activity
19972009
most citedMAMBO Mapping of Spitzer c2d Small Clouds and Cores

625 citations · 919 across the 10 of their papers we have counts for

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Showing 2004Show all

10 papers · 1 filter

astro-ph2004

The connection between star formation and stellar mass: Specific star formation rates to redshift one

Georg Feulner, Yuliana Goranova, Niv Drory +2

We investigate the contribution of star formation to the growth of stellar mass in galaxies over the redshift range 0.5 < z < 1.1 by studying the redshift evolution of the specific…

astro-ph2004

The star formation rate history in the FORS Deep and GOODS South Fields

A. Gabasch, M. Salvato, R. P. Saglia +8

We measure the star formation rate (SFR) as a function of redshift z up to z \~4.5, based on B, I and (I+B) selected galaxy catalogues from the FORS Deep Field (FDF) and the K-sele…

astro-ph2004

Comparing spectroscopic and photometric stellar mass estimates

N. Drory, R. Bender, U. Hopp

The purpose of this letter is to compare the quality of different methods for estimating stellar masses of galaxies. We compare the results of (a) fitting stellar population synthe…

astro-ph2004

High Resolution Observations of the Near-Infrared Emission from NGC 6822 Hubble V

Sungho Lee, Soojong Pak, Sang-Gak Lee +4

We observed Hubble V, the brightest HII region complex in the dwarf irregular galaxy NGC 6822, at near-infrared (1.8--2.4 um) wavelengths using the Cooled Grating Spectrometer 4 (C…

astro-ph2004

A new mass-ratio for the X-ray Binary X2127+119 in M15?

L. van Zyl, Z. Ioannou, P. A. Charles +1

The luminous low-mass X-ray binary X2127+119 in the core of the globular cluster M15 (NGC 7078), which has an orbital period of 17 hours, has long been assumed to contain a donor s…

astro-ph2004

Mapping stationary axisymmetric phase-space distribution functions by orbit libraries

J. Thomas, R. P. Saglia, R. Bender +4

This is the first of a series of papers dedicated to unveil the mass composition and dynamical structure of a sample of flattened early type galaxies in the Coma cluster. We descri…