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MID-Radio Telescope, Single Pixel Feed Packages for the Square Kilometer Array: An Overview
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123
Advances in optical engineering for future telescopes
Published 2021-06-01“…Among these, the Nautilus space observatory requires challenging alignment of segmented multi-order diffractive elements. …”
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124
A compact receiver system for simultaneous measurements of mesospheric CO and O<sub>3</sub>
Published 2016-02-01“…The first measurement series from October 2014 until April 2015 taken at the Onsala Space Observatory, OSO (57° N, 12° E), is analysed. …”
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125
Galileo L10 Satellites: Orbit, Clock and Signal-in-Space Performance Analysis
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126
Bi-Spectral Infrared Algorithm for Cloud Coverage over Oceans by the JEM-EUSO Mission Program
Published 2021-09-01“…Specifically, this article evaluates a method to determine the cloud map from the images provided by a simple bi-spectral infrared camera within the framework of JEM-EUSO (The Joint Experiment Missions-Extrem Universe Space Observatory). This program involves different experiments whose aim is determining properties of Ultra-High Energy Cosmic Ray (UHECR) via the detection of atmospheric fluorescence light. …”
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127
Evolution of the Outflow in the Water Fountain Source IRAS 18043–2116
Published 2023-01-01Get full text
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128
Spektr–UF Mission Spectrograph Space Qualified CCD Detector Subsystem
Published 2023-09-01“…Spektr–UF (World Space Observatory Ultraviolet, WSO-UV) is a Russian-led international collaboration aiming to develop a large space-borne 1.7 m Ritchey–Chretién telescope with science instruments to study the Universe in ultraviolet wavelengths. …”
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129
Far-infrared properties of submillimeter and optically faint radio galaxies
Published 2010“…We use deep observations obtained with the Photodetector Array Camera and Spectrometer (PACS) onboard the Herschel Space Observatory to study the far-infrared (FIR) properties of submillimeter and optically faint radio galaxies (SMGs and OFRGs). …”
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130
Far-infrared properties of submillimeter and optically faint radio galaxies
Published 2010“…We use deep observations obtained with the Photodetector Array Camera and Spectrometer (PACS) onboard the Herschel Space Observatory to study the far-infrared (FIR) properties of submillimeter and optically faint radio galaxies (SMGs and OFRGs). …”
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The LOFAR two-metre sky survey deep fields: the star-formation rate–radio luminosity relation at low frequencies
Published 2021“…The LOFAR Surveys Key Science Project is transforming our understanding of the low-frequency radio sky, with the 150 MHz data over the European Large Area Infrared Space Observatory Survey-North 1 field reaching an rms sensitivity of 20 μJy beam−1 over 10 deg2 at 6 arcsec resolution. …”
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132
Goods-Herschel measurements of the dust attenuation of typical star-forming galaxies at high redshift: Observations of ultraviolet-selected galaxies at z ∼ 2
Published 2012“…We take advantage of the sensitivity and resolution of the Herschel Space Observatory at 100 and 160 μm to directly image the thermal dust emission and investigate the infrared luminosities (L IR) and dust obscuration of typical star-forming (L*) galaxies at high redshift. …”
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133
The Radio Parallax of the Crab Pulsar: A First VLBI Measurement Calibrated with Giant Pulses
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Galaxy and Mass Assembly (GAMA): Low-redshift Quasars and Inactive Galaxies Have Similar Neighbors
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Reconstruction and searching ozone data periodicities in southern Brazil (29ºS, 53ºW) Reconstrução e procura de periodicidades nos dados de ozonio região sul do Brasil (29ºS, 53ºW)...
Published 2012-07-01“…In this work, a reconstruction of ozone time series obtained by Brewer spectrophotometer from 1994 to 2008 at the Southern Space Observatory (SSO) - 29ºS, 53ºW - Southern Brazil is presented. …”
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137
Waves and Magnetism in the Solar Atmosphere (WAMIS)
Published 2016-02-01“…These comprehensive observations are not provided by any current single ground-based or space observatory. The fundamental advancements achieved by the near-space observations of WAMIS on coronal field would point the way for future ground based and orbital instrumentation.…”
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The need for a multi-purpose, optical–NIR space facility after HST and JWST
Published 2021“…Abstract In the early 2030s, after the end of operations for the epochal Hubble Space Telescope and the long-anticipated James Webb Space Telescope, astrophysics will lose access to a general purpose high-spatial resolution space observatory to cover the UV–optical–NIR wavelength range with a variety of imaging bandpasses and high-multiplexing mid-resolution spectroscopy. …”
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139
The evolution of the dust temperatures of galaxies in the SFR-M-* plane up to z similar to 2
Published 2014“…We study the evolution of the dust temperature of galaxies in the SFR-Mâ̂- plane up to z ~ 2 using far-infrared and submillimetre observations from the Herschel Space Observatory taken as part of the PACS Evolutionary Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) guaranteed time key programmes. …”
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Herschel unveils a puzzling uniformity of distant dusty galaxies
Published 2010“…The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. …”
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