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20032021
most citedLyman continuum leakage from low-mass galaxies with Mstar < 1.E8 Msun

145 citations · 559 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2021★ 145 cited

Lyman continuum leakage from low-mass galaxies with Mstar < 1.E8 Msun

Y. I. Izotov, G. Worseck, D. Schaerer +5

We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of nine low-mass star-forming galaxies at redshifts, z, in the range 0.3179-0.4524,…

astro-ph.GA2021★ 63 cited

Low-redshift compact star-forming galaxies as analogues of high-redshift star-forming galaxies

Y. I. Izotov, N. G. Guseva, K. J. Fricke +3

We compare the relations among various integrated characteristics of ~25,000 low-redshift (z<1.0) compact star-forming galaxies (CSFGs) from Data Release 16 (DR16) of the Sloan Dig…

astro-ph.GA2019★ 47 cited

Low-redshift lowest-metallicity star-forming galaxies in the SDSS DR14

Y. I. Izotov, N. G. Guseva, K. J. Fricke +1

We present a sample of low-redshift (z<0.133) candidates for extremely low-metallicity star-forming galaxies with oxygen abundances 12+logO/H<7.4 selected from the Data Release 14…

astro-ph2008★ 24 cited

Improved orbital solution and masses for the very low-mass multiple system LHS 1070

A. Seifahrt, T. Roell, R. Neuhaeuser +5

We present a refined orbital solution for the components A, B, and C of the nearby late-M type multiple system LHS 1070. By combining astrometric datapoints from NACO/VLT, CIAO/SUB…

astro-ph2007★ 50 cited

2D velocity fields of simulated interacting disc galaxies

T. Kronberger, W. Kapferer, S. Schindler +1

We investigate distortions in the velocity fields of disc galaxies and their use to reveal the dynamical state of interacting galaxies at different redshift. For that purpose, we m…

astro-ph2006★ 69 cited

Quiet Sun magnetic fields from simultaneous inversions of visible and infrared spectropolarimetric observations

Itahiza Dominguez Cerdena, Jorge Sanchez Almeida, Franz Kneer

We study the quiet Sun magnetic fields using spectropolarimetric observations of the infrared and visible Fe I lines at 6301.5, 6302.5, 15648 and 15653 A. Magnetic field strengths…