Ground-based and airborne instrumentation for astronomy

By J. Vandersteen, G. Raskin, T. Agócs, J. Morren, R. Østensen, W. Pessemier, S. Prins, Jan Swevers, S. Tulloch, H. Winckel and 1 more. 2010

829 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/5957878f200efc5c6f729602b13125a1df875c87

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Citations in the corpus

• The Habitability of Planets Orbiting M-dwarf Stars (2016, background): “The detection of the magnetic fields of the stars themselves with SPIRou will enable the detailed study of the impact of these fields upon planet occurrence (Artigau et al., 2014).”
• Shadows and spirals in the protoplanetary disk HD 100453 (2016, background): “Such a companion was detected in the cavity of the disk HD 142527 (Biller et al. 2012; Close et al. 2014) and found to be on an eccentric orbit (Lacour et al. 2016).”
• The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics from 10 to 100 au (2019, methodology): “Each frame of integral field spectroscopy data from GPI is processed with the GPI Data Reduction Pipeline (DRP; Perrin et al. 2014, 2016).”
• Dawes Review 6: The Impact of Companions on Stellar Evolution (2016, unknown): “…have LBV-like mass-loss rates and in four cases progenitors are known, e.g., SN 1961V (Smith et al., 2011b; Kochanek, Szczygiel, & Stanek, 2011), 2005gl (GalYam & Leonard, 2009), 2010jl (Smith et al., 2011b), and 2009ip (Smith et al. 2010, Foley et al. 2011; see also Smith (2014) for a review).”
• The COSMOS2015 galaxy stellar mass function . Thirteen billion years of stellar mass assembly in ten snapshots (2017, methodology): “…galaxies’ spectral energy distribution (SED), may cause systematics in their redshift distribution, or in following steps of the analysis, such as the evaluation of stellar mass (for a comparison among various SED fitting code, we refer to Conroy 2013; Mitchell et al. 2013; Mobasher et al. 2015).”
• The Zwicky Transient Facility: Observing System (2014, methodology): “CCD Controllers Five Archon CCD controllers, manufactured by Semiconductor Technology Associates (STA) (Bredthauer 2014) are mounted outside the telescope tube at the ends of two spider vanes.”
• Galaxy and mass assembly (GAMA): End of survey report and data release 2 (2015, background): “In addition, Sharp et al. (2013) found that the transmission of a given fibre also depends on the fibre’s distance from the plate centre, which they mainly attributed to radial variations of the apparent fibre diameter, of focal ratio degradation and of non-telecentricity.”
• The CARMENES Search for Exoplanets around M Dwarfs: A Low-mass Planet in the Temperate Zone of the Nearby K2-18 (2018, unknown): “For this study, observations were carried out with the high-resolution spectrograph CARMENES (Quirrenbach et al. 2014), which is the first operational spectrograph that is designed to obtain precise RVs in the visible and in the near-infrared (NIR) simultaneously.”
• Discovery of a warm, dusty giant planet around HIP 65426 (2017, unknown): “Also, note that the rotational velocities for single late-B and early-A stars in the Sco-Cen association and in the β Pic group match well typical values for the normal stars in the Zorec et al. (2012) catalog (while binaries typically rotate slower, as also found for field stars).”
• Illuminating gravitational waves: A concordant picture of photons from a neutron star merger (2017, methodology): “S1, S2, S3, S4, S5, S6, S7, S8, S9, S10 Table S1, S2, S3 References (48-175) Movie S1”
• The Karl G. Jansky Very Large Array Sky Survey (VLASS). Science Case and Survey Design (2019, background): “In the optical, both the Zwicky Transient Facility (ZTF; Smith et al. 2014) and the Large Synoptic Survey Telescope (LSST; Ivezić et al. 2019) will provide access to information on optical transients, and LSST will also produce a deep, multiband galaxy survey over the whole southern sky.”
• Gaia Data Release 2 (2018, background): “2008) minus Harps (Queloz et al. 2001; Mayor et al. 2003) and Sophie minus Elodie (Baranne et al.”
• SPHERE: the exoplanet imager for the Very Large Telescope (2019, unknown): “Coupling SPHERE with existing high-resolution spectro-graphs at the VLT has recently been proposed either in the visible with ESPRESSO (Lovis et al. 2017) or in the NIR with CRIRES + (Vigan et al. 2018b).”