Publications:

Journals

• A. Bauer, N. Drory, G.J. Hill, G. Feulner: Specific Star Formation Rates to Redshift 1.5, 2005, ApJL, in press, astro-ph/0412358
  
  
• P. Saracco, M. Longhetti, P. Severgnini, R. Della Ceca, V. Braito, F. Mannucci, R. Bender, N. Drory, G. Feulner, U. Hopp, C. Maraston: The density of very massive evolved galaxies to z ~ 1.7, 2005, MNRAS Letters, in press, astro-ph/0412020
  
  
• G. Feulner, Yu. Goranova, N. Drory, U. Hopp, R. Bender: The connection between star formation and stellar mass: Specific star formation rates to redshift one, 2005, MNRAS Letters, in press, astro-ph/0411774 (MUNICS VII)
  
  
• P. Severgnini, R. Della Ceca, V. Braito, P. Saracco, M. Longhetti, R. Bender, N. Drory, G. Feulner, U. Hopp, F. Mannucci, C. Maraston: Looking for obscured QSOs in the X-ray emitting ERO population, 2005, A&A, in press, astro-ph/0410434
  
  
• N. Drory, R. Bender, G. Feulner, U. Hopp, C. Maraston, J. Snigula, G. J. Hill: The Munich Near-Infrared Cluster Survey (MUNICS) - VI. The stellar masses of K-band selected field galaxies to z ~ 1.2, 2004, ApJ, 608, 742, astro-ph/0403041 (MUNICS VI)
  
  
• N. Drory, R. Bender, G. Feulner, U. Hopp, C. Maraston, J. Snigula, G. J. Hill: The Munich Near-Infrared Cluster Survey (MUNICS) - II. The K-Band Luminosity Function of Field Galaxies to z ~ 1.2, 2003, ApJ, 595, 698, astro-ph/0306299 (MUNICS II)
  
  
• G. Feulner, R. Bender, N. Drory, U. Hopp, J. Snigula, and G.J. Hill: The Munich Near-Infrared Cluster Survey (MUNICS) - V. The evolution of the rest-frame K-band and J-band galaxy luminosity functions to z = 0.7, 2003, MNRAS, 342, 605, astro-ph/0302517 (MUNICS V)
  
  
• P. Saracco, M. Longhetti, P. Severgnini, R. Della Ceca, F. Mannucci, R. Bender, N. Drory, G. Feulner, F. Ghinassi, U. Hopp, and C. Maraston: Massive z~1.3 evolved galaxies revealed, 2003, A&A, 398, 127, astro-ph/0211394
  
  
• J. Snigula, N. Drory, R. Bender, C.S. Botzler, G. Feulner, and U. Hopp: The Munich Near-Infrared Cluster Survey -- IV. Biases in the Completeness of Near-Infrared Imaging Data, 2002, MNRAS, 336, 1329, astro-ph/0207455 (MUNICS IV)
  
  
• N. Drory, R. Bender, J. Snigula, G. Feulner, U. Hopp, C. Maraston, G.J. Hill, and C. Mendes de Oliveira: The Munich Near-Infrared Cluster Survey (MUNICS) - Number density evolution of massive field galaxies to z = 1.2 as derived from the K-Band Selected Survey, 2001, ApJL, 562, 111, astro-ph/0110543 (MUNICS III)
  
  
• N. Drory, G. Feulner, R. Bender, C. S. Botzler, U. Hopp, C. Maraston, C. Mendes de Oliveira, and J. Snigula: The Munich Near-Infrared Cluster Survey - I. Field Selection, object extraction, and photometry, 2001, MNRAS, 325, 550, astro-ph/0102354 (MUNICS I)
  
  

Conference Proceedings

• N. Drory, R. Bender, G. Feulner, G.J. Hill, U. Hopp, C. Maraston, J. Snigula: The MUNICS Project: Galaxy Assembly at 0 < z < 1; R. Bender & A. Renzini (eds) - ESO/USM Workshop "Multiwavelength Mapping of Galaxy Formation and Evolution", Springer, 2004, astro-ph/0312345
  
