. J., Shimasaku, K., Coppin, Kirsten, Pope, A., Ivison, R.J., Hanami, Hitoshi, Serjeant, Stephen, Clements, David L., Priddey, Robert, Dunlop, James S., Takata, T., Aretxaga, Itziar, Chapman, S.C., Eales, Stephen A., Farrah, Duncan, Granato, G.L., Halpern, Mark, Hughes, D.H., van Kampen, Eelco, Scott, D., Sekiguchi, K., Smail, Ian, and Vaccari, Mattia

Abstract

We have studied the submillimetre ( submm) properties of the following classes of near- infraredselected ( NIR- selected) massive galaxies at high redshifts: BzK- selected star- forming galaxies ( BzKs); distant red galaxies ( DRGs); and extremely red objects ( EROs). We used the SCUBA HAlf Degree Extragalactic Survey ( SHADES), the largest uniform submm survey to date. Partial overlap of SIRIUS/ NIR images and SHADES in Subaru/ XMM - Newton deep field has allowed us to identify four submm- bright NIR- selected galaxies, which are detected in the mid- IR, 24 m, and the radio, 1.4 GHz. We find that all of our submm- bright NIR- selected galaxies satisfy the BzK selection criteria, i. e. BzK = ( z - K) AB - ( B - z) AB >= - 0.2, except for one galaxy whose B - z and z - K colours are however close to the BzK colour boundary. Two of the submm- bright NIR- selected galaxies satisfy all of the selection criteria we considered, i. e. they belong to the BzK - DRG - ERO overlapping population, or ` extremely red' BzKs. Although these extremely red BzKs are rare ( 0.25 arcmin(-2)), up to 20 per cent of this population could be submm galaxies. This fraction is significantly higher than that found for other galaxy populations studied here. Via a stacking analysis, we have detected the 850- mu m flux of submm- faint BzKs and EROs in our SCUBAmaps. While the contribution of z similar to 2 BzKs to the submm background is about 10 - 15 per cent and similar to that from EROs typically at z similar to 1, BzKs have a higher fraction (similar to 30 per cent) of submm flux in resolved sources compared with EROs and submm sources as a whole. From the spectral energy distribution ( SED) fitting analysis for both submm- bright and submm- faint BzKs, we found no clear signature that submm- bright BzKs are experiencing a specifically luminous evolutionary phase, compared with submm- faint BzKs. An alternative explanation might be that submm- bright BzKs are more massive than submm- faint on

Published
2007

9. A pilot study for the SCUBA-2 ‘All-Sky’ Survey

Author

Mackenzie, Todd, primary, Braglia, Filiberto G., additional, Gibb, Andy G., additional, Scott, Douglas, additional, Jenness, Tim, additional, Serjeant, Stephen, additional, Thompson, Mark, additional, Berry, David, additional, Brunt, Christopher M., additional, Chapin, Edward, additional, Chrysostomou, Antonio, additional, Clements, Dave, additional, Coppin, Kristen, additional, Economou, Frossie, additional, Evans, A., additional, Friberg, Per, additional, Greaves, Jane, additional, Hill, T., additional, Holland, Wayne, additional, Ivison, R. J., additional, Knapen, Johan H., additional, Jackson, Neal, additional, Joncas, Gilles, additional, Morgan, Larry, additional, Mortier, Angela, additional, Pearson, Chris, additional, Pestalozzi, Michele, additional, Pope, Alexandra, additional, Richer, John, additional, Urquhart, J. S., additional, Vaccari, Mattia, additional, Weferling, Bernd, additional, White, Glenn, additional, and Zhu, Ming, additional

Published
2011
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10. DISCOVERY OF A GIANT Lyα EMITTER NEAR THE REIONIZATION EPOCH

Author

Ouchi, Masami, primary, Ono, Yoshiaki, additional, Egami, Eiichi, additional, Saito, Tomoki, additional, Oguri, Masamune, additional, McCarthy, Patrick J., additional, Farrah, Duncan, additional, Kashikawa, Nobunari, additional, Momcheva, Ivelina, additional, Shimasaku, Kazuhiro, additional, Nakanishi, Kouichiro, additional, Furusawa, Hisanori, additional, Akiyama, Masayuki, additional, Dunlop, James S., additional, Mortier, Angela M. J., additional, Okamura, Sadanori, additional, Hayashi, Masao, additional, Cirasuolo, Michele, additional, Dressler, Alan, additional, Iye, Masanori, additional, Jarvis, Matt J., additional, Kodama, Tadayuki, additional, Martin, Crystal L., additional, McLure, Ross J., additional, Ohta, Kouji, additional, Yamada, Toru, additional, and Yoshida, Michitoshi, additional

