papers

Publications (18)

astro-ph.CO2013

Lyman continuum leaking galaxies - Search strategies and local candidates

Nils Bergvall, Elisabet Leitet, Erik Zackrisson +1

Star-forming dwarf galaxies leaking Lyman-continuum (LyC) radiation may have played an important role in the reionization of the Universe. Local galaxies exhibiting LyC leakage cou…

astro-ph.GA2015

Kinematics of Haro11 - the miniature Antennae

Göran Östlin, Thomas Marquart, Robert Cumming +5

(abridged) Luminous blue compact galaxies are among the most active galaxies in the local universe in terms of their star formation rate per unit mass. They may be seen as the loca…

astro-ph.GA2009

Stellar kinematics in blue compact galaxies

Robert J. Cumming, Göran Östlin, Thomas Marquart +3

In a programme of observations of local luminous blue compact galaxies (BCGs), we are investigating kinematics by using tracers of both stars and ionized gas. Here we summarise our…

astro-ph.IM2020

HIRES, the high-resolution spectrograph for the ELT

Alessandro Marconi, Manuel Abreu, Vardan Adibekyan +99

HIRES will be the high-resolution spectrograph of the European Extremely Large Telescope at optical and near-infrared wavelengths. It consists of three fibre-fed spectrographs prov…

astro-ph.GA2014

The Lyman-alpha Reference Sample: I. Survey outline and first results for Markarian 259

Göran Östlin, Matthew Hayes, Florent Duval +19

The Lyman-alpha reference sample (LARS) is a program with the Hubble Space Telescope (HST) that provides a sample of local universe laboratory galaxies in which to study the astrop…

astro-ph.IM2026

The Tartu Observatory Fiber-fed Echelle Spectrograph (TOFES) Data Reduction Pipeline

Sandipan P. D. Borthakur, Tõnis Eenmäe, Nikolai Piskunov +9

We introduce the data reduction pipeline for the Tartu Observatory Fiber-fed Echelle Spectrograph (TOFES). TOFES is installed in the Coudé room and will be connected to the 1.5 m…

astro-ph2003

Can Microlensing Explain the Long-Term Optical Variability of Quasars?

Erik Zackrisson, Nils Bergvall, Thomas Marquart +1

Although controversial, the scenario of microlensing as the dominant mechanism for the long-term optical variability of quasars does provide a natural explanation for both the stat…

astro-ph.IM2018

Inside a VAMDC data node - Putting standards into practical software

Samuel Regandell, Thomas Marquart, Nikolai Piskunov

Access to molecular and atomic data is critical for many forms of remote sensing analysis across different fields. Many atomic and molecular databases are however highly specialize…

astro-ph2007

Stellar dynamics of blue compact galaxies. II. Further indications of a merger in ESO 338-IG04

Robert J. Cumming, Kambiz Fathi, Göran Östlin +5

Luminous blue compact galaxies, common at z~1 but now relatively rare, show disturbed kinematics in emission lines. As part of a programme to understand their formation and evoluti…

astro-ph.IM2020

Optimal extraction of echelle spectra: getting the most from observations

Nikolai Piskunov, Ansgar Wehrhahn, Thomas Marquart

The price of instruments and observing time on modern telescopes is quickly increasing with the size of the primary mirror. Therefore, it is worth revisiting the data reduction alg…

astro-ph2004

The starburst phenomenon from the optical/near-IR perspective

Nils Bergvall, Thomas Marquart, Göran Östlin +1

The optical/near-IR stellar continuum carries unique information about the stellar population in a galaxy, its mass function and star-formation history. Star-forming regions displa…

astro-ph.CO2012

Deep multiband surface photometry on star forming galaxies: I. A sample of 24 blue compact galaxies

Genoveva Micheva, Göran Östlin, Nils Bergvall +5

[Abridged] We present deep optical and near-infrared UBVRIHKs imaging data for 24 blue compact galaxies (BCGs). The sample contains luminous dwarf and intermediate-mass BCGs which…

astro-ph.GA2015

Local starburst galaxies and their descendants

Nils Bergvall, Thomas Marquart, Michael J. Way +4

Despite strong interest in the starburst (hereafter SB) phenomenon, the concept remains ill-defined. We use a strict definition of SB to examine the statistical properties of local…

astro-ph.CO2012

Deep multiband surface photometry on star forming galaxies: II. A volume limited sample of 21 emission lines galaxies

Genoveva Micheva, Göran Östlin, Erik Zackrisson +6

We present deep surface photometry of a volume--limited sample of 21 UM emission line galaxies in broadband optical UBVRI and near infra-red (NIR) HKs filters. The sample comprises…

astro-ph.IM2026

An archive of reduced and telluric-corrected CRIRES+ L- and M-band spectra with slit-tilt and wavelength calibrations

Thomas Marquart, Alexis Lavail

The high-resolution near-infrared spectrograph CRIRES+ at ESO VLT covers the Y, J, H, K, L and M bands. The U-Ne and Fabry-Perot calibration light sources, however, only work up to…

astro-ph.GA2023

The Lyman Reference Sample XIV: Lyman imaging of 45 low redshift star-forming galaxies and inferences on global emission

Jens Melinder, Göran Östlin, Matthew Hayes +18

We present Ly imaging of 45 low redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formatio…

astro-ph.EP2026

VLT/CRIRES+ observations of warm Neptune WASP-107 b: Challenges in detecting molecules with ground-based transmission spectroscopy of cooler and cloudy exoplanets

Linn Boldt-Christmas, Adam D. Rains, Nikolai Piskunov +15

Atmospheres of transiting exoplanets can be studied spectroscopically using space-based or ground-based observations. Each has its own strengths and weaknesses, so there are benefi…

astro-ph.IM2026

ANDES, the high-resolution spectrograph for the ELT: design and performance analysis of the YJH spectrograph

Vinooja Thurairethinam, David Lee, James Stevenson +29

The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is a powerful second-generation high-resolution spectroscopic instrument for the Extremely Large Telescope (ELT). The UBV…