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

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.

Itziar Aretxaga | Marco P. Viero | Julian Borrill | Andrew Jaffe | Enzo Pascale | Etienne Pointecouteau | Douglas Scott | Anthony N. Lasenby | Eduardo Gonzalez-Solares | Gavin Dalton | David H. Hughes | Manda Banerji | Sugata Kaviraj | Qi Guo | Grant Wilson | Jordi Cepa | Edward Chapin | Yannick Mellier | Denis Burgarella | Silvia Masi | Neal Jackson | Asantha Cooray | Hien Nguyen | Felipe Menanteau | Kirpal Nandra | Alexandra Pope | Shuji Matsuura | J. Richard Bond | Mark Halpern | Yan Gong | John P. Hughes | Shaun Cole | Alexandre Amblard | Fabrizio Brighenti | Jeff Cooke | Shahab Joudaki | Toshinobu Takagi | Edward L. Wright | Shirley Ho | Elena Pierpaoli | Joaquin Vieira | Patricio Vielva | Yong-Seon Song | Paolo de Bernardis | Luca Conversi | Diego Herranz | Paolo Serra | Joss Bland-Hawthorn | Rob Ivison | Ivan Valtchanov | Francesco Piacentini | Denis Barkats | Gaelen Marsden | Enrique Martinez-Gonzalez | Jason Glenn | Paola Andreani | Nabila Aghanim | Maarten Baes | Duncan Farrah | David Shupe | Gilles Joncas | Veronique Buat | Bahram Mobasher | Geraint Lewis | Ismael Perez-Fournon | Lyman Page | Nick Seymour | Matt J. Jarvis | Michael Pohlen | Markos Trichas | Stephen Serjeant | Ofer Lahav | Matt Griffin | Karim Benabed | Stefania Pandolfi | Xuelei Chen | Marius Millea | Ramin Skibba | Lingyu Wang | Loretta Dunne | Simon Dye | Angela Mortier | Mattia Vaccari | Tobias Marriage | Chris Pearson | Michael Zemcov | Michael Rowan-Robinson | Andrew Blain | Petri Vaisanen | David Spergel | Isaac Roseboom | Amir Hajian | Carla Sofia Carvalho | Encarni Romero-Colmenero | Subhanjoy Mohanty | Grazia Umana | David Frayer | Eiichiro Komatsu | Mathew Page | Nicola Loaring | Kevin Huffenberger | Marcos Lopez-Caniego | Chao-Lin Kuo | Filipe Abdalla | Guillaume Patanchon | Mark Devlin | Eiichi Egami | Gianluca Polenta | George Efstathiou | Alessandro Melchiorri | Caitlin Casey | Kavilan Moodley | Neelima Sehgal | John Peacock | David Buote | Corrado Trigilio | Benne W. Holwerda | Jonathan Horner | Evanthia Hatziminaoglou | Glenn White | Carrie Bridge | Simona Vegetti | Matt Hilton | Alain Omont | Paolo Natoli | Julie Wardlow | William Vacca | Mario G. Santos | Suzanne Staggs | Rolando Dunner | Pasquale Temi | Carlton Baugh | Alan Heavens | Dipak Munshi | Taotao Fang | Manoj Kaplinghat | Sergio Colafrancesco | Leon Koopmans | Jose M. Diego | Antonio Cava | Johan Knapen | Rosalind Hopwood | Steven Crawford | Jose Afonso | Erminia Calabrese | Mattia Negrello | Marcella Veneziani | Seb Oliver | Daniel J. B. Smith | Myung Gyoon Lee | Matthew W. L. Smith | Joanna Dunkley | Licia Verde | Min S. Yun | Alessandro Boselli | Scott Chapman | Andy Lawrence | Elisabete da Cunha | Nicola Bartolo | Roland de Putter | James Dunlop | Sabino Matarrese | Colin Borys | Gerald H. Moriarty-Schieven | Olivier Dore | Eric Murphy | Eric Switzer | Patrizia Ferrero | Mark Gurwell | Tommaso Giannantonio | Paul P. van der Werf | Sudeep Das | Alberto Franceschini | Luigi Danese | Helmut Dannerbauer | Ken Ganga | Hiranya Peiris | Herve Dole | Pier-Stefano Corasaniti | Steve Eales | Kurt van der Heyden | Jonathan Sievers | Mark Thompson | Sam Kim | Raphael Gavazzi | Ranga Ram Chary | Bernhard Schulz | David L. Clements | Lindsay King | Theodore Kisner | R. Belen Barreiro | Raymond Carlberg | Peter Coles | Louis R. Levenson | Cedric Lacey | William G. Mathews | Roberta Paladini | Edo Ibar | Steve Maddox | Richard McMahon | Carlos Frenk | Giulia Rodighiero | Christopher Cantalupo | Michael Schneider | Aprajita Verma | Jonathan Davies | Sudhanshu Barway | Joseph Smidt | Duncan Hanson | Ali Ahmad Khostovan | Christopher C. Frazer | Marian Douspis | Alexei Kniazev | Jason Stevens | Baltasar Vila Vilaro | Francesco deBernardis | Gianfranco deZotti | Joaquin Gonzalez-Nuevo Gonzalez | Ketron Mitchell-Wynne | Robbie Auld | Andrew Baker | Elizabeth Barton | Elia Stefano Battistelli | Alexander Beelen | JamesJ. Bock | Francois R. Bouchet | Robert Bussmann | Alexander Conley | Catherine Cress | Martin Hardcastle | Sebastien Heinis | Timothy Jenness | Lerothodi L. Leeuw | MichalJ. Michalowski | Ludovic Montier | Pablo G. Perez-Gonz | Jason Rawlings | ErikD. Reese | Emma Rigby | Miguel Sanchez-Portal | Fabian Schmidt | Chris Sedgwick | BlakeD. Sherwin | Jo Short | Anthony Smith | Tsutomu Takeuchi | Katherine Tugwell | Eelco vanKampen | Ludovic vanWaerbeke | C. Kevin Xu

