Resource Type: Survey / Content Level: Research - STScI NAVO Directory Search Results

ID:: ivo://irsa.ipac/Bolocam/Images/Bolocam_LH
Title:: Bolocam Lockman Hole Map
Short Name:: Bolocam_LH
Date:: 23 May 2023 20:55:52
Publisher:: NASA/IPAC Infrared Science Archive
Description:: A deep 1.1 mm survey using Bolocam of the Lockman Hole, producing a map and galaxy candidate list. This survey encompasses 324 square arcmin to an rms noise level (filtered for point sources) of 1.4 mJy/beam. This project is described by Laurent et al., ApJ, 2005.

ID:: ivo://irsa.ipac/Bolocam/Images/Bolocam_Planck_SZ
Title:: Bolocam Planck SZ Cluster
Short Name:: Bolocam_PlanckSZ
Date:: 23 May 2023 20:55:52
Publisher:: NASA/IPAC Infrared Science Archive
Description:: Caltech Submillimeter Observatory data corresponding to 46 galaxy clusters which have been observed by Bolocam at 2.1mm.

ID:: ivo://irsa.ipac/Spitzer/Images/CosmicDawn
Title:: Cosmic Dawn
Short Name:: CosmicDawn
Date:: 07 Apr 2023
Publisher:: NASA/IPAC Infrared Science Archive
Description:: Cosmic Dawn is a new infrared survey covering the three Euclid deep fields and four other Euclid calibration fields using Spitzer's Infrared Array Camera (IRAC). These new observations are combined with all relevant IRAC archival data of these fields in order to produce the deepest possible mosaics of these regions. In total, these observations represent nearly 11% of the total Spitzer mission time. The resulting mosaics cover a total of approximately 71.5 deg^2 in the 3.6 and 4.5 micron bands, and approximately 21.8 deg^2 in the 5.8 and 8 micron bands. They reach at least 24 AB magnitude in the 3.6 micron band and up to ~5 mag deeper in the deepest regions. The astrometry is tied to the Gaia astrometric reference system, and the typical astrometric uncertainty for sources with 16 < [3.6] < 19 is 0.15". The photometric calibration is in excellent agreement with previous WISE measurements. Given that the Spitzer Space Telescope has now been decommissioned these mosaics are likely to be the definitive reduction of these IRAC data. This survey therefore represents an essential first step in assembling multi-wavelength data on the Euclid deep fields which are set to become some of the premier fields for extragalactic astronomy in the 2020s.

ID:: ivo://3CRSnapshots
Title:: 3CRSnapshots
Short Name:: 3CRSnap
Date:: 09 May 2019 11:36:55
Publisher:: 3CR Snapshot Team
Description:: The naming authority for the 3CRSnapshot resources managed at the Observatoire de Strasbourg

ID:: ivo://irsa.ipac/Spitzer/Images/Cygnus-X
Title:: Cygnus-X: A Spitzer Legacy Survey of the Cygnus-X Complex
Short Name:: Cygnus-X
Date:: 27 Oct 2022 19:00:00
Publisher:: NASA/IPAC Infrared Science Archive
Description:: The Cygnus-X region is one of the brightest regions of the sky at all wavelengths and one of the richest known regions of star formation of the Galaxy. The goals of the Cygnus-X survey are to provide a detailed picture of the processes that govern the evolution of massive star forming complexes, to study star formation in the massive star forming complex environment, and to provide a rich sample of intermediate to high mass protostars spanning the full range of protostellar evolution. The project will also allow us to assess the role of feedback in a massive OB star/molecular cloud complex. The survey imaged a ~24 square degree region centered near 20:30:25, +40:00 (J2000). The IRAC images had a median coverage of 3x12s high dynamic range (HDR) frames, and the MIPS data were taken in fast scanning mode in the 24 and 70 μm bands.

ID:: ivo://wfau.roe.ac.uk/denis-dsa
Title:: Deep Near Infrared Survey of the Southern Sky (DENIS)
Date:: 04 Dec 2019 13:34:37
Publisher:: WFAU, Institute for Astronomy, University of Edinburgh
Description:: Catalog of astrometry and photometry of detected point sources in the Far red optical (0.82-micron I-band) and near-infrared (1.25-micron J- and 2.15-micron Ks bands). ~16,700 square degrees of the southern sky

ID:: ivo://irsa.ipac/DSS/Images
Title:: Digitized Sky Survey
Short Name:: DSS
Date:: 27 Oct 2022 19:00:00
Publisher:: NASA/IPAC Infrared Science Archive
Description:: The Digitized Sky Survey (DSS) is a ground-based imaging survey of the entire sky in several colors. The survey, performed with Palomar and UK Schmidt telescopes, produced photographic plates that were later digitized at the Space Telescope Science Institute (STScI) to produce the Hubble Guide Stars Catalog (GSC). Each plate produced by the Survey covers 6.5 x 6.5 degrees of the sky, and the plates have been digitized using a modified PDS microdensitometer. The digital images have a pixel size of either 25 microns (1.7 arcsec per pixel) or 15 microns (1.0 arcsec per pixel), and are 14000 x 14000 or 23040 x 23040 pixels per side. The images are stored on 12-inch optical media and are difficult to access quickly.

ID:: ivo://vopdc.obspm/gepi/vopsat/esor
Title:: ESO-R Survey
Short Name:: ESO-R
Date:: 10 Nov 2022
Publisher:: Paris Astronomical Data Centre - GEPI
Description:: VO-compliant publication of Schmidt survey ESO-R of the southern sky digitized with the MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI).

ID:: ivo://irsa.ipac/Euclid/Images/ERO
Title:: Euclid ERO
Short Name:: Euclid_ERO
Date:: 18 Jun 2024 16:17:50
Publisher:: NASA/IPAC Infrared Science Archive
Description:: The ERO program is an initiative of the Euclid Science Team / ESA to collect 1 day of observations to showcase the Euclid mission and its capabilities before the start of the nominal survey. The ERO data products available at IRSA for the convenience of the US astronomy community are the same data products that are available through ESAC. The FITS files were processed with an ERO-specific pipeline, which is different from the standard Euclid pipeline that will be used for future data releases.

ID:: ivo://irsa.ipac/Spitzer/Images/ELFLock
Title:: Eureka LBNL Far-IR Lockman Hole (ELFLock) Maps
Short Name:: ELFLock
Date:: 26 Apr 2023 17:15:24
Publisher:: NASA/IPAC Infrared Science Archive
Description:: The Eureka Lawrence Berkeley National Laboratory (LBNL) Far-IR Lockman Hole (ELFLock) maps are intended to measure the Far-IR background radiation with 160-micron observations from the Multiband Imaging Photometer for Spitzer (MIPS). The download gives the largest contiguous low-cirrus 160 micron far-infrared map made with Spitzer data, covering 8.5 square degrees. It also differs from standard Spitzer-processed mosaic maps in that the background information is preserved, where it is normally removed by median filtering (for point-source studies). The map is composed of BCD data from S16 processing of data sets with these Spitzer Astronomical Observation Requests (AORs). Its flux units are MJy/Sr and the pixel size is 15.9", though flux = 0.0 for pixels without data.

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