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Дата изменения: Thu May 20 00:11:30 2010 Дата индексирования: Tue Oct 2 06:53:02 2012 Кодировка: |
10 April 2010:
Extremely deep 1.4 GHz VLA observations of GOODS-North
Glenn Morrison (IfA, U. Hawaii; CFHT) and colleagues have released extremely deep VLA 1.4 GHz
observations of the GOODS-North field. 165 hours of VLA observations in the A, B, C and D configurations
were combined to produce an image with RMS noise of 3.9 microJy per beam at phase center, one of the
deepest radio data observations ever made. The observations are described and source catalogs
are presented in Morrison et al. 2010, ApJ, 188, 178.
FITS data files are available at
data release.
02 March 2010:
VLT/ISAAC imaging of the Hubble Ultradeep Field
The GOODS ESO team has released
extremely deep K-band images of the Hubble Ultradeep Field.
The data products combine deep VLT/ISAAC K-band imaging obtained by Ivo Labbe and collaborators
with previous GOODS ISAAC K-band imaging in this area. The final image has a total exposure time
of 25.3 hours, with a net PSF FWHM of 0.36 arcsec, and reaches a median 5-sigma point source limiting
magnitude of 25.6, 0.67 mag deeper than the GOODS ISAAC K-band data alone. The image products are
available from the ESO Archive.
19 January 2010:
Hubble Space Telescope Multicycle Treasury Program for GOODS and other fields
A temporary web site briefly describes the project
and will be expanded in the future. In particular,
a detailed abstract
gives more information about the fields, filters and exposure times. This same abstact,
along with those of two other approved Multicycle Treasury Programs, is also
available at the STScI MCTP web site.
29 December 2009:
Gemini / FLAMINGOS-2 infrared spectroscopic survey of GOODS-South
22 December 2009:
First Herschel observations of the GOODS fields.
15 December 2009:
Second and final data release (v2.0) of VLT/VIMOS spectroscopy for GOODS-S
7 December 2009:
GOODS ISAAC data paper: Retzlaff et al. 2010, A&A, 511, 50
1 November 2009:
The CXC director's office has announced plans for an additional 2 Msec of Chandra exposure time
on the Chandra Deep Field South (CDF-S, including GOODS-S), which will increase the total exposure
time to 4 Msec. Observations are likely to be carried out in two parts, in Spring 2010 and 2011, respectively.
24 April 2009:
VLT/VIMOS U- and R-band imaging data products (v1.0) for GOODS-S
1 November 2008:
Public release of
Chandra Deep Field South 2 Msec data and catalogs
22 May 2008:
GOODS HST/ACS version 2.0 data release
18 February 2008:
First public release of VLT/VIMOS spectroscopy for GOODS-S.
16 January 2008:
GOODS-Herschel Open Time Key Program accepted!
31 October 2007:
Third and final release of VLT/FORS2 spectroscopic data products for GOODS-S.
10 September 2007:
Final (v2.0) release of VLT/ISAAC JHKs imaging for GOODS-S
1 September 2006:
Postdoc opportunities at NOAO
29 December 2005:
Third GOODS Spitzer data release (DR3):
24 December 2005:
Second release of VLT/FORS2 spectroscopic data products for GOODS-S.
1 December 2005:
GOODS postdoctoral position(s) at NOAO
27 September 2005:
GOODS observations of a candidate
massive post-starburst galaxy at z=6.5.
10 May 2005:
Second GOODS Spitzer data release (DR2):
9 February 2005:
First interim GOODS Spitzer data release (DR1+):
27 October 2004:
First GOODS Spitzer data release (DR1):
25 June 2004:
First release of VLT/FORS2 spectroscopic data products for GOODS-S.
24 June 2004:
GOODS IMAX Film released
1 June 2004:
Press release on GOODS Spitzer+HST+Chandra observations of hidden black holes
and optically invisible galaxies.
28 May 2004:
ESO and
ESA Press Releases on AVO/GOODS science:
Discovering missing black holes: First Science from a Virtual Observatory
24 May 2004:
v1.0 ESO/ISAAC GOODS data release
27 April 2004:
r1.1z GOODS ACS catalogs are now available.
