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Start Over Publisher NASA/IPAC Infrared Science Archive
91. Dust Around Nearby Stars
ID:
ivo://irsa.ipac/Herschel/Images/DUNES
Title:
Dust Around Nearby Stars
Short Name:
DUNES
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The DUst around NEarby Stars (DUNES, Eiroa et al. 2013) Herschel Open Time Key Program (KPOT_ceiroa_1) is a survey of 133 stars in 130 fields with the Herschel/PACS photometer. All target stars were observed with the PACS 100 and 160 micron filters. A subset of stars were additionally observed with the PACS 70 micron filter and the SPIRE 250, 350 and 500 micron filters.
92. Dust Around Nearby Stars (DUNES) Catalog
ID:
ivo://irsa.ipac/Herschel/Catalog/DUNES
Title:
Dust Around Nearby Stars (DUNES) Catalog
Short Name:
DUNES Catalog
Date:
01 Oct 2018 20:27:20
Publisher:
NASA/IPAC Infrared Science Archive
Description:
DUst around NEarby Stars (DUNES, Eiroa et al. 2013) is a Herschel open time deep key program to perform a deep and systematic survey for faint, cold debris disks. A sample of 133 nearby (d<25 pc) main sequence stars between 0.2 and 2 solar masses were observed with PACS and SPIRE. The DUNES catalog provides Herschel photometry, links to the Herschel images and SED plot, as well as quantities from ancillary data and other missions.
93. Dust in Nearby Galaxies with Spitzer (DUSTiNGS)
ID:
ivo://irsa.ipac/Spitzer/Images/DUSTiNGS
Title:
Dust in Nearby Galaxies with Spitzer (DUSTiNGS)
Short Name:
DUSTiNGS
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
DUSTiNGS consists of a sample of 50 dwarf galaxies within 1.5 Mpc, which have been mapped with IRAC channels 1 and 2 (3.6 and 4.5 microns). The sample consists of 37 dwarf spheroidal, 8 dwarf irregular, and 5 transition-type galaxies. The DUSTiNGS data release includes images and source catalogs based on uniform Spitzer 3.6 and 4.5 micron observations.
94. Dust in Nearby Galaxies with Spitzer (DUSTiNGS) Full Catalog
ID:
ivo://irsa.ipac/Spitzer/Catalog/DUSTiNGS/DUSTiNGS-Full
Title:
Dust in Nearby Galaxies with Spitzer (DUSTiNGS) Full Catalog
Short Name:
DUSTiNGS Full
Date:
01 Oct 2018 20:27:17
Publisher:
NASA/IPAC Infrared Science Archive
Description:
DUSTiNGS consists of a sample of 50 dwarf galaxies within 1.5 Mpc, which have been mapped with IRAC channels 1 and 2 (3.6 and 4.5 microns). The sample consists of 37 dwarf spheroidal, 8 dwarf irregular, and 5 transition-type galaxies. The DUSTiNGS data release includes images and source catalogs based on uniform Spitzer 3.6 and 4.5 micron observations. The catalogs are available in "full" and "good" versions, where quality cuts based on photometric accuracy and source morphology have been applied to the latter. See Boyer et al. (2015) for details.
95. Dust in Nearby Galaxies with Spitzer (DUSTiNGS) Good Source Catalog
ID:
ivo://irsa.ipac/Spitzer/Catalog/DUSTiNGS/DUSTiNGS-GSC
Title:
Dust in Nearby Galaxies with Spitzer (DUSTiNGS) Good Source Catalog
Short Name:
DUSTiNGS GSC
Date:
01 Oct 2018 20:27:17
Publisher:
NASA/IPAC Infrared Science Archive
Description:
DUSTiNGS consists of a sample of 50 dwarf galaxies within 1.5 Mpc, which have been mapped with IRAC channels 1 and 2 (3.6 and 4.5 microns). The sample consists of 37 dwarf spheroidal, 8 dwarf irregular, and 5 transition-type galaxies. The DUSTiNGS data release includes images and source catalogs based on uniform Spitzer 3.6 and 4.5 micron observations. The catalogs are available in "full" and "good" versions, where quality cuts based on photometric accuracy and source morphology have been applied to the latter. See Boyer et al. (2015) for details.
96. eHOPS Aquila SED Data Catalog
ID:
ivo://irsa.ipac/Herschel/Catalog/eHOPS/eHOPSAquilaPhot
Title:
