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Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 04/2016, Volume 588, p. A61
Journal Article
Comptes rendus - Physique, ISSN 1631-0705, 2012, Volume 13, Issue 1, pp. 46 - 53
3D mapping of matter distribution in the Universe through the 21 cm radio emission of atomic hydrogen (H ) is a complementary approach to optical surveys for... 
Radio-interférométrie à 21 cm | Cosmology | Dark energy | Cosmologie | Énergie noire | 21 cm radio interferometry | PHYSICS, MULTIDISCIPLINARY | OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | Beams (radiation) | Measuring instruments | Digital | Mapping | Radio | Atomic structure | Interferometry | Three dimensional
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 2, p. 1950
  The spherical harmonics m-mode decomposition is a powerful sky map reconstruction method suitable for radio interferometers operating in transit mode. It can... 
Radio astronomy | Astrophysics | Star maps | Spectrum analysis | Milky Way | Star & galaxy formation | Interferometry
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 2, pp. 1950 - 1950
The spherical harmonics m-mode decomposition is a powerful sky map reconstruction method suitable for radio interferometers operating in transit mode. It can... 
Reconstruction | Bulging | Noise | Spherical harmonics | Symbols | Visibility | Arrays | Transit
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 2, pp. 1950 - 1966
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 03/2019, Volume 623, p. A76
Context. The Large Synoptic Survey Telescope (LSST) survey will image billions of galaxies every few nights for ten years, and as such, should be a major... 
OSCILLATION SPECTROSCOPIC SURVEY | DISTANCE | EVOLUTION | galaxies: distances and redshifts | ASTRONOMY & ASTROPHYSICS | large-scale structure of Universe | DARK ENERGY | BARYON ACOUSTIC-OSCILLATIONS | ULTRAVIOLET
Journal Article
天文和天体物理学研究:英文版, ISSN 1674-4527, 2016, Volume 16, Issue 10, pp. 71 - 80
We apply our sky map reconstruction method for transit type interferometers to the Tianlai cylin- der array. The method is based on spherical harmonic... 
map making | method: transit telescope | cosmology: observation | HI intensity mapping | ASTRONOMY & ASTROPHYSICS | Reconstruction | Gratings (spectra) | Beams (radiation) | Noise | Transfer functions | Arrays | Interferometers | Cylinders
Journal Article
08/2011
Large Scale Structures (LSS) in the universe can be traced using the neutral atomic hydrogen HI through its 21cm emission. Such a 3D matter distribution map... 
Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Annals of the New York Academy of Sciences, ISSN 0077-8923, 09/1995, Volume 759, Issue 1, pp. 664 - 667
Journal Article
SEVENTEENTH TEXAS SYMPOSIUM ON RELATIVISTIC ASTROPHYSICS AND COSMOLOGY, ISSN 0077-8923, 1995, Volume 759, Issue 1, pp. 664 - 667
Journal Article
02/2019
Imaging billions of galaxies every few nights during ten years, LSST should be a major contributor to precision cosmology in the 2020 decade. High precision... 
Physics - Cosmology and Nongalactic Astrophysics
Journal Article
by Schlegel, David J and Kollmeier, Juna A and Aldering, Greg and Bailey, Stephen and Baltay, Charles and Bebek, Christopher and BenZvi, Segev and Besuner, Robert and Blanc, Guillermo and Bolton, Adam S and Bouri, Mohamed and Brooks, David and Buckley-Geer, Elizabeth and Cai, Zheng and Crane, Jeffrey and Dey, Arjun and Doel, Peter and Fan, Xiaohui and Ferraro, Simone and Font-Ribera, Andreu and Gutierrez, Gaston and Guy, Julien and Heetderks, Henry and Huterer, Dragan and Infante, Leopoldo and Jelinsky, Patrick and Johns, Matthew and Karagiannis, Dionysios and Kent, Stephen M and Kim, Alex G and Kneib, Jean-Paul and Kronig, Luzius and Konidaris, Nick and Lahav, Ofer and Lampton, Michael L and Lang, Dustin and Leauthaud, Alexie and Liguori, Michele and Linder, Eric V and Magneville, Christophe and Martini, Paul and Mateo, Mario and McDonald, Patrick and Miller, Christopher J and Moustakas, John and Myers, Adam D and Mulchaey, John and Newman, Jeffrey A and Nugent, Peter E and Palanque-Delabrouille, Nathalie and Padmanabhan, Nikhil and Piro, Anthony L and Poppett, Claire and Prochaska, Jason X and Pullen, Anthony R and Rabinowitz, David and Ramirez, Solange and Rix, Hans-Walter and Ross, Ashley J and Samushia, Lado and Schaan, Emmanuel and Schubnell, Michael and Seljak, Uros and Seo, Hee-Jong and Shectman, Stephen A and Silber, Joseph and Simon, Joshua D and Slepian, Zachary and Soares-Santos, Marcelle and Tarle, Greg and Thompson, Ian and Valluri, Monica and Wechsler, Risa H and White, Martin and Wilson, Michael J and Yeche, Christophe and Zaritsky, Dennis