22 December 2003:
r1.0z GOODS ACS catalogs are now available.
18 December 2003:
SIRTF renamed the Spitzer Space Telescope.
9 December 2003:More ESO/VLT FORS2 spectroscopy
1 December 2003: GOODS postdoctoral
positions
5 September 2003: ESO/VLT FORS2 spectroscopy.
4 September 2003:
First images with SIRTF/IRAC
4 September 2003:
GOODS publications
29 August 2003:
V1.0 GOODS HST/ACS Data
Release
25 August 2003: SIRTF is up!
20 June 2003: GOODS in the news!
6 June 2003:
Version v0.5 release
27 May 2003:
GOODS transient search results
8 October 2002:
The GOODS team congratulates
Co-Investigator Riccardo Giacconi on the
award of the 2002 Nobel Prize in Physics for
his pioneering work on X-Ray astrophysics.
7 October 2002:
Version v0.5 data release begun with Epoch-1, reduced B, V, i, z ACS images in the CDF-S. Release information available here.
25 September 2002:
First CDF-S ACS transient search successfully completed.
9 April 2002:
ESO VLT/ISAAC CDF-S near-infrared data (version 0.5) release
9 April 2002:
CTIO 4m/MOSAIC CDF-S U-band data (version 0.5) release
15 March 2002:
SIRTF spacecraft and cryogenic telescope assembly
mated together....we have an observatory!
6 December 2001: GOODS HST Treasury Program approved.
3 October 2001:
SIRTF Astronomical Observing Requests (AORs) submitted. These are the "phase 2"
formatted instructions for the detailed structure of SIRTF observations.
They will be used by the SSC to implement and schedule the GOODS program.
14 February 2001:
First KPNO 4m FLAMINGOS
observations for GOODS!
17 November 2000:
The GOODS proposal was approved for the SIRTF Legacy program.
Two proposals for very large, multi-year programs of Hubble Space Telescope observations
of GOODS and other cosmological survey fields have been jointly approved, with a total
observing time of 902 orbits. The project will survey the rest-frame optical wavelength
properties of galaxies at 1.5 < z < 3, make a census of star-forming galaxies at 6 < z < 9,
and will detect type Ia supernovae at z > 1.5 for cosmological studies.
Drs. Sandra Faber (University of California Santa Cruz)
and Harry Ferguson (STScI) are the co-PIs for the merged program, which will use the
Wide Field Camera 3 infrared channel (WFC3-IR), as well as the Advanced Camera for Surveys
(ACS) optical imager, to obtain data in five fields: GOODS-North and -South, the Extended
Groth Strip (EGS), the UK Infrared Deep Sky Survey (UKIDSS) Ultra-Deep Survey (UDS) field,
and the Cosmic Evolution Survey (COSMOS) field. A total solid angle of approximately
900 square arcminutes will be surveyed with deep near-infrared J- and H-band WFC3-IR imaging.
Additionally, about 40% of the GOODS area will be imaged to substantially deeper limits,
and in the Y-band (1.05 micron) filter as well, enabling the identification and study of
very high redshift galaxies. GOODS-North is in the HST Continuous Viewing Zone,
enabling ultraviolet observations in that field with the WFC3-UVIS channel. Distant
supernovae detected in the WFC3-IR imaging will be followed up with a combination
of grism spectroscopy and photometric monitoring of their light curves.
Mark Dickinson (NOAO) and Anthony Gonzalez (Univ. Florida) are co-PIs for an NOAO Survey Program
to obtain near-infrared spectra of 1000 galaxies in GOODS-South with the
FLAMINGOS-2 multi-object spectrograph
(see also the UF F2 web site) at the
Gemini-South observatory.
The NOAO Survey Program will be supplemented by additional guaranteed time granted to the FLAMINGOS-2
principal investigator, Steve Eikenberry (UF). This will be the first large-scale near-infrared
spectroscopic survey of high redshift galaxies and is designed to measure redshifts and nebular line
diagnostics for galaxies and AGN primarily at 1.4 < z < 2.5. The observations will be carried out over
two years in 2010 and 2011.
