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1. Full Text Lyman-alpha forests cool warm dark matter
by Baur, Julien and Palanque-Delabrouille, Nathalie and Yèche, Christophe and Magneville, Christophe and Viel, Matteo
Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, 08/2016, Volume 2016, Issue 8, pp. 12 - 12
The free-streaming of keV-scale particles impacts structure growth on scales that are probed by the Lyman-alpha forest of distant quasars. Using an... 
neutrino masses from cosmology | dark matter simulations | Lyman alpha forest | THERMAL HISTORY | SCALE STRUCTURE | OSCILLATION SPECTROSCOPIC SURVEY | POWER SPECTRUM | ASTRONOMY & ASTROPHYSICS | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | STERILE NEUTRINOS | GALAXIES | MILKY-WAY | DATA RELEASE | PHYSICS, PARTICLES & FIELDS | Physics - Cosmology and Nongalactic Astrophysics | RED SHIFT | RESOLUTION | KEV RANGE | SIMULATION | LYMAN LINES | NONLUMINOUS MATTER | QUASARS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NONLINEAR PROBLEMS | GRAVITINOS | RELICT RADIATION | SPECTRA
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2. Full Text Neutrino masses and cosmology with Lyman-alpha forest power spectrum
by Palanque-Delabrouille, Nathalie and Yèche, Christophe and Baur, Julien and Magneville, Christophe and Rossi, Graziano and Lesgourgues, Julien and Borde, Arnaud and Burtin, Etienne and Legoff, Jean-Marc and Rich, James and Viel, Matteo and Weinberg, David
Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, 11/2015, Volume 2015, Issue 11, pp. 11 - 11
We present constraints on neutrino masses, the primordial fluctuation spectrum from inflation, and other parameters of the ACDM model, using the... 
neutrino masses from cosmology | cosmological parameters from LSS | Lyman alpha forest | OSCILLATION SPECTROSCOPIC SURVEY | ASTRONOMY & ASTROPHYSICS | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | GALAXIES | DATA RELEASE | ANISOTROPY | UNIVERSE | PHYSICS, PARTICLES & FIELDS | Physics - Cosmology and Nongalactic Astrophysics | TENSORS | COSMOLOGICAL CONSTANT | LIMITING VALUES | RESOLUTION | EV RANGE | CORRELATIONS | INFLATIONARY UNIVERSE | PROBES | COSMOLOGY | EVOLUTION | MICROWAVE RADIATION | NONLUMINOUS MATTER | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | FLUCTUATIONS | SCALARS | COSMOLOGICAL INFLATION | NEUTRINOS | OSCILLATIONS | BARYONS
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3. Full Text Quasar host environments: The view from Planck
by Verdier, Loïc and Melin, Jean-Baptiste and Bartlett, James G and Magneville, Christophe and Palanque-Delabrouille, Nathalie and Yèche, Christophe
Astronomy and Astrophysics, ISSN 0004-6361, 04/2016, Volume 588
We measure the far-infrared emission of the general quasar (QSO) population using Planck observations of the Baryon Oscillation Spectroscopic Survey QSO... 
Galaxies: clusters: general | Methods: data analysis | Cosmology: observations | Methods: statistical | Large-scale structure of Universe | Quasars: general | MM MAMBO/IRAM-30 M | quasars: general | galaxies: clusters: general | methods: data analysis | HIGH-REDSHIFT QUASARS | large-scale structure of Universe | STAR-FORMATION | LUMINOSITY FUNCTION | SUPERMASSIVE BLACK-HOLES | OSCILLATION SPECTROSCOPIC SURVEY | methods: statistical | ACTIVE GALACTIC NUCLEI | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | BARYON ACOUSTIC-OSCILLATIONS | cosmology: observations | SDSS-III | Quasars | Red shift | Dust | Halos | Emission spectroscopy | Synchrotrons | Emission | Sunyaev-Zeldovich effect | Physics - Cosmology and Nongalactic Astrophysics
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4. Full Text Quasar host environments: The view fromPlanck
by Verdier, Loïc and Melin, Jean-Baptiste and Bartlett, James G and Magneville, Christophe and Palanque-Delabrouille, Nathalie and Yèche, Christophe
Astronomy & Astrophysics, ISSN 0004-6361, 04/2016, Volume 588, p. A61
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5. Full Text BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures
by Ansari, Réza and Campagne, Jean-Eric and Colom, Pierre and Magneville, Christophe and Martin, Jean-Michel and Moniez, Marc and Rich, James and Yèche, Christophe
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
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6. Sky reconstruction from transit visibilities: PAON-4 and Tianlai dish array
by Jiao Zhang and Reza Ansari and Xuelei Chen and Jean-Eric Campagne and Christophe Magneville and Fengquan Wu
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
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7. Sky reconstruction from transit visibilities: PAON-4 and Tianlai dish array
by Zhang, Jiao and Ansari, Reza and Chen, Xuelei and Campagne, Jean-Eric and Magneville, Christophe and Wu, Fengquan
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
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8. Full Text Sky reconstruction from transit visibilities: PAON-4 and Tianlai dish array
by Zhang, Jiao and Ansari, Reza and Chen, Xuelei and Campagne, Jean-Eric and Magneville, Christophe and Wu, Fengquan
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 2, pp. 1950 - 1966
The spherical harmonics m-mode decomposition is a powerful sky map reconstruction method suitable for radio interferometers operating in transit mode. It can... 
Techniques: interferometric | Methods: data analysis | Cosmology: observations | Large-scale structure of Universe | Methods: numerical | Radio lines: galaxies | methods: data analysis | large-scale structure of Universe | I MASS FUNCTION | TO 0.8 | methods: numerical | NONCOPLANAR ARRAYS | MAPPING EXPERIMENTS | LARGE-SCALE STRUCTURES | radio lines: galaxies | COSMOLOGY | ASTRONOMY & ASTROPHYSICS | BASE-LINES | cosmology: observations | RADIO INTERFEROMETRY | DATA RELEASE | WIDE-FIELD | techniques: interferometric
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9. Full Text Impact of photometric redshifts on the galaxy power spectrum BAO scale in the LSST survey
by Ansari, R and Choyer, A and Habibi, F and Magneville, C and Moniez, M and Plaszczynski, S and Renault, C and Ricol, JS and Souchard, J
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
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10. Full Text Sky reconstruction for the Tianlai cylinder array
by Jiao Zhang Shi-Fan Zuo Reza Ansari Xuelei Chen Yi-Chao Li Feng-Quan Wu Jean-Eric Campagne Christophe Magneville
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
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11. Full Text 21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction
by Ansari, R and Campagne, J. E and Colom, P and Goff, J. M. Le and Magneville, C and Martin, J. M and Moniez, M and Rich, J and Yèche, C
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
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12. Full Text E.R.O.S. SEARCH FOR MICROLENSING OF STARS BY LOW MASS OBJECTS IN THE GALACTIC HALO
by MAGNEVILLE, Christophe
Annals of the New York Academy of Sciences, ISSN 0077-8923, 09/1995, Volume 759, Issue 1, pp. 664 - 667
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13. Integration and testing of the DESI multi-object spectrograph: Performance tests and results for the first unit out of ten
by Perruchot, S and Guy, J and Le Guillou, L and Blanc, P.-E and Ronayette, S and Régal, X and Castagnoli, G and Sepulveda, E and Le Van Suu, A and Jullo, E and Cuby, J.-G and Karkar, S and Ghislain, P and Repain, P and Carton, P.-H and Magneville, C and Ealet, A and Escoffier, S and Secroun, A and Cousinou, M.-C and Honscheid, K and Elliot, A and Jelinsky, P and Brooks, D and Tarlè, G
Proceedings of SPIE - The International Society for Optical Engineering, ISSN 0277-786X, 2018, Volume 10702
DESI | integration | qualification | multi-object spectrograph | performance | Dark energy
Conference Proceeding
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14. Progress in the construction and testing of the Tianlai radio interferometers
by Das, Santanu and Anderson, Christopher J and Ansari, Reza and Campagne, Jean-Eric and Charlet, Daniel and Chen, Xuelei and Chen, Zhiping and Cianciara, Aleksander J and Colom, Pierre and Cong, Yanping and Gayley, Kevin G and Geng, Jingchao and Hao, Jie and Huang, Qizhi and Keith, Celeste S and Li, Chao and Li, Jixia and Li, Yichao and Liu, Chao and Liu, Tao and Magneville, Christophe and Marriner, John P and Martin, Jean-Michel and Moniez, Marc and Oxholm, Trevor M and Pen, Ue-Li and Perdereau, Olivier and Peterson, Jeffrey B and Shi, Huli and Shu, Lin and Stebbins, Albert and Sun, Shijie and Timbie, Peter T and Torchinsky, Steve and Tucker, Gregory S and Wang, Guisong and Wang, Rongli and Wang, Xin and Wang, Yougang and Wu, Fengquan and Xu, Yidong and Yu, Kaifeng and Zhang, Jiao and Zhang, Juyong and Zhang, Le and Zhu, Jialu and Zuo, Shifan
Proceedings of SPIE - The International Society for Optical Engineering, ISSN 0277-786X, 2018, Volume 10708
intensity-mapping | cosmology | neutral hydrogen | Radio interferometry
Conference Proceeding
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15. Full Text EROS search for microlensing of stars by low mass objects in the galactic halo
by Magneville, C
SEVENTEENTH TEXAS SYMPOSIUM ON RELATIVISTIC ASTROPHYSICS AND COSMOLOGY, ISSN 0077-8923, 1995, Volume 759, Issue 1, pp. 664 - 667
MULTIDISCIPLINARY SCIENCES
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16. Full Text Impact of photometric redshifts on the galaxy power spectrum and BAO scale in the LSST survey
by Ansari, Reza and Choyer, Adeline and Habibi, Farhang and Magneville, Christophe and Moniez, Marc and Plaszczynski, Stéphane and Renault, Cécile and Ricol, Jean-Stéphane and Souchard, Julien
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
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17. Full Text Astro2020 APC White Paper: The MegaMapper: a z > 2 spectroscopic instrument for the study of Inflation and Dark Energy
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
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18. Full Text The DESI Experiment Part I: Science,Targeting, and Survey Design
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... 
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19. Full Text The DESI Experiment Part II: Instrument Design
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... 
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20. Full Text DUNE: The Dark Universe Explorer
by Réfrégier, Alexandre and Boulade, Olivier and Mellier, Yannick and Milliard, Bruno and Pain, Reynald and Michaud, Joel and Safa, Frédéric and Amara, Adam and Astier, Pierre and Barrelet, Etienne and Bertin, Emmanuel and Boulade, Sébastien and Cara, Christophe and Claret, Arnaud and Georges, Laurent and Grange, Robert and Guy, Julien and Koeck, Charles and Kroely, Laurent and Magneville, Christophe and Palanque-Delabrouille, Nathalie and Regnault, Nicolas and Smadja, Gérard and Schimd, Carlo and Sun, Zhihong
Proceedings of SPIE - The International Society for Optical Engineering, ISSN 0277-786X, 2006, Volume 6265
Understanding the nature of Dark Matter and Dark Energy is one of the most pressing issues in cosmology and fundamental physics. The purpose of the DUNE (Dark... 
Weak lensing | Dark matter | Supernovae | Wide field imaging | Drift scan | Dark energy | Korsch telescope | CCD detectors | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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