Published
2009
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11. The SCUBA HAlf Degree Extragalactic Survey – VI. 350-μm mapping of submillimetre galaxies

Author

Coppin, Kristen, primary, Halpern, Mark, additional, Scott, Douglas, additional, Borys, Colin, additional, Dunlop, James, additional, Dunne, Loretta, additional, Ivison, Rob, additional, Wagg, Jeff, additional, Aretxaga, Itziar, additional, Battistelli, Elia, additional, Benson, Andrew, additional, Blain, Andrew, additional, Chapman, Scott, additional, Clements, Dave, additional, Dye, Simon, additional, Farrah, Duncan, additional, Hughes, David, additional, Jenness, Tim, additional, van Kampen, Eelco, additional, Lacey, Cedric, additional, Mortier, Angela, additional, Pope, Alexandra, additional, Priddey, Robert, additional, Serjeant, Stephen, additional, Smail, Ian, additional, Stevens, Jason, additional, and Vaccari, Mattia, additional

Published
2008
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12. The Herschel ATLAS: A Large Area Extragalactic Survey with Herschel

Author

Clements, David, Robotham, Aaron, Omont, Alain, Lapi, Andrea, Papageorgiou, Andreas, Lawrence, Andy, Evans, Aneurin, Sanson, Anne, Cooray, Asantha, Edge, Alastair, Boselli, Alessandro, Beelen, Alexandre, Dariush, Ali, Amblard, Alexandre, Mortier, Angela, Cava, Antonio, Verma, Aprajita, Bain, Andrew, Schulz, Bernhard, Sibthorpe, Bruce, Chapman, Bob, Bridge, Carrie, Baugh, Carlton, Pearson, Chris, Sedgwick, Chris, Frenk, Carlos, Vlahakis, Cat, Lacey, Cedric, Popescu, Christina, Frayer, David, Hill, David, Smith, Daniel, Hughes, Dave, Bonfield, David, Burgarella, Denis, Rigopoulou, Dimitra, Benford, Dominic, Scott, Douglas, Farrah, Duncan, Ibar, Eduardo, Barton, Elizabeth, Kampen, Dimitra, Rigby, Emma, Gonzales-Solares, Eduardo, Hatziminaoglou, Evanthia, Bertoldi, Frank, Bendo, George, White, Glenn, Dalton, Gavin, Zotti, Gianfranco, Rodighiero, Giulia, Lagache, Guilaine, Patancon, Guillaume, Gomez, Haley, Dannerbauer, Helmut, Dole, Herve, Browne, Ian, Smail, Ian, Perez-Fournon, Ismael, Aretxaga, Itziar, Valtchanov, Ivan, Ftitz, Jacopo, Bock, James, Virdee, Jasmeer, Stevens, Jason, Geach, Jim, Gonzalez-Nuevo, Joaquin, Liske, Jochen, Peacock, John, Tedds, Jonathan, Puget, Jean-Loup, Woong-Seob, Jeong, Davies, Jon, Gardner, Jonathan, Dunlop, Jim, Xu, Kevin, Nandra, Kirpal, Leeuw, Lerothodi, Dunne, Loretta, Cortese, Luca, Danese, Luigi, Fan, Lulu, Thompson, Mark, Bremer, Malcolm, Hardcastle, Martin, Jarvis, Matt, Negrello, Mattia, Rowan-Robinson, Michael, Schneider, Michael, Michalowski, Michal, Lopez-Caniego, Marcos, Trichas, Marcos, Maarten Baes, Birkinshaw, Mark, Vaccari, Mattia, Gyoon Lee, Myung, Pohlen, Michael, Page, Matt, Kouichiro, Nakaniski, Christopher, Natalie, Castro Rodriguez, Nieves, Almaini, Omar, Andreani, Paolo, Serra, Paolo, Panuzzo, Pasquale, Temi, Pasquale, Werf, Paul, Coles, Peter, Mauskopf, Phil, Chanial, Pierre, Carlberg, Ray, Mann, Robert, Tuffs, Richard, Ivison, Rob, Auld, Robbie, Buttiglione, Sara, Samui, Saumyadip, Jester, Sebastian, Cole, Shaun, Driver, Simon, Dye, Simon, Pak, Soojong, Serjeant, Stephen, Flynn, Stephen, Phillips, Steve, Rawlings, Steve, Eales, Steve, Maddox, Steve, Mohanty, Subhanjoy, Nakagawa, Takao, Jenness, Tim, Mauch, Tom, Takagi, Toshi, Takeuchi, Tsutomu, Muller, Thomas, Buat, Veronique, Gear, Walter, and Sutherland, Will

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-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.

14. 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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