Dust biasing of damped Lyman alpha systems : a Bayesian analysisPONTZEN, Andrew; PETTINI, Max.Monthly notices of the Royal Astronomical Society (Print). 2009, Vol 393, Num 2, pp 557-568, issn 0035-8711, 12 p.Article

New insights into the stellar content and physical conditions of star-forming galaxies at z = 2-3 from spectral modellingBRINCHMANN, Jarle; PETTINI, Max; CHARLOT, Stéphane et al.Monthly Notices of the Royal Astronomical Society. 2008, Vol 385, Num 2, pp 769-782, issn 0035-8711, 14 p.Article

THE TEMPERATURE-DENSITY RELATION IN THE INTERGALACTIC MEDIUM AT REDSHIFT (z) = 2.4RUDIE, Gwen C; STEIDEL, Charles C; PETTINI, Max et al.The Astrophysical journal. 2012, Vol 757, Num 2, issn 0004-637X, L30.1-L30.6, 2Article

DETECTION OF THE TRANSVERSE PROXIMITY EFFECT : RADIATIVE FEEDBACK FROM BRIGHT QSOsGONCALVES, Thiago S; STEIDEL, Charles C; PETTINI, Max et al.The Astrophysical journal. 2008, Vol 676, Num 2, pp 816-835, issn 0004-637X, 20 p., 1Article

A search for damped Lyman a systems towards radio-loud quasars I: the optical surveyELLISON, Sara L; YORK, Brian A; PETTINI, Max et al.Monthly Notices of the Royal Astronomical Society. 2008, Vol 388, Num 3, pp 1349-1360, issn 0035-8711, 12 p.Article

The most metal-poor damped Lyα systems: insights into chemical evolution in the very metal-poor regimeCOOKE, Ryan; PETTINI, Max; STEIDEL, Charles C et al.Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 417, Num 2, pp 1534-1558, issn 0035-8711, 25 p.Article

The direct detection of lyman continuum emission from star-forming galaxies at z∼3SHAPLEY, Alice E; STEIDEL, Charles C; PETTINI, Max et al.The Astrophysical journal. 2006, Vol 651, Num 2, pp 688-703, issn 0004-637X, 16 p., 1Article

The ultraviolet spectrum of the gravitationally lensed galaxy 'the Cosmic Horseshoe': a close-up of a star-forming galaxy at z ~ 2QUIDER, Anna M; PETTINI, Max; SHAPLEY, Alice E et al.Monthly notices of the Royal Astronomical Society (Print). 2009, Vol 398, Num 3, pp 1263-1278, issn 0035-8711, 16 p.Article

The kinematics of morphologically selected z ∼ 2 galaxies in the goods-north fieldERB, Dawn K; STEIDEL, Charles C; SHAPLEY, Alice E et al.The Astrophysical journal. 2004, Vol 612, Num 1, pp 122-130, issn 0004-637X, 9 p., 1Article

On the reliability of C IV λ1549 as an abundance indicator for high-redshift star-forming galaxiesCROWTHER, Paul A; PRINJA, Raman K; PETTINI, Max et al.Monthly Notices of the Royal Astronomical Society. 2006, Vol 368, Num 2, pp 895-902, issn 0035-8711, 8 p.Article

Evidence for solar metallicities in massive star-forming galaxies at z ≥ 2SHAPLEY, Alice E; ERB, Dawn K; PETTINI, Max et al.The Astrophysical journal. 2004, Vol 612, Num 1, pp 108-121, issn 0004-637X, 14 p., 1Article

DIFFUSE Lyα EMITTING HALOS: A GENERIC PROPERTY OF HIGH-REDSHIFT STAR-FORMING GALAXIESSTEIDEL, Charles C; BOGOSAVLJEVIC, Milan; SHAPLEY, Alice E et al.The Astrophysical journal. 2011, Vol 736, Num 2, issn 0004-637X, 160.1-160.18, 1Article

A newly discovered DLA and associated Lyα emission in the spectra of the gravitationally lensed quasar UM 673A,BCOOKE, Ryan; PETTINI, Max; STEIDEL, Charles C et al.Monthly notices of the Royal Astronomical Society (Print). 2010, Vol 409, Num 2, pp 679-693, issn 0035-8711, 15 p.Article

