ZUR REINDARSTELLUNG VON TRITIUMMARKIERTEN PYRIMIDINDERIVATEN. II: DARSTELLUNG VON 5-CYANO-(6-³H) URACIL = PURIFICATION DE DERIVES DE PYRIMIDINE TRITIES. II: PREPARATION DE CYANO-5 URACILE (³H)-6HEISE KH; NOLL S.1979; ISOTOPENPRAXIS; DDR; DA. 1979; VOL. 15; NO 9; PP. 292-293; BIBL. 5 REF.Article

PASSIVE AND ACTIVE RESIDENTIAL SOLAR HEATING: A COMPARATIVE ECONOMIC ANALYSIS OF SELECT DESIGNSROACH F; NOLL S; BEN DAVID S et al.1979; ENERGY; GBR; DA. 1979; VOL. 4; NO 4; PP. 623-644; BIBL. 13 REF.Article

ZUR REINDARSTELLUNG VON TRITIUMMARKIERTEN PYRIMIDINDERIVATEN. I. MARKIERUNG VON 5-HYDROXYURACIL UND 5-AMINOURACIL DURCH KATALYTISCHEN H-T-AUSTAUSCH. = PREPARATION DE DERIVES DE PYRIMIDINE PURS MARQUES AU TRITIUM. I. MARQUAGE D'HYDROXY-5 URACILE ET D'AMINO-5 URACILE PAR ECHANGE CATALYTIQUE H-TNOLL S; KIESSLING M; HEISE KH et al.1977; ISOTOPENPRAXIS; DTSCH.; DA. 1977; VOL. 13; NO 9; PP. 324-325; ABS. ANGL. RUSSE; BIBL. 4 REF.Article

Prospects for solar energy: the impact of the national energy planROACH F; NOLL S; BEN-DAVID S. et alii et al.1977, 46 p.Report

PHI-GKS: an implementation to support GKS-3D and PHIGSNOLL, S; POLLER, J.Computers & graphics. 1988, Vol 12, Num 2, pp 163-172, issn 0097-8493Article

Presence of dust with a UV bump in massive, star-forming galaxies at 1 < z < 2.5NOLL, S; PIERINI, D; PANNELLA, M et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 472, Num 2, pp 455-469, issn 0004-6361, 15 p.Article

The life stages of weight : Setting achievable goals appropriate to each womanHAMILTON, M. A; NONAS, C; NOLL, S et al.International journal of fertility and women's medicine. 2000, Vol 45, Num 1, pp 5-12, issn 1534-892XArticle

Passive and active residential solar heating: a comparative economic analysis of select designsROACH, F; NOLL, S; BEN-DAVID, S et al.Energy (Oxford). 1979, Vol 4, Num 4, pp 623-644Article

A deep i-selected multiwaveband galaxy catalogue in the COSMOS fieldGABASCH, A; GORANOVA, Y; HOPP, U et al.Monthly Notices of the Royal Astronomical Society. 2008, Vol 383, Num 4, pp 1319-1335, issn 0035-8711, 17 p.Article

Population synthesis modelling of luminous infrared galaxies at intermediate redshiftGIOVANNOLI, E; BUAT, V; NOLL, S et al.Astronomy and astrophysics (Berlin. Print). 2011, Vol 525, issn 0004-6361, A150.1-A150.13, 2Article

Electrochemical mediator-based delignification: Mediator properties and process performanceMICKEL, M; KIM, H.-C; NOLL, S et al.Journal of the Electrochemical Society. 2003, Vol 150, Num 12, pp B595-E600, issn 0013-4651Article

Technetium and rhenium complexes of mercapto-containing peptides. I: TC(V) and Re(V) complexes with mercaptoacetyl diglycine (MAG₂) and X-ray structure of AsPh₄[TcO(MAG₂)].C₂H₅OHJOHANNSEN, B; NOLL, B; LEIBNITZ, P et al.Inorganica chimica acta. 1993, Vol 210, Num 2, pp 209-214, issn 0020-1693Article

Lyα emission galaxies at a redshift of z ≈ 5.7 in the FORS deep fieldTAPKEN, C; APPENZELLER, I; GABASCH, A et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 455, Num 1, pp 145-152, issn 0004-6361, 8 p.Article

The Tully-Fisher relation at intermediate redshiftBÖHM, A; ZIEGLER, B. L; SAGLIA, R. P et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 420, Num 1, pp 97-114, issn 0004-6361, 18 p.Article

The evolution of the luminosity functions in the FORS Deep Field from low to high redshift. I. The blue bandsGABASCH, A; BENDER, R; MEHLERT, D et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 421, Num 1, pp 41-58, issn 0004-6361, 18 p.Article

Frequency and properties of bars in cluster and field galaxies at intermediate redshiftsBARAZZA, F. D; JABLONKA, P; RUDNICK, G et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 497, Num 3, pp 713-728, issn 0004-6361, 16 p.Article

Evolution of red-sequence cluster galaxies from redshift 0.8 to 0.4: ages, metallicities, and morphologiesSANCHEZ-BLAZQUEZ, P; JABLONKA, P; DE LUCIA, G et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 499, Num 1, pp 47-68, issn 0004-6361, 22 p.Article

Spectroscopy of clusters in the ESO distant cluster survey (EDisCS). II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fieldsMILVANG-JENSEN, B; NOLL, S; PELLO, R et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 482, Num 2, pp 419-449, issn 0004-6361, 31 p.Article