[1]  Peter Schneider,et al.  Gravitational Lensing: Strong, Weak and Micro , 2006 .

[2]  Max Tegmark Measuring Cosmological Parameters with Galaxy Surveys , 1997, astro-ph/9706198.

[3]  S. White,et al.  A Universal Density Profile from Hierarchical Clustering , 1996, astro-ph/9611107.

[4]  J. Frieman,et al.  Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey , 2004, astro-ph/0408003.

[5]  M. Sauvage,et al.  Clouds, filaments, and protostars: TheHerschel Hi-GAL Milky Way , 2010, 1005.3317.

[6]  L. Verde,et al.  Large scale structure, the cosmic microwave background, and primordial non-gaussianity , 1999, astro-ph/9906301.

[7]  L. Moscardini,et al.  The potential of X-ray cluster surveys to constrain primordial non-Gaussianity , 2010, 1003.0841.

[8]  M. Heidelberg,et al.  The infrared luminosity of galaxy clusters , 2008, 0808.2404.

[9]  R. Chary,et al.  SEARCHING FOR THE HIGHEST REDSHIFT SOURCES IN 250–500 μm SUBMILLIMETER SURVEYS , 2010, 1005.0386.

[10]  Sarah Bridle,et al.  Cosmology with photometric redshift surveys , 2004 .

[11]  Alexandre Amblard,et al.  Anisotropy Studies of the Unresolved Far-Infrared Background , 2007, astro-ph/0703592.

[12]  M. Halpern,et al.  ACTPol: a polarization-sensitive receiver for the Atacama Cosmology Telescope , 2010, Astronomical Telescopes + Instrumentation.

[13]  J. Mohr,et al.  Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys , 2000, astro-ph/0002336.

[14]  R. Nichol,et al.  Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies , 2005, astro-ph/0501171.

[15]  Edwin Sirko,et al.  Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak , 2007 .

[16]  Herschel-ATLAS: blazars in the SDP field , 2010, 1005.2407.

[17]  F. Mannucci,et al.  The extinction law at high redshift and its implications , 2010, 1006.4463.

[18]  Forecasting cosmic parameter errors from microwave background anisotropy experiments , 1997, astro-ph/9702100.

[19]  N. Ross,et al.  The C iv linewidth distribution for quasars and its implications for broad-line region dynamics and virial mass estimation , 2010, 1005.5287.

[20]  R. Nichol,et al.  Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS , 2007, 0705.3323.

[21]  Weak lensing of the CMB: extraction of lensing information from the trispectrum , 2002, astro-ph/0204068.

[22]  R. Sheth,et al.  An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier , 2001, astro-ph/0105113.

[23]  David N. Spergel,et al.  Acoustic signatures in the primary microwave background bispectrum , 2000, astro-ph/0005036.

