The Advanced Camera for the Hubble Space Telescope

被引:204
|
作者
Ford, H
Bartko, F
Bely, P
Broadhurst, T
Burrows, C
Cheng, E
Clampin, M
Crocker, J
Feldman, P
Golimowski, D
Hartig, G
Illingworth, G
Kimble, R
Lesser, M
Miley, G
Neff, S
Postman, M
Sparks, W
Tsvetanov, Z
White, R
Sullivan, P
Krebs, C
Leviton, D
LaJeunesse, T
Burmester, B
Fike, S
Johnson, R
Slusher, B
Volmer, P
Woodruff, B
机构
关键词
D O I
10.1117/12.324464
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Advanced Camera for the Hubble Space Telescope has three cameras. The first, the Wide Field Camera, will be a high-throughput (44% at 600 nm, including the HST OTA), wide field (200 " x204 "), 4096 x 4096 pixel CCD optical and I-band camera that is half-critically sampled at 500 nm. The second, the High Resolution Camera (HRC), is a 1024 x 1024 pixel CCD camera that is critically sampled at 500 nm. The HRC has a 26 " x29 " field of view and 29% throughput at 250 nm. The HRC optical path includes a coronagraph that will improve the HST contrast near bright objects by a factor of similar to 10 at 900 nm. The third camera, the Solar-Blind Camera, is a far-ultraviolet, pulse-counting array that has a relatively high throughput (6% at 121.6 nm) over a 26 " x29 " field of view. The Advanced Camera for Surveys (ACS) will increase HST's capability for surveys and discovery by a factor of similar to 10 at 800 nm. The ACS science team will use similar to 60% of its dedicated time to make deep surveys of 15 clusters of galaxies at redshifts between 0.2 and 2. We will map the large-scale distribution of dark matter around two low redshift rich clusters and investigate the evolution of galaxies and clusters of galaxies between redshifts of 0.5 and 1. We will study young galaxies and clusters of galaxies in fields centered on high-redshift radio galaxies. HRC images of an unbiased sample of early-type galaxies will be searched for small (r similar to 100 pc) nuclear disks; subsequent spectroscopic observations of the disks will be used to measure the central masses to determine if massive black holes are present. We will use the HRC coronagraph to take broad-band, narrow-band, and polarimetric images of quasars and BL Lacs at redshifts between 0.2 and 0.5. We will use a novel polarimetric technique to measure geometric distances to galaxies and provide independent measures of H-0. The coronagraph will be used to search nearby stars for proto-planetary disks, brown dwarf companions, and planets.
引用
收藏
页码:234 / 248
页数:15
相关论文
共 50 条
  • [1] The Advanced Camera for the Hubble Space Telescope
    Ford, H
    Feldman, P
    Golimowski, D
    Tsvetanov, Z
    Bartko, F
    Crocker, J
    Bely, P
    Brown, R
    Burrows, C
    Clampin, M
    Hartig, G
    Postman, M
    Rafal, M
    Sparks, W
    White, R
    Broadhurst, T
    Illingworth, G
    Kelly, T
    Woodruff, B
    Cheng, E
    Kimble, R
    Krebs, C
    Neff, S
    Lesser, M
    Miley, G
    SPACE TELESCOPES AND INSTRUMENTS IV, 1996, 2807 : 184 - 196
  • [2] The advanced camera for surveys coronagraph on the Hubble Space Telescope
    Krist, J
    Hartig, G
    Clampin, M
    Golimowski, D
    Ford, H
    Illingworth, G
    HIGH-CONTRAST IMAGING FOR EXO-PLANET DETECTION, 2003, 4860 : 20 - 31
  • [3] Detection of planets with the Hubble Space Telescope Advanced Camera for surveys
    Sparks, WB
    Brown, R
    Burrows, C
    Clampin, M
    Krist, JE
    Ford, H
    Feldman, PD
    Golimowski, D
    BIOASTRONOMY'99, A NEW ERA IN BIOASTRONOMY, PROCEEDINGS, 2000, 213 : 131 - +
  • [4] Planet detection using the Advanced Camera for Surveys on the Hubble Space Telescope
    Sparks, WB
    Krist, J
    Clampin, M
    Ford, H
    BIOASTRONOMY 2002: LIFE AMONG THE STARS, 2004, (213): : 107 - 110
  • [5] The photometric performance and calibration of the Hubble Space Telescope Advanced Camera for Surveys
    Sirianni, M
    Jee, MJ
    Benítez, N
    Blakeslee, JP
    Martel, AR
    Meurer, G
    Clampin, M
    De Marchi, G
    Ford, HC
    Gilliland, R
    Hartig, GF
    Illingworth, GD
    Mack, J
    McCann, WJ
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2005, 117 (836) : 1049 - 1112
  • [6] Slitless grism spectroscopy with the Hubble Space Telescope advanced camera for surveys
    Pasquali, A
    Pirzkal, N
    Larsen, S
    Walsh, JR
    Kümmel, M
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2006, 118 (840) : 270 - 287
  • [7] Hubble Space Telescope advanced camera for surveys narrowband imaging of the Kepler supernova remnant
    Sankrit, Ravi
    Blair, William P.
    Frattare, Lisa M.
    Rudnick, Lawrence
    DeLaney, Tracey
    Harrus, Ilana M.
    Ennis, Jessica A.
    ASTRONOMICAL JOURNAL, 2008, 135 (02): : 538 - 547
  • [8] HUBBLE SPACE TELESCOPE/ADVANCED CAMERA FOR SURVEYS CONFIRMATION OF THE DARK SUBSTRUCTURE IN A520
    Jee, M. J.
    Hoekstra, H.
    Mahdavi, A.
    Babul, A.
    ASTROPHYSICAL JOURNAL, 2014, 783 (02):
  • [9] Calibration of Hubble Space Telescope advanced camera for surveys emission-line filters
    O'Dell, CR
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2004, 116 (822) : 729 - 733
  • [10] The COSMOS survey:: Hubble Space Telescope advanced camera for surveys observations and data processing
    Koekemoer, A. M.
    Aussel, H.
    Calzetti, D.
    Capak, P.
    Giavalisco, M.
    Kneib, J.-P.
    Leauthaud, A.
    Le Fevre, O.
    McCracken, H. J.
    Massey, R.
    Mobasher, B.
    Rhodes, J.
    Scoville, N.
    Shopbell, P. L.
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2007, 172 (01): : 196 - 202