activity
19972023
most citedWeak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements

440 citations · 5k across the 112 of their papers we have counts for

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Showing astro-ph.GAShow all

18 papers · 1 filter

astro-ph.GA2023★ 26 cited

FAST reveals new evidence for M94 as a merger

Ruilei Zhou, Ming Zhu, Yanbin Yang +4

We report the first high-sensitivity HI observation toward the spiral galaxy M94 with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). From these observations, we…

astro-ph.GA2022★ 26 cited

The LOFAR view of giant, early-type galaxies: radio emission from active nuclei and star formation

A. Capetti, M. Brienza, B. Balmaverde +7

We study the properties and the origin of the radio emission in the most luminous early-type galaxies (ETGs) in the nearby Universe (MK<-25, recession velocity < 7,500 km/s) as see…

astro-ph.GA2022★ 27 cited

A 2-3 mm high-resolution molecular line survey towards the centre of the nearby spiral galaxy NGC 6946

Cosima Eibensteiner, Ashley T. Barnes, Frank Bigiel +30

The complex physical, kinematic, and chemical properties of galaxy centres make them interesting environments to examine with molecular line emission. We present new " (${\sim…

astro-ph.GA2021★ 2 cited

Extragalactic globular clusters with Euclid and other wide surveys

Ariane Lançon, S. Larsen, K. Voggel +14

Globular clusters play a role in many areas of astrophysics, ranging from stellar physics to cosmology. New ground-based optical surveys complemented by observations from space-bas…

astro-ph.GA2021★ 9 cited

Low star formation efficiency due to turbulent adiabatic compression in the Taffy bridge

B. Vollmer, J. Braine, B. Mazzilli-Ciraulo +1

The Taffy system (UGC 12914/15) consists of two massive spiral galaxies which had a head-on collision about 20 Myr ago. New sensitive, high-resolution CO(1-0) observations of the T…

astro-ph.GA2020★ 308 cited

The third realization of the International Celestial Reference Frame by very long baseline interferometry

P. Charlot, C. S. Jacobs, D. Gordon +17

A new realization of the International Celestial Reference Frame (ICRF) is presented based on the work achieved by a working group of the International Astronomical Union (IAU) man…

astro-ph.GA2020★ 7 cited

A study of extragalactic planetary nebulae populations based on spectroscopy. I. Data compilation and first findings

Gloria Delgado-Inglada, Jorge García-Rojas, Grazyna Stasińska +1

We compile published spectroscopic data and [O III] magnitudes of almost 500 extragalactic planetary nebulae (PNe) in 13 galaxies of various masses and morphological types. This is…

astro-ph.GA2020★ 12 cited

Detection of deuterated molecules, but not of lithium hydride, in the z=0.89 absorber toward PKS1830-211

S. Muller, E. Roueff, J. H. Black +8

Deuterium and lithium are light elements of high cosmological and astrophysical importance. In this work we report the first detection of deuterated molecules and a search for lith…

astro-ph.GA2019★ 125 cited

The 1.28 GHz MeerKAT DEEP2 Image

T. Mauch, W. D. Cotton, J. J. Condon +101

We present the confusion-limited 1.28 GHz MeerKAT DEEP2 image covering one FWHM primary beam area with FWHM resolution and Jy/beam rms nois…

astro-ph.GA2019★ 61 cited

Diffuse ionized gas and its effects on nebular metallicity estimates of star-forming galaxies

N. Vale Asari, G. S. Couto, R. Cid Fernandes +5

We investigate the impact of the diffuse ionized gas (DIG) on abundance determinations in star-forming (SF) galaxies. The DIG is characterised using the H equivalent width ($W_{…

astro-ph.GA2018★ 17 cited

The host galaxies of luminous type 2 AGN at 0.3-0.4

J. J. Urbano-Mayorgas, M. Villar Martín, F. Buitrago +7

We study the morphological and structural properties of the host galaxies associated with 57 optically-selected luminous type 2 AGN at 0.3-0.4: 16 high-luminosity Seyfert 2…

astro-ph.GA2018★ 4 cited

Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4

V. Casasola, L. Magrini, F. Combes +6

The aim of this paper is the spectroscopic study of 13 galaxies belonging to the field of the protocluster associated with the radio galaxy (RG) 7C 1756+6520 at z = 1.4156. In part…

astro-ph.GA2018★ 32 cited

Characterising the Circum-Galactic Medium of Damped Lyman- Absorbing Galaxies

Ramona Augustin, Celine Peroux, Palle Moller +8

Gas flows in and out of galaxies through their circumgalactic medium (CGM) are poorly constrained and direct observations of this faint, diffuse medium remain challenging. We use a…

astro-ph.GA2018★ 36 cited

Spatially Resolved Metal Gas Clouds

Celine Peroux, Hadi Rahmani, Fabrizio Arrigoni Battaia +1

We now have mounting evidences that the circumgalactic medium (CGM) of galaxies is polluted with metals processed through stars. The fate of these metals is however still an open q…

astro-ph.GA2017★ 27 cited

Detection of CH+, SH+, and their 13C- and 34S- isotopologues toward PKS1830-211

S. Muller, H. S. P. M"uller, J. H. Black +13

The z=0.89 molecular absorber toward PKS1830-211 provides us with the opportunity to probe the chemical and physical properties of the interstellar medium in the disk of a galaxy a…

astro-ph.GA2015★ 39 cited

Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf Spheroidal galaxy?

L. Sbordone, L. Monaco, C. Moni Bidin +8

The tidal disruption of the Sagittarius dwarf Spheroidal galaxy (Sgr dSph) is producing the most prominent substructure in the Milky Way (MW) halo, the Sagittarius Stream. Aside fr…

astro-ph.GA2015★ 34 cited

On the cosmic evolution of the specific star formation rate

M. D. Lehnert, W. van Driel, L. Le Tiran +2

The apparent correlation between the specific star formation rate (sSFR) and total stellar mass (M_star) of galaxies is a fundamental relationship indicating how they formed their…

astro-ph.GA2009★ 74 cited

Ram pressure stripping of the multiphase ISM in the Virgo cluster spiral galaxy NGC 4438

B. Vollmer, M. Soida, A. Chung +4

Ram pressure stripping of the multiphase ISM is studied in the perturbed Virgo cluster spiral galaxy NGC 4438. This galaxy underwent a tidal interaction ~100 Myr ago and is now str…