[24]  J. Silk,et al.  Probability of the most massive cluster under non-Gaussian initial conditions , 2010, 1006.1950.

[25]  R. Thacker,et al.  On the Spatial Correlations of Lyman Break Galaxies , 2003, astro-ph/0305342.

[26]  M.Vaccari,et al.  Herschel unveils a puzzling uniformity of distant dusty galaxies , 2010, 1005.2859.

[27]  S. Maddox,et al.  Herschel ATLAS: The cosmic star formation history of quasar host galaxies , 2010, 1005.2410.

[28]  Lloyd Knox,et al.  Correlations in the Far-Infrared Background , 1999, astro-ph/9906399.

[29]  Princeton University,et al.  Probing Early Structure Formation with Far-Infrared Background Correlations , 2000, astro-ph/0009151.

[30]  K. Coppin,et al.  Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3 , 2010, 1005.1071.

[31]  Ravi Sheth,et al.  Halo Models of Large Scale Structure , 2002, astro-ph/0206508.

[32]  Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies , 2004, astro-ph/0408564.

[33]  A. Melchiorri,et al.  Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys , 2010, 1004.5467.

[34]  Andrew J. Connolly,et al.  Measuring the Matter Density Using Baryon Oscillations in the SDSS , 2006, astro-ph/0608635.

[35]  J. Peacock,et al.  Halo occupation numbers and galaxy bias , 2000, astro-ph/0005010.

[36]  M. Donahue,et al.  Herschel photometry of brightest cluster galaxies in cooling flow clusters , 2010, 1005.1211.

[37]  Edward J. Wollack,et al.  FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE * OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.

[38]  A. W. Blain,et al.  A vigorous starburst in the SCUBA galaxy N2 850.4 , 2003, astro-ph/0303128.

[39]  Abhirup Datta,et al.  BRIGHT SOURCE SUBTRACTION REQUIREMENTS FOR REDSHIFTED 21 cm MEASUREMENTS , 2010 .

[40]  Garching,et al.  The LOFAR EoR Data Model: (I) Effects of Noise and Instrumental Corruptions on the 21-cm Reionization Signal-Extraction Strategy , 2009, 0901.3359.

[41]  Shirley Ho,et al.  Finding the Missing Baryons Using CMB as a Backlight , 2009 .

[42]  J. Valle,et al.  Status of global fits to neutrino oscillations , 2004, hep-ph/0405172.

[43]  B. Garilli,et al.  Mid- and far-infrared luminosity functions and galaxy evolution from multiwavelength Spitzer observations up to z ~ 2.5 , 2009, 0910.5649.

[44]  D. Elbaz,et al.  HerMES: The SPIRE confusion limit , 2010, 1005.2207.

[45]  P. A. R. Ade,et al.  ANGULAR POWER SPECTRA OF THE MILLIMETER-WAVELENGTH BACKGROUND LIGHT FROM DUSTY STAR-FORMING GALAXIES WITH THE SOUTH POLE TELESCOPE , 2009, 0912.4315.

[46]  Klaus Dolag,et al.  Non-Gaussian halo assembly bias , 2010, 1004.1637.

[47]  J. Kneib,et al.  First detection of the Sunyaev Zel'dovich effect increment at λ < 650 μm , 2010, 1005.3824.

[48]  D. Eisenstein,et al.  Non-linear Structure Formation and the Acoustic Scale , 2022 .

[49]  R. Chary,et al.  New Observational Constraints and Modeling of the Infrared Background: Dust Obscured Star-Formation at z>1 and Dust in the Outer Solar System , 2010, 1003.1731.

[50]  M. Franx,et al.  ULTRAVIOLET LUMINOSITY FUNCTIONS FROM 132 z ∼ 7 AND z ∼ 8 LYMAN-BREAK GALAXIES IN THE ULTRA-DEEP HUDF09 AND WIDE-AREA EARLY RELEASE SCIENCE WFC3/IR OBSERVATIONS , 2010, 1006.4360.

[51]  X.Chen,et al.  Non-Gaussianity as a probe of the physics of the primordial universe and the astrophysics of the low redshift universe , 2009, 0902.4759.

[52]  S. Maddox,et al.  A search for debris disks in the Herschel-ATLAS , 2010, 1005.3018.

[53]  M. Halpern,et al.  Breaking the ‘redshift deadlock’– I. Constraining the star formation history of galaxies with submillimetre photometric redshifts , 2001, astro-ph/0111547.

