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81
Low-voltage Power Supply Subsystem for a Sub-Orbital Particle Physic Instrument
Published 2014-01-01“…The Japanese Experiment Module–Extreme Universe Space Observatory (JEM-EUSO) is a wide-field (+/-~30°of aperture) 2.5m refractor telescope to be installed in the International Space Station (ISS). …”
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82
GNSS-IR Model of Sea Level Height Estimation Combining Variational Mode Decomposition
Published 2021-01-01“…In order to verify the validity of the new GNSS-IR model, the measurement data provided by the Onsala Space Observatory in Sweden is used to evaluate the performance of the algorithm and its stability in high-elevation range. …”
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83
Absolute calibration of the JEM-EUSO photodetection modules
Published 2023-01-01“…The JEM-EUSO (Joint Experiment Missions for Extreme Universe Space Observatory) collaboration constructs a series of balloon and orbital telescopes to detect fluorescent UV emission from the Earth atmosphere, with the primary aim to study ultra-high-energy cosmic rays (UHECRs) from space. …”
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84
Six years of mesospheric CO estimated from ground-based frequency-switched microwave radiometry at 57° N compared with satellite instruments
Published 2012-11-01“…Ground-based measurements of mesospheric CO made at the Onsala Space Observatory, OSO, (57° N, 12° E) are presented. The dataset covers the period 2002–2008 and is hence uniquely long for ground-based observations. …”
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85
INFRARED COUNTERPARTS OF X-RAY GALAXIES
Published 2019-11-01“…In this paper we make identification and cross-correlate of the infrared and X-ray observational data, build a distribution of a selected sample sources by types and attempted to analyze types of the extragalactic objects at distances up to z = 0.1 using observational data of relevant space observatories. Data from a leading X-ray space observatory XMM-Newton were used to compile the largest catalog of X-ray sources. …”
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86
Observations on breeding behaviour of a pair of endangered Egyptian Vultures Neophron percnopterus (Linnaeus, 1758) over three breeding seasons in the plains of Punjab, India
Published 2020-06-01“…The site is located in the hollow of a ventilation window of the Space Observatory in Punjabi University, Patiala, Punjab. …”
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87
A commercial radio receiver for lower ionosphere monitoring: Initial results
Published 2004-04-01“…The system was installed at the Southern Space Observatory (OES/CRSPE/INPE) in Sāo Martinho da Serra, Brazil (29.43°S, 53.8°W, B = 23350 nT). …”
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88
Kinematically engaged yoke system for segmented lens-based space telescope integration and testing
Published 2023-01-01“…The paradigm-shifting investigation described here calls for a new type of scalable space telescope that redefines the available light-collecting area in space. The Nautilus Space Observatory, enabled by multiple-order diffractive optics (the MODE lens), is ushering in the advent of large space telescope lenses designed to search for biosignatures on a thousand exo-earths. …”
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89
Evolution of dust temperature of galaxies through cosmic time as seen by Herschel
Published 2010“…We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-North as part of the PACS Extragalactic Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) key programmes. …”
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90
H-ATLAS: PACS imaging for the Science Demonstration Phase
Published 2010“…We describe the reduction of data taken with the PACS instrument on board the Herschel Space Observatory in the Science Demonstration Phase of the Herschel-ATLAS (H-ATLAS) survey, specifically data obtained for a 4 × 4 deg2 region using Herschel's fast-scan (60 arcsec s-1) parallel mode. …”
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91
Far-infrared line deficits in galaxies with extreme L /M ratios
Published 2011“…A deficit of the [C II] 158 μm line relative to L was previously found with the Infrared Space Observatory, but now we show for the first time that this is a general aspect of all far-infrared fine structure lines, regardless of their origin in the ionized or neutral phase of the interstellar medium. …”
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92
Stacked average far-infrared spectrum of dusty star-forming galaxies from the Herschel /SPIRE Fourier Transform Spectrometer
Published 2017“…We present stacked average far-infrared spectra of a sample of 197 dusty star-forming galaxies (DSFGs) at 0.005 < z < 4 using about 90% of the Herschel Space Observatory SPIRE Fourier Transform Spectrometer (FTS) extragalactic data archive based on 3.5 years of science operations. …”
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93
Far-infrared line deficits in galaxies with extreme LFIR/M H2 ratios
Published 2011“…A deficit of the [C II] 158 μm line relative to LFIR was previously found with the Infrared Space Observatory, but now we show for the first time that this is a general aspect of all far-infrared fine structure lines, regardless of their origin in the ionized or neutral phase of the interstellar medium. …”
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94
The European Large Area ISO survey - VIII. 90-mu m final analysis and source counts
Published 2004“…We present a re-analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 90-μm observations carried out with ISOPHOT, an instrument on board the ISO of the European Space Agency. …”
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95
The ALCHEMI Atlas: Principal Component Analysis Reveals Starburst Evolution in NGC 253
Published 2024-01-01Get full text
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96
The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis
Published 2022-01-01“…The PDR Toolbox enables novel analysis of data from telescopes such as the Infrared Space Observatory, Spitzer, Herschel, the Stratospheric Terahertz Observatory, the Stratospheric Observatory for Infrared Astronomy, the Submillimeter Wave Astronomy Satellite, the Atacama Pathfinder Experiment, the Atacama Large Millimeter/submillimeter Array, and the JWST.…”
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97
EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
Published 2023-01-01“…The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) experiment will make new measurements from suborbital space as a precursor for future space missions that will address the challenge of the extremely low fluxes of ultra-high energy cosmic rays (UHECR) and very high energy (VHE) neutrinos. …”
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98
A Comprehensive Study of Soft X-ray Absorption Features in GX 13+1 Using XMM-Newton Observations
Published 2023-10-01“…In this study, a comprehensive analysis of the reflection grating spectrometer (RGS) data (energy range 0.33 keV to 2.5 keV) of GX 13+1 from the XMM-Newton space observatory was conducted. Numerous absorption lines have been described in earlier publications, although the majority of these investigations focused on the energy range between 3 keV and 10 keV. …”
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99
Observations of interacting galaxies NGC 2341 and NGC 2342 in X-ray band
Published 2018-12-01“…The source of information for this work is the XMM-Newton X-ray space observatory of ESA. According to this telescope observation results, the light curves and the emission spectrum of the objects of study were built. …”
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100
The Detection of UHECRs with the EUSO-TA Telescope
Published 2019-01-01“…EUSO-TA is a cosmic ray detector developed by the JEM-EUSO (Joint Experiment Missions for Extreme Universe Space Observatory) Collaboration, observing during nighttime the fluorescence light emitted along the path of extensive air showers in the atmosphere. …”
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