07/2019
MegaMapper is a proposed ground-based experiment to measure Inflation parameters and Dark Energy from galaxy redshifts at 2
Journal Article
by DESI Collaboration and Aghamousa, Amir and Aguilar, Jessica and Ahlen, Steve and Alam, Shadab and Allen, Lori E and Prieto, Carlos Allende and Annis, James and Bailey, Stephen and Balland, Christophe and Ballester, Otger and Baltay, Charles and Beaufore, Lucas and Bebek, Chris and Beers, Timothy C and Bell, Eric F and Bernal, José Luis and Besuner, Robert and Beutler, Florian and Blake, Chris and Bleuler, Hannes and Blomqvist, Michael and Blum, Robert and Bolton, Adam S and Briceno, Cesar and Brooks, David and Brownstein, Joel R and Buckley-Geer, Elizabeth and Burden, Angela and Burtin, Etienne and Busca, Nicolas G and Cahn, Robert N and Cai, Yan-Chuan and Cardiel-Sas, Laia and Carlberg, Raymond G and Carton, Pierre-Henri and Casas, Ricard and Castander, Francisco J and Cervantes-Cota, Jorge L and Claybaugh, Todd M and Close, Madeline and Coker, Carl T and Cole, Shaun and Comparat, Johan and Cooper, Andrew P and Cousinou, M. -C and Crocce, Martin and Cuby, Jean-Gabriel and Cunningham, Daniel P and Davis, Tamara M and Dawson, Kyle S and de la Macorra, Axel and De Vicente, Juan and Delubac, Timothée and Derwent, Mark and Dey, Arjun and Dhungana, Govinda and Ding, Zhejie and Doel, Peter and Duan, Yutong T and Ealet, Anne and Edelstein, Jerry and Eftekharzadeh, Sarah and Eisenstein, Daniel J and Elliott, Ann and Escoffier, Stéphanie and Evatt, Matthew and Fagrelius, Parker and Fan, Xiaohui and Fanning, Kevin and Farahi, Arya and Farihi, Jay and Favole, Ginevra and Feng, Yu and Fernandez, Enrique and Findlay, Joseph R and Finkbeiner, Douglas P and Fitzpatrick, Michael J and Flaugher, Brenna and Flender, Samuel and Font-Ribera, Andreu and Forero-Romero, Jaime E and Fosalba, Pablo and Frenk, Carlos S and Fumagalli, Michele and Gaensicke, Boris T and Gallo, Giuseppe and Garcia-Bellido, Juan and Gaztanaga, Enrique and Fusillo, Nicola Pietro Gentile and Gerard, Terry and Gershkovich, Irena and Giannantonio, Tommaso and Gillet, Denis and Gonzalez-de-Rivera, Guillermo and Gonzalez-Perez, Violeta and Gott, Shelby and Graur, Or and Gutierrez, Gaston and Guy, Julien and ...
10/2016
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth... 
Journal Article
by DESI Collaboration and Aghamousa, Amir and Aguilar, Jessica and Ahlen, Steve and Alam, Shadab and Allen, Lori E and Prieto, Carlos Allende and Annis, James and Bailey, Stephen and Balland, Christophe and Ballester, Otger and Baltay, Charles and Beaufore, Lucas and Bebek, Chris and Beers, Timothy C and Bell, Eric F and Bernal, José Luis and Besuner, Robert and Beutler, Florian and Blake, Chris and Bleuler, Hannes and Blomqvist, Michael and Blum, Robert and Bolton, Adam S and Briceno, Cesar and Brooks, David and Brownstein, Joel R and Buckley-Geer, Elizabeth and Burden, Angela and Burtin, Etienne and Busca, Nicolas G and Cahn, Robert N and Cai, Yan-Chuan and Cardiel-Sas, Laia and Carlberg, Raymond G and Carton, Pierre-Henri and Casas, Ricard and Castander, Francisco J and Cervantes-Cota, Jorge L and Claybaugh, Todd M and Close, Madeline and Coker, Carl T and Cole, Shaun and Comparat, Johan and Cooper, Andrew P and Cousinou, M. -C and Crocce, Martin and Cuby, Jean-Gabriel and Cunningham, Daniel P and Davis, Tamara M and Dawson, Kyle S and de la Macorra, Axel and De Vicente, Juan and Delubac, Timothée and Derwent, Mark and Dey, Arjun and Dhungana, Govinda and Ding, Zhejie and Doel, Peter and Duan, Yutong T and Ealet, Anne and Edelstein, Jerry and Eftekharzadeh, Sarah and Eisenstein, Daniel J and Elliott, Ann and Escoffier, Stéphanie and Evatt, Matthew and Fagrelius, Parker and Fan, Xiaohui and Fanning, Kevin and Farahi, Arya and Farihi, Jay and Favole, Ginevra and Feng, Yu and Fernandez, Enrique and Findlay, Joseph R and Finkbeiner, Douglas P and Fitzpatrick, Michael J and Flaugher, Brenna and Flender, Samuel and Font-Ribera, Andreu and Forero-Romero, Jaime E and Fosalba, Pablo and Frenk, Carlos S and Fumagalli, Michele and Gaensicke, Boris T and Gallo, Giuseppe and Garcia-Bellido, Juan and Gaztanaga, Enrique and Fusillo, Nicola Pietro Gentile and Gerard, Terry and Gershkovich, Irena and Giannantonio, Tommaso and Gillet, Denis and Gonzalez-de-Rivera, Guillermo and Gonzalez-Perez, Violeta and Gott, Shelby and Graur, Or and Gutierrez, Gaston and Guy, Julien and ...
10/2016
DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of... 
Journal Article
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