[54]  M. Birkinshaw,et al.  The Sunyaev-Zel’dovich Effect , 1998, astro-ph/9808050.

[55]  P. A. R. Ade,et al.  THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE 600 < ℓ < 8000 COSMIC MICROWAVE BACKGROUND POWER SPECTRUM AT 148 GHz , 2010, 1001.2934.

[56]  Ravi K. Sheth Giuseppe Tormen Large scale bias and the peak background split , 1999 .

[57]  D. Elbaz,et al.  HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm , 2010, 1005.2184.

[58]  G. Gavazzi,et al.  The Herschel Virgo Cluster Survey , 2017 .

[59]  M. Halpern,et al.  A study of the Sunyaev–Zel'dovich increment using archival SCUBA data , 2006, astro-ph/0612708.

[60]  Pair correlations and merger bias , 2005, astro-ph/0507650.

[61]  R. Emery,et al.  The physical properties of the dust in the RCW 120 HII region as seen by Herschel , 2010, 1005.1565.

[62]  Wayne Hu,et al.  Cosmic microwave background lensing reconstruction on the full sky , 2003 .

[63]  D. Huterer,et al.  Imprints of primordial non-Gaussianities on large-scale structure: Scale-dependent bias and abundance of virialized objects , 2007, 0710.4560.

[64]  B. Reipurth Handbook of Star Forming Regions, Volume I: The Northern Sky , 2008 .

[65]  A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope , 2006, astro-ph/0611409.

[66]  G. W. Pratt,et al.  The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y-SZ-M-500 relation , 2009, 0910.1234.

[67]  Hee-Jong SeoDaniel J. Eisenstein Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys , 2003 .

[68]  Edinburgh,et al.  The LABOCA survey of the Extended Chandra Deep Field South: A photometric redshift survey of submillimetre galaxies , 2010, 1006.2137.

[69]  Early dark energy cosmologies , 2006, astro-ph/0601544.

[70]  I. Ribas,et al.  Cold DUst around NEarby Stars (DUNES). First results A resolved exo-Kuiper belt around the solar-like star zeta(2) Ret , 2010, 1005.3151.

[71]  Christopher Hirata,et al.  Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group , 2009, 0901.0721.

[72]  P. A. R. Ade,et al.  SPT-CL J0546-5345: A MASSIVE z>1 GALAXY CLUSTER SELECTED VIA THE SUNYAEV–ZEL'DOVICH EFFECT WITH THE SOUTH POLE TELESCOPE , 2010, 1006.5639.

[73]  S. Bhatnagar,et al.  DETECTION OF SIGNALS FROM COSMIC REIONIZATION USING RADIO INTERFEROMETRIC SIGNAL PROCESSING , 2009, 0908.2639.

[74]  D. Eisenstein,et al.  Improved Forecasts for the Baryon Acoustic Oscillations and Cosmological Distance Scale , 2007, astro-ph/0701079.

[75]  F. Schmidt Cosmological Simulations of Normal-Branch Braneworld Gravity , 2009, 0910.0235.

[76]  P. A. R. Ade,et al.  MEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE , 2009, 0912.4317.

[77]  M. Zaldarriaga,et al.  Probing primordial non-Gaussianity with large - scale structure , 2003, astro-ph/0312286.

[78]  A. Bolton,et al.  Detection of a dark substructure through gravitational imaging , 2009, 0910.0760.

[79]  Edinburgh,et al.  Breaking the ‘redshift deadlock’– II. The redshift distribution for the submillimetre population of galaxies , 2002, astro-ph/0205313.

[80]  N. Slavnov Integral operators with the generalized sine kernel on the real axis , 2010, 1005.5047.

[81]  Y. P. Jing,et al.  The Correlation function of clusters of galaxies and the amplitude of mass fluctuations in the Universe , 1996 .

[82]  L. Verde,et al.  The Effect of Primordial Non-Gaussianity on Halo Bias , 2008, 0801.4826.

[83]  L. Verde,et al.  The Abundance of High-Redshift Objects as a Probe of Non-Gaussian Initial Conditions , 2000, astro-ph/0001366.

[84]  Olivier Boulade,et al.  DUNE: the Dark Universe Explorer , 2006, SPIE Astronomical Telescopes + Instrumentation.

[85]  A. Cimatti,et al.  The far-infrared/radio correlation as probed by Herschel , 2010, 1005.1072.