Searching for [CLC][ITAL]z[/ITAL][/CLC] ≃ 6 Objects with the [ITAL]Hubble Space Telescope[/ITAL] Advanced Camera for Surveys: Preliminary Analysis of a Deep Parallel Field

2003 ◽  
Vol 585 (2) ◽  
pp. L93-L96 ◽  
Author(s):  
Haojing Yan ◽  
Rogier A. Windhorst ◽  
Seth H. Cohen
2007 ◽  
Vol 172 (1) ◽  
pp. 196-202 ◽  
Author(s):  
A. M. Koekemoer ◽  
H. Aussel ◽  
D. Calzetti ◽  
P. Capak ◽  
M. Giavalisco ◽  
...  

2011 ◽  
Vol 195 (2) ◽  
pp. 18 ◽  
Author(s):  
D. J. Radburn-Smith ◽  
R. S. de Jong ◽  
A. C. Seth ◽  
J. Bailin ◽  
E. F. Bell ◽  
...  

1996 ◽  
Vol 158 ◽  
pp. 249-250
Author(s):  
E. M. Sion ◽  
M. Huang ◽  
F. H. Cheng ◽  
I. Hubeny ◽  
P. Szkody

AbstractWe present a preliminary analysis of the UV spectrum of the dwarf nova VW Hyi during early quiescence, obtained with the Faint Object Spectrograph (FOS) on the Hubble Space Telescope (HST). The data were obtained approximately one day after the end of a normal outburst.


2004 ◽  
Vol 213 ◽  
pp. 107-110
Author(s):  
William B. Sparks ◽  
John Krist ◽  
Mark Clampin ◽  
Holland Ford

The Advanced Camera for Surveys was installed on the Hubble Space Telescope in March 2002. The instrument science team will search for planets using direct imaging with the ACS coronagraph and with precise astrometric and photometric measurement of suitable stars and disks. The camera is operational and performing to expectation.


1996 ◽  
Vol 158 ◽  
pp. 223-224
Author(s):  
K. Schaefer ◽  
H. Bond ◽  
G. Chanmugam

We have used the High Speed Photometer (HSP) aboard the Hubble Space Telescope to observe the magnetic cataclysmic variables VV Pup, AM Her, and V834 Cen in the UV (1400…3300 Å) with 0.01 s time resolution. We detected low frequency flickering in all three systems, and compare the time-scales with the predictions of King (1989). At higher frequencies we searched for shock oscillations from the accretion column(s) in these systems. The data were analyzed using the Gabor transform wavelet-like technique (Heil & Walnut 1989) to search for frequency evolution throughout each observation. Preliminary analysis suggests the detection of rapid UV quasi-periodic oscillations (QPOs) in VV Pup at 0.74 Hz, and at 4.4 Hz in V834 Cen. As in ground based observations, our observations failed to yield any rapid QPOs in AM Her itself.


2005 ◽  
Vol 13 ◽  
pp. 171-172
Author(s):  
John P. Blakeslee

AbstractThe superior resolution and large format of the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST) make it a powerful new tool in the study of extra-galactic globular cluster (GC) systems. We summarize some early results on GC populations from the ACS GTO program, concentrating on the extreme cases of the isolated dwarf NGC 2915 and the core of the massive lensing cluster Abell 1689.


2004 ◽  
Vol 600 (2) ◽  
pp. L163-L166 ◽  
Author(s):  
Adam G. Riess ◽  
Louis-Gregory Strolger ◽  
John Tonry ◽  
Zlatan Tsvetanov ◽  
Stefano Casertano ◽  
...  

1992 ◽  
Vol 397 ◽  
pp. L35 ◽  
Author(s):  
I. R. King ◽  
J. M. Deharveng ◽  
R. Albrecht ◽  
C. Barbieri ◽  
J. C. Blades ◽  
...  

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