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HUBBLE-SPACE-TELESCOPE

Spectroscopy from the Hubble space telescope cosmic origins spectrogragh of the southern nova like BB Doradus in an intermedicate state

Spectroscopy from the Hubble space telescope cosmic origins spectrogragh of the southern nova like BB Doradus in an intermedicate state

... the Hubble Space Telescope Cosmic Origins Spectrograph ( HST / COS ) , as part of a 122 orbit HST / COS program to measure the WD effective temperature in CVs in the low state or ...

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Signature of Saturn's auroral cusp:simultaneous Hubble Space Telescope FUV observations and upstream solar wind monitoring

Signature of Saturn's auroral cusp:simultaneous Hubble Space Telescope FUV observations and upstream solar wind monitoring

... the Hubble Space Telescope (HST) was used to obtain the first image of the north aurora [Ge´rard et ...the Space Telescope Imaging Spectrograph (STIS) between 11 October 1997 and 29 ...

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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

... the Hubble Space Telescope ...the Hubble Ultra Deep Field, and followed as part of the CANDELS+CLASH Supernova project, comprising the SN search components from those two HST multi-cycle ...

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Accretion disk reverberation with Hubble Space Telescope observations of NGC 4593 : evidence for diffuse continuum lags

Accretion disk reverberation with Hubble Space Telescope observations of NGC 4593 : evidence for diffuse continuum lags

... The Seyfert 1 galaxy NGC 4593 was monitored spectroscopically with the Hubble Space Telescope as part of a reverberation mapping campaign that also included Swift, Kepler, and ground-based ...

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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 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 ...

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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 ...

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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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No neon, but jets in the remarkable recurrent nova M31N 2008 12a?   Hubble Space Telescope spectroscopy of the 2015 eruption

No neon, but jets in the remarkable recurrent nova M31N 2008 12a? Hubble Space Telescope spectroscopy of the 2015 eruption

... on Hubble Space Telescope Space Telescope Imaging Spectrograph ultraviolet spectroscopy taken within days of the predicted 2015 eruption, coupled with Keck spectroscopy of the 2013 ...

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The host galaxies and explosion sites of long duration gamma ray bursts: Hubble Space Telescope near infrared imaging

The host galaxies and explosion sites of long duration gamma ray bursts: Hubble Space Telescope near infrared imaging

... We present the results of a Hubble Space Telescope WFC3/F160W SNAPSHOT sur- vey of the host galaxies of 39 long-duration gamma-ray bursts (LGRBs) at z < 3. We have non-detections of hosts at the ...

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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*

... large 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 ...

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A Hubble Space Telescope transit light curve for GJ 436b

A Hubble Space Telescope transit light curve for GJ 436b

... In this paper we present an analysis of a transit light curve for GJ 436b obtained with the Fine Guidance Sensor (FGS) instru- ment on the Hubble Space Telescope (HST). Following the an- nouncement ...

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Hubble Space Telescope ultraviolet light curves reveal interesting properties of CC Sculptoris and RZ Leonis

Hubble Space Telescope ultraviolet light curves reveal interesting properties of CC Sculptoris and RZ Leonis

... The advantage of spectral data obtained in time-tag mode with the Hubble Space Telescope ( HST ) is that light curves can be constructed by summing the fl ux over wavelength. Thus, we were able to ...

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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

... here 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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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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Measurements of extragalactic background light from the far UV to the far IR from deep ground  and space based galaxy counts

Measurements of extragalactic background light from the far UV to the far IR from deep ground and space based galaxy counts

... of space-based facilities ( GALEX, Hubble Space Telescope ( HST ) , Spitzer, and Herschel ) and large ground-based facilities ( VLT, Subaru ) , deep fi eld data have now been obtained across ...

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Revision of earth-sized Kepler planet candidate properties with high-resolution imaging by the Hubble space telescope

Revision of earth-sized Kepler planet candidate properties with high-resolution imaging by the Hubble space telescope

... While the majority (>2000) of the Kepler planet candidates reside in apparently single-star systems, this percentage is likely due to a selection effect that avoids binary targets ( Kratter & Perets 2012 ) . ...

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EG and: Far ultraviolet spectroscopic explorer and Hubble space telescope STIS monitoring of an eclipsing symbiotic binary

EG and: Far ultraviolet spectroscopic explorer and Hubble space telescope STIS monitoring of an eclipsing symbiotic binary

... with space-based observation scheduling requirements, permitting a well-sampled data set over the binary orbital ...and Space Telescope Imaging Spectrograph (STIS) data it is possible to obtain high ...

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Relativistic deflection of background starlight measures the mass of a nearby white dwarf star

Relativistic deflection of background starlight measures the mass of a nearby white dwarf star

... the Hubble Space Telescope to measure the analogous process of astrometric microlensing caused by a nearby star, the white dwarf Stein 2051 ...

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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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MOA 2010 BLG 328Lb : a sub Neptune orbiting very Late M dwarf?

MOA 2010 BLG 328Lb : a sub Neptune orbiting very Late M dwarf?

... formally significant, this difference could also be caused by rather modest systematic errors and we found that the parallax is preferred rather than the xallarap. High angular resolution follow-up observations with the ...

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