  
• C.S. Botzler, J. Snigula, R. Bender, N. Drory, G. Feulner, G.J. Hill, U. Hopp, C. Maraston, and C. Mendes de Oliveira: Large-Scale Structure in the NIR-Selected MUNICS Survey, to appear in "The Evolution of Galaxies III. From Simple Approaches to Self-Consistent Models", proceedings of the 3rd EuroConference on the evolution of galaxies, held in Kiel, Germany, July 16-20, 2002, astro-ph/0210329
  
  
• N. Drory, R. Bender, J. Snigula, G. Feulner, U. Hopp, C. Maraston, G.J. Hill, and C. Mendes de Oliveira: The Mass Function of Field Galaxies at 0.4 < z < 1.2 Derived From the MUNICS K-Selected Sample; in: R. Bender & A. Renzini (eds) - ESO/USM Workshop 'The Mass of Galaxies at Low and High Redshift', Springer, 2002, astro-ph/0201207
  
  
• N. Drory, R. Bender, J. Snigula, G. Feulner, U. Hopp, C. Maraston, G.J. Hill, and C. Mendes de Oliveira: The Integrated Mass Function of Massive Field Galaxies to z = 1.2 as Derived from the K-Band Selected MUNICS Survey; in: M. Treyer & L. Tresse (eds) - 'Where's the Matter? Tracing Dark and Bright Matter with the New Generation of Large Scale Surveys', Frontier Group, 2001, p. 38
  
  
• G. Feulner, J. Snigula, N. Drory, R. Bender, U. Hopp, C. S. Botzler, C. Mendes de Oliveira, and G. J. Hill: The Munich Near-Infrared Cluster Survey (MUNICS): Radio Sources and Quasar Environments; in: M. Treyer & L. Tresse (eds) - 'Where's the Matter? Tracing Dark and Bright Matter with the New Generation of Large Scale Surveys', Frontier Group, 2001, p. 355
  
  
• G. Feulner, N. Drory, U. Hopp, J. Snigula, R. Bender, C. Maraston, C. S. Botzler, and C. Mendes de Oliveira: Field Galaxy Evolution from the Munich Near-Infrared Cluster Survey (MUNICS); in: A. J. Banday, S. Zaroubi, and M. Bartelmann (eds) - 'Mining the Sky - Proceedings of the MPA/ESO/MPE Workshop held at Garching, Germany', Springer Verlag, 2001, p. 211
  
  
• N. Drory, U. Hopp, R. Bender, G. Feulner, J. Snigula, C. Mendes de Oliveira, and G. Hill: The Munich Near-IR Cluster Survey (MUNICS); in: A. Mazure, O. LeFevre & V. Le Brun (eds) - 'Clustering At High Redshift', 2000, ASP Conf. Series, 200 astro-ph/9910268
  
  
• N. Drory, U. Hopp, C. Mendes de Oliveira, R. Bender, G. Hill, and R. P. Saglia: MUNICS - a near infrared search for high-redshifted clusters of galaxies, Astron. Ges. Abstract Ser. 14, 60 (1998)
  
  
• C. Mendes de Oliveira, U. Hopp, R. Bender, N. Drory, R. P. Saglia: A NIR search for high-redshift clusters; in ``Science with Gemini'', ed. Beatriz Barbuy (1998) astro-ph/9810021
  
  
• C. Mendes de Oliveira, N. Drory, U. Hopp, R. Bender, and R. P. Saglia: The MUNICS project -- a multicolor survey of distant galaxies; in ``Wide Field Surveys in Cosmology'', eds. Y. Mellier and S. Colombi, Editions Frontieres (1998) astro-ph/9809406
  
  

Theses

PhD Theses (all at the Ludwig-Maximilians-Universität München)

• N. Drory: A Near-Infrared Selected Photometric Survey of Distant Galaxies, 2002
  
  
• C.S. Botzler: Finding Structures in Photometric Redshift Surveys, 2004
  
  
• G. Feulner: A Near-Infrared Selected Galaxy Redshift Survey, 2004

Diploma Theses (German, all at the Ludwig-Maximilians-Universität München)

• C.S. Botzler: Dichteentwicklung von Galaxienhaufen, 1999
  
  
• G. Feulner: Optische Komplementärbeobachtungen zur Suche nach Galaxienhaufen im Infraroten, 2000
  
  
• J. Snigula: Analyse der Galaxienverteilungen in den Quasarfeldern des MUNICS-Surveys, 2001