The host galaxies of strong Ca π quasar absorption systems at z < 0.5ZYCH, Berkeley J; MURPHY, Michael T; PETTINI, Max et al.Monthly Notices of the Royal Astronomical Society. 2007, Vol 379, Num 4, pp 1409-1422, issn 0035-8711, 14 p.Article

The connection between galaxies and intergalactic absorption lines at redshift 2 ≤ z ≤ 3ADELBERGER, Kurt L; SHAPLEY, Alice E; STEIDEL, Charles C et al.The Astrophysical journal. 2005, Vol 629, Num 2, pp 636-653, issn 0004-637X, 18 p., 1Article

The spatial clustering of star-forming galaxies at redshifts 1.4 ≤ z ≤ 3.5ADELBERGER, Kurt L; STEIDEL, Charles C; PETTINI, Max et al.The Astrophysical journal. 2005, Vol 619, Num 2, pp 697-713, issn 0004-637X, 17 p., 1Article

Large-scale outflows from z ~ 0.7 starburst galaxies identified via ultrastrong Mg II quasar absorption linesNESTOR, Daniel B; JOHNSON, Benjamin D; WILD, Vivienne et al.Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 412, Num 3, pp 1559-1572, issn 0035-8711, 14 p.Article

PHYSICAL CONDITIONS IN A YOUNG, UNREDDENED, LOW-METALLICITY GALAXY AT HIGH REDSHIFTERB, Dawn K; PETTINI, Max; SHAPLEY, Alice E et al.The Astrophysical journal. 2010, Vol 719, Num 2, pp 1168-1190, issn 0004-637X, 23 p., 1Article

Morphologies of galaxies in and around a protocluster at z = 2.300PETER, Annika H. G; SHAPLEY, Alice E; LAW, David R et al.The Astrophysical journal. 2007, Vol 668, Num 1, pp 23-44, issn 0004-637X, 22 p., 1Article

Ultraviolet to mid-infrared observations of star-forming galaxies at z ∼ 2 : Stellar masses and stellar populationsSHAPLEY, Alice E; STEIDEL, Charles C; ERB, Dawn K et al.The Astrophysical journal. 2005, Vol 626, Num 2, pp 698-722, issn 0004-637X, 25 p., 1Article

The nature of H I absorbers in gamma-ray burst afterglows: clues from hydrodynamic simulationsPONTZEN, Andrew; DEASON, Alis; GOVERNATO, Fabio et al.Monthly notices of the Royal Astronomical Society (Print). 2010, Vol 402, Num 3, pp 1523-1535, issn 0035-8711, 13 p.Article

THE RELATIONSHIP BETWEEN STELLAR POPULATIONS AND Lyα EMISSION IN LYMAN BREAK GALAXIESKORNEI, Katherine A; SHAPLEY, Alice E; ERB, Dawn K et al.The Astrophysical journal. 2010, Vol 711, Num 2, pp 693-710, issn 0004-637X, 18 p., 1Article

HIGH-REDSHIFT STARBURSTING DWARF GALAXIES REVEALED BY γ-RAY BURST AFTERGLOWSCHEN, Hsiao-Wen; PERLEY, Daniel A; POLLACK, Lindsey K et al.The Astrophysical journal. 2009, Vol 691, Num 1, pp 152-174, issn 0004-637X, 23 p., 1Article

THE KILOPARSEC-SCALE KINEMATICS OF HIGH-REDSHIFT STAR-FORMING GALAXIESLAW, David R; STEIDEL, Charles C; ERB, Dawn K et al.The Astrophysical journal. 2009, Vol 697, Num 2, pp 2057-2082, issn 0004-637X, 26 p., 1Article

THE SIGHTLINE TO Q2343-BX415 : CLUES TO GALAXY FORMATION IN A QUASAR ENVIRONMENT'RIX, Samantha A; PETTINI, Max; STEIDEL, Charles C et al.The Astrophysical journal. 2007, Vol 670, Num 1, pp 15-38, issn 0004-637X, 24 p., 1Article