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Space telescope

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

... Hubble Space Telescope (HST) and near-Jupiter spacecraft by Nichols et ...HST Space Telescope Imaging Spectrograph (STIS) for 47 orbits from 16 May to 18 July, primarily using ∼45 min time tag ...

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Spitzer space telescope measurements of dust reverberation lags in the Seyfert 1 galaxy NGC 6418

Spitzer space telescope measurements of dust reverberation lags in the Seyfert 1 galaxy NGC 6418

... CROSS-CORRELATION CODES RESULTS In an effort to give a comprehensive picture of the results obtained by different software packages used to determine the lag time between light curves we have included this appendix with ...

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Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno

... The detailed morphological response of the far-ultraviolet auroras to the interplane- tary medium has been examined previously using the Hubble Space Telescope (HST) and near-Jupiter spacecraft by Nichols ...

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A Spitzer Space Telescope Study of the Debris Disks around Four SDSS White Dwarfs

A Spitzer Space Telescope Study of the Debris Disks around Four SDSS White Dwarfs

... We present Spitzer Space Telescope data of four isolated white dwarfs that were previously known to harbor circumstellar gaseous disks. Infrared Array Camera photometry shows a significant infrared excess ...

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Chandra and Hubble Space Telescope observations of dark gamma ray bursts and their host galaxies

Chandra and Hubble Space Telescope observations of dark gamma ray bursts and their host galaxies

... We present a study of 21 dark gamma-ray burst (GRB) host galaxies, predominantly using X-ray afterglows obtained with the Chandra X-Ray Observatory (CXO) to pre- cisely locate the burst in deep Hubble Space ...

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A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

... The fi rst billion years are a crucial epoch in cosmic history. This is when the fi rst stars and galaxies formed and the universe underwent a major phase transition from a neutral to an ionized state. Our understanding of ...

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A New Method for Wide-field Near-IR Imaging with the Hubble Space Telescope

A New Method for Wide-field Near-IR Imaging with the Hubble Space Telescope

... We present a new technique for wide and shallow observations using the near-infrared channel of Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST). Wide-field near-IR surveys with HST are ...

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A `starless' core that isn't: detection of a source in the L1014 dense core with the Spitzer Space Telescope

A `starless' core that isn't: detection of a source in the L1014 dense core with the Spitzer Space Telescope

... We present observations of L1014, a dense core in the Cygnus region previously thought to be starless, but data from the Spitzer Space Telescope show the presence of an embedded source. We propose a model ...

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A Segmented aperture space telescope modeling tool and its application to remote sensing as understood through image quality and image utility

A Segmented aperture space telescope modeling tool and its application to remote sensing as understood through image quality and image utility

... aperture space telescope cannot be ...large telescope to be folded, placed within a launch vehicle, survive the launch without attaining additional aberrations, and then unfold once ...

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Hubble space telescope high-resolution imaging of Kepler small and cool exoplanet host stars

Hubble space telescope high-resolution imaging of Kepler small and cool exoplanet host stars

... Hubble Space Telescope imaging with the WFC3 of 23 stars that host particularly interesting Kepler planet candidates based on their small size and cool equilibrium temperature ...

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Identifying Galaxy Mergers with Quantitative Morphological Parameters in Simulated James Webb Space Telescope Images

Identifying Galaxy Mergers with Quantitative Morphological Parameters in Simulated James Webb Space Telescope Images

... In Kartaltepe et al. (2015), several classifiers make visual classifications of Hub- ble Space Telescope (HST) Cosmic Assembly Near-infrared Dark Energy Legacy Survey (CANDELS; Grogin et al. 2011; Koekemoer ...

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A Hubble Space Telescope transit light curve for GJ 436b

A Hubble Space Telescope transit light curve for GJ 436b

... Since the reported detection of transits for GJ 436b there have been a flurry of follow-up observations and analyses of the system. So far, published results include complete analyses (i.e. data reduction and light curve ...

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A Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations From Candels

A Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations From Candels

... We report the discovery of a Type Ia supernova (SN Ia) at redshift z = 1.55 with the infrared detector of the Wide Field Camera 3 (WFC3-IR) on the Hubble Space Telescope (HST). This object was discovered in ...

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A Lack of Planets in 47 Tucanae from a Hubble Space Telescope Search*

A Lack of Planets in 47 Tucanae from a Hubble Space Telescope Search*

... Hubble Space Telescope project to observe a significant ( ∼ 34,000) ensemble of main-sequence stars in the globular cluster 47 Tucanae with a goal of defining the frequency of inner orbit, gas giant ...

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Space Telescope and Optical Reverberation Mapping Project  VI  : reverberating disk models for NGC 5548

Space Telescope and Optical Reverberation Mapping Project VI : reverberating disk models for NGC 5548

... We see that the Swift points consistently yield f val- ues close to unity, indicating good agreement between the reverberating disk model and the data for these points. The fits to the HST light curves yield f factors ...

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Near-infrared Hubble Space Telescope polarimetry of a complete sample of narrow-line radio galaxies

Near-infrared Hubble Space Telescope polarimetry of a complete sample of narrow-line radio galaxies

... The HST observational details are presented in Table 1. The HST provides an actual spatial resolution of 0.22 arcsec (and a theoretical spatial resolution of 0.21 arcsec) at 2.05 µm. This is much better than achieved in ...

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Phase-resolved Hubble Space Telescope ultraviolet spectroscopy

Phase-resolved Hubble Space Telescope ultraviolet spectroscopy

... An important point to bear in mind here, however, is that it is not possible to reproduce the line profiles observed between phases 0.875 and 1.525 solely by superimposing a broad, varia[r] ...

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Hubble space telescope parallaxes of AM CVn stars and astrophysical consequences

Hubble space telescope parallaxes of AM CVn stars and astrophysical consequences

... in space density with Galactic height z = r sin b, ...local space density of ρ(0) = 2 × 10 −8 β −1 pc −3 for the short-period AM CVns that have high ...

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Space telescope and optical reverberation mapping project  I  Ultraviolet observations of the Seyfert 1 galaxy NGC 5548 with the cosmic origins spectrograph on Hubble Space Telescope

Space telescope and optical reverberation mapping project I Ultraviolet observations of the Seyfert 1 galaxy NGC 5548 with the cosmic origins spectrograph on Hubble Space Telescope

... To characterize the emission-line structure of NGC 5548 and guide our selection of continuum windows for our emission-line flux measurements, we fit a heuristic model to the lines and cont[r] ...

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A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae

A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae

... vations is presented in Fig. 10, combined with the masses to pro- vide an indication of the relative evolution of size with luminosity for our core-collapse transient host sample. The compact and low- mass nature of the ...

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