Early observations from the Herschel Space Observatory were presented at a workshop
in Madrid, Spain on 17-18 December 2009. The GOODS-North field was observed during
Science Demonstration Phase observations by both the PACS and SPIRE instrument teams
as part of their guaranteed time programs.
Presentations from the workshop
include images and early scientific results for GOODS-N:
See Balestra et al., A&A, in press
This data paper describes the deep near-infrared imaging of GOODS-S with VLT ISAAC.
Reduced public data products are available at
the ESO GOODS web site
See Nonino et al. 2009
See Luo et al. 2008
The new v2.0 images incorporate additional ACS data taken as part of the continued
search for high redshift in HST Cycles 12 and 13. The new data increase the exposure time
in the F850LP band by factors of 2.3 and 1.7 in GOODS-N and -S, respectively,
with more modest increments in F775W and F606W as well. Catalogs (r2.0z) are also available,
as well as a new ACS cutout image server.
David Elbaz (CEA/Saclay) is PI for an open time Key Program of far-infrared obserations of the GOODS fields
using the Herschel Space Observatory, whose launch is planned for later in 2008. The program has been
awarded 362.6 hours of Herschel observing time, and consists of the following components:
The "superdeep" observations of GOODS-S match the exposure times planned for the equivalent program on GOODS-South
in the Guaranteed Time Key Programs (PACS and HerMES). The "ultradeep" observations will cover a portion
of GOODS-S with PACS with the longest exposure times and faintest flux limits planned for the observatory.
See Vanzella et al., 2008, A&A 478, 83,
The Great Observatories Origins Deep Survey. VLT/FORS2 spectroscopy in the GOODS-South Field: Part III
Two or more postdoc positions for (1) new post-GOODS far-infrared (MIPS)
Spitzer Legacy survey of the ECDFS and EGS; (2) "inter-survey" research
combining data from GOODS, the new MIPS Legacy survey, NDWFS/Bootes, etc.
Application deadline: 31 Oct 2006; however, early applications will be
considered immeditely for the Spitzer Legacy positions.
IRAC "superdeep" images for second-epoch observations of both GOODS fields
See Vanzella et al., 2006, A&A 454, 423,
The Great Observatories Origins Deep Survey. VLT/FORS2 spectroscopy in the GOODS-South Field: Part II
One or more postdoc positions working on GOODS and other surveys,
with Mark Dickinson at NOAO.
Press releases from the
Spitzer Science
Center and
Space Telescope Science Institute
MIPS 24 micron images and source lists for GOODS-S, and new (v0.3)
rereductions of IRAC images for GOODS-S.
MIPS 24 micron images and source lists for GOODS-N
IRAC "superdeep" images for first-epoch observations of both GOODS fields
See Vanzella et al., 2005, A&A 434, 53,
The Great Observatories Origins Deep Survey. VLT/FORS2 spectroscopy in the GOODS-South Field
See README file for a detailed explanation.
See README file for a detailed explanation.
See
early release images and press information
Updated/expanded release of redshifts and spectra from the
GOODS ESO spectroscopic campaign.
One or more postdoc positions working on GOODS, especially SIRTF
data, with Mark Dickinson at NOAO.
First data release from the
GOODS ESO spectroscopic campaign.
Papers by the GOODS team and from others in the astronomical community
using GOODS data.
Mosaicked stacks combining all 5 epochs of observation are available
for ftp.
See README
file for more details and this NOTE
on current availability and updates.
See
pictures of launch
and regular updates on mission status at the
SIRTF Science Center web pages
See
STScI press release on HST + Chandra observations, and reports at
CNN,
NY Times,
and elswhere.
CDF-S Epochs 1-5 and HDF-N Epoch 1-4, B,V,i & z have been released and are available to the public. The v0.5 data release will be complete 7/19/03 with the release of HDF-N Epoch 5.
The full complement of eight transient searches has been completed and public results are posted here.
In HST Cycle 11, the GOODS team will carry out a large
observing program of deep, multicolor, optical imaging of
the GOODS fields using the
Advanced Camera for Surveys. The program will image
the GOODS fields in four filters to "near-HDF" depths,
repeating the observations in several epochs in order to
search for very distant supernovae.
Announcements, press releases and articles:
Copyright © 2009 The Association of Universities for
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