scholarly journals MUSE deep-fields: the Ly α luminosity function in the Hubble Deep Field-South at 2.91 < z < 6.64

2017 ◽  
Vol 471 (1) ◽  
pp. 267-278 ◽  
Author(s):  
Alyssa B. Drake ◽  
Bruno Guiderdoni ◽  
Jérémy Blaizot ◽  
Lutz Wisotzki ◽  
Edmund Christian Herenz ◽  
...  
Keyword(s):  
Luminosity Function ◽  
Deep Fields ◽  
Hubble Deep Field

scholarly journals A MUSE View of the HDFS: The Lyα Luminosity Function out to z~6

2015 ◽  
Vol 11 (S319) ◽  
pp. 12-15
Author(s):  
Alyssa B. Drake ◽  
Bruno Guiderdoni ◽  
Jérémy Blaizot ◽  
Johan Richard ◽  
Roland Bacon ◽  
...  
Keyword(s):  
Current Literature ◽  
Luminosity Function ◽  
Homogeneous Sample ◽  
Detection Power ◽  
Preliminary Results ◽  
Hubble Ultra Deep Field ◽  
Hubble Deep Field ◽  
The Universe

AbstractWe present preliminary results from MUSE on the Lyα luminosity function in the Hubble Deep Field South (HDFS). Using a large homogeneous sample of LAEs selected through blind spectroscopy, we utilise the unprecedented detection power of MUSE to study the progenitors of L* galaxies back to when the Universe was just ~2 Gyr old. We present these results in the context of the current literature, and highlight the importance of the forthcoming Hubble Ultra Deep Field (HUDF) study with MUSE, which will increase the size of our sample by a factor of ~ 10.

scholarly journals Probing the evolution of the near-infrared luminosity function of galaxies to z = 3 in the Hubble Deep Field-South

2006 ◽  
Vol 367 (1) ◽  
pp. 349-365 ◽  
Author(s):  
P. Saracco ◽  
A. Fiano ◽  
G. Chincarini ◽  
E. Vanzella ◽  
M. Longhetti ◽  
...  
Keyword(s):  
Luminosity Function ◽  
Near Infrared ◽  
Hubble Deep Field

scholarly journals Quasars

1999 ◽  
Vol 194 ◽  
pp. 97-104
Author(s):  
Patrick S. Osmer
Keyword(s):  
Luminosity Function ◽  
Theoretical Work ◽  
Observational Research ◽  
Host Galaxies ◽  
Field Evolution ◽  
Research Problems ◽  
Hubble Deep Field

I review recent results for quasars and discuss how they are related to activity in galaxies. Topics included are studies of quasar host galaxies with HST; searches for quasars in the Hubble Deep Field; evolution of the quasar luminosity function; news highlights from astro-ph; and current observational research problems and their relation to theoretical work.

Galaxy Luminosity Function: Applications and Cosmological Implications

2005 ◽  
Vol 201 ◽  
pp. 519-520
Author(s):  
Tsutomu T. Takeuchi ◽  
Kohji. Yoshikawa ◽  
Takako T. Ishii
Keyword(s):  
Monte Carlo ◽  
Monte Carlo Simulations ◽  
Statistical Methods ◽  
Luminosity Function ◽  
Photometric Redshift ◽  
Hubble Deep Field ◽  
Galaxy Luminosity Function

We studied the statistical methods for the estimation of the luminosity function (LF) of galaxies by Monte Carlo simulations. After examining the performance of these methods, we analyzed the photometric redshift data of the Hubble Deep Field prepared by Fernández-Soto et al. (1999). We also derived luminosity density ρL at B- and I-band. Our B-band estimation is roughly consistent with that of Sawicki, Lin, & Yee (1997), but a few times lower at 2.0 < z < 3.0. The evolution of ρL(I) is found to be less prominent.

The Evolution of the Luminosity Function in Deep Fields: A Comparison with Cold Dark Matter Models

2001 ◽  
Vol 551 (1) ◽  
pp. L45-L48 ◽  
Author(s):  
F. Poli ◽  
N. Menci ◽  
E. Giallongo ◽  
A. Fontana ◽  
S. Cristiani ◽  
...  
Keyword(s):  
Dark Matter ◽  
Luminosity Function ◽  
Cold Dark Matter ◽  
Deep Fields

scholarly journals A MOLECULAR LINE SCAN IN THE HUBBLE DEEP FIELD NORTH: CONSTRAINTS ON THE CO LUMINOSITY FUNCTION AND THE COSMIC H2DENSITY

2014 ◽  
Vol 782 (2) ◽  
pp. 79 ◽  
Author(s):  
F. Walter ◽  
R. Decarli ◽  
M. Sargent ◽  
C. Carilli ◽  
M. Dickinson ◽  
...  
Keyword(s):  
Luminosity Function ◽  
Molecular Line ◽  
Line Scan ◽  
Hubble Deep Field
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