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20022009
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations

Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA20097 cited

Re-analysis of the radio luminosity function of Galactic HII regions

R. Paladini, G. de Zotti, A. Noriega-Crespo +1

We have re-analyzed continuum and recombination lines radio data available in the literature in order to derive the luminosity function (LF) of Galactic HII regions. The study is p…

astro-ph.GA2009166 cited

Dynamical masses of early-type galaxies at z~2: Are they truly superdense?

Michele Cappellari, S. di Serego Alighieri, A. Cimatti +11

We measured stellar velocity dispersions sigma and dynamical masses of 9 massive (M~10^11 Msun) early-type galaxies (ETG) from the GMASS sample at redshift 1.4<z<2.0. The sigma are…

astro-ph.GA2009564 cited

The ACS Nearby Galaxy Survey Treasury

Julianne J. Dalcanton, Benjamin F. Williams, Anil C. Seth +24

The ACS Nearby Galaxy Survey Treasury (ANGST) is a systematic survey to establish a legacy of uniform multi-color photometry of resolved stars for a volume-limited sample of nearby…

astro-ph.GA200916 cited

Mid-UV Narrow-Band Indices of Evolved Simple Stellar Populations

Miguel Chavez, Emanuele Bertone, Javier Morales-Hernandez +1

We explore the properties of selected mid-ultraviolet (1900-3200 angstrom) spectroscopic indices of simple stellar populations (SSPs). We incorporate the high resolution UVBLUE ste…

astro-ph.GA200928 cited

The HELLAS2XMM Survey. XII. The infrared/sub-millimeter view of an X-ray selected Type 2 quasar at z=2

C. Vignali, F. Pozzi, J. Fritz +11

We present multi-wavelength observations (from optical to sub-millimeter, including Spitzer and SCUBA) of H2XMMJ 003357.2-120038 (also GD158_19), an X-ray selected, luminous narrow…

astro-ph.GA200922 cited

Pre-nova X-ray observations of V2491 Cyg (Nova Cyg 2008b)

A. Ibarra, E. Kuulkers, J. P. Osborne +12

Classical novae are phenomena caused by explosive hydrogen burning on an accreting white dwarf. So far, only one classical nova has been identified in X-rays before the actual opti…