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Results 1 to 25 of 7807

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Fluram labeling of high density NH2 surfacesPIPPIG, F; HOLLÄNDER, A.Applied surface science. 2007, Vol 253, Num 16, pp 6817-6823, issn 0169-4332, 7 p.Article

How Future Space-Based Weak-Lensing Surveys Might Obtain Photometric Redshifts IndependentlySORBA, R; SAWICKI, M.Publications of the Astronomical Society of the Pacific. 2011, Vol 123, Num 905, pp 777-788, issn 0004-6280, 12 p.Article

Estimating photometric redshifts using support vector machinesWADADEKAR, Yogesh.Publications of the Astronomical Society of the Pacific. 2005, Vol 117, Num 827, pp 79-85, issn 0004-6280, 7 p.Article

Can Self-Organizing Maps Accurately Predict Photometric Redshifts?WAY, M. J; KLOSE, C. D.Publications of the Astronomical Society of the Pacific. 2012, Vol 124, Num 913, pp 274-279, issn 0004-6280, 6 p.Article

EZ: A Tool For Automatic Redshift MeasurementGARILLI, B; FUMANA, M; FRANZETTI, P et al.Publications of the Astronomical Society of the Pacific. 2010, Vol 122, Num 893, pp 827-838, issn 0004-6280, 12 p.Article

Empirical Optical k-Corrections for RedshiftsWESTRA, Eduard; GELLER, Margaret J; KURTZ, Michael J et al.Publications of the Astronomical Society of the Pacific. 2010, Vol 122, Num 897, pp 1258-1284, issn 0004-6280, 27 p.Article

The carnegie supernova project : The low-redshift surveyHAMUY, Mario; FOLATELLI, Gaston; FREEDMAN, Wendy L et al.Publications of the Astronomical Society of the Pacific. 2006, Vol 118, Num 839, pp 2-20, issn 0004-6280, 19 p.Article

High Redshift Galaxies in the Hubble Ultra Deep FieldHATHI, Nimish P.Publications of the Astronomical Society of the Pacific. 2008, Vol 120, Num 873, pp 1255-1257, issn 0004-6280, 3 p.Article

A QSO discovered at the redshift of the extended x-ray cluster RX j0152.7-1357BURBIDGE, E. M; GUTIERREZ, C. M; ARP, H et al.Publications of the Astronomical Society of the Pacific. 2006, Vol 118, Num 839, pp 124-128, issn 0004-6280, 5 p.Article

The physical nature of Lyα-emitting galaxies at z = 3.1GAWISER, Eric; VAN DOKKUM, Pieter G; HERRERA, David et al.The Astrophysical journal. 2006, Vol 642, Num 1, issn 0004-637X, L13-L16, 2Article

A Dual-Narrowband Survey for Hα Emitters at Redshift of 2.2: Demonstration of the Technique and Constraints on the Hα Luminosity FunctionLEE, Janice C; CHUN LY; SPITLER, Lee et al.Publications of the Astronomical Society of the Pacific. 2012, Vol 124, Num 917, pp 782-797, issn 0004-6280, 16 p.Article

L'évolution de l'Univers = The evolution of the UniversePEEBLES, J; SCHRAMM, D; TURNER, E et al.Pour la science. 1994, Num 206, pp 52-58, issn 0153-4092, NSArticle

Optical response characteristics arising from delocalized electrons in phase change materialsHO, H. W; BAI, K; SONG, W. D et al.Acta materialia. 2013, Vol 61, Num 5, pp 1757-1763, issn 1359-6454, 7 p.Article

The effect of electric field strength on electroplex emission at the interface of NPB/PBD organic light-emitting diodesZHAO, De-Wei; ZHENG XU; ZHANG, Fu-Jun et al.Applied surface science. 2007, Vol 253, Num 8, pp 4025-4028, issn 0169-4332, 4 p.Article

General formula for comparison of clock rates- : applications to cosmos and solar systemCHONGMING XU; XUEJUN WU; BRÜNING, Erwin et al.Classical and quantum gravity (Print). 2005, Vol 22, Num 23, pp 5015-5028, issn 0264-9381, 14 p.Article

Are high-redshift quasars blurry?STEINBRING, Eric.The Astrophysical journal. 2007, Vol 655, Num 2, pp 714-717, issn 0004-637X, 4 p., 1Article

Dark energy reflections in the redshift-space quadrupoleYAMAMOTO, Kazuhiro; BASSETT, Bruce A; NISHIOKA, Hiroaki et al.Physical review letters. 2005, Vol 94, Num 5, pp 051301.1-051301.4, issn 0031-9007Article

Improved templates for photometric redshifts of submillimeter sourcesHUNT, L. K; MAIOLINO, R.The Astrophysical journal. 2005, Vol 626, Num 1, pp L15-L18, issn 0004-637X, 2Article

A 3.5-Gyr-old galaxy at redshift 1.55DUNLOP, J; PEACOCK, J; SPINRAD, H et al.Nature (London). 1996, Vol 381, Num 6583, pp 581-584, issn 0028-0836Article

Photometric Redshift Biases from Galaxy EvolutionJONATHAN MACDONALD, C; BERNSTEIN, Gary.Publications of the Astronomical Society of the Pacific. 2010, Vol 122, Num 890, pp 485-489, issn 0004-6280, 5 p.Article

A NEW DETERMINATION OF THE HIGH-REDSHIFT TYPE Ia SUPERNOVA RATES WITH THE HUBBLE SPACE TELESCOPE ADVANCED CAMERA FOR SURVEYSKUZNETSOVA, N; BARBARY, K; FADEYEV, V et al.The Astrophysical journal. 2008, Vol 673, Num 2, pp 981-998, issn 0004-637X, 18 p., 1Article

Subaru deep survey. v. a census of lyman break galaxies at z ~ 4 and 5 in the subaru deep fields: Photometric propertiesOUCHI, Masami; SHIMASAKU, Kazuhiro; MIYAZAKI, Masayuki et al.The Astrophysical journal. 2004, Vol 611, Num 2, pp 660-684, issn 0004-637X, 25 p., 1Article

A high deuterium abundance at redshift z = 0.7WEBB, J. K; CARSWELL, R. F; LANZETTA, K. M et al.Nature (London). 1997, Vol 388, Num 6639, pp 250-252, issn 0028-0836Article

A nearby massive galaxy cluster behind the Milky WayKRAAN-KORTEWEG, R. C; WOUDT, P. A; CAYATTE, V et al.Nature (London). 1996, Vol 379, Num 6565, pp 519-521, issn 0028-0836Article

Search and redshift survey for IRAS galaxies behind the Northern Milky WayTAKATA, T; YAMADA, T; SAITO, M et al.Astronomy & astrophysics. Supplement Series (Print). 1994, Vol 104, Num 3, pp 529-555, issn 0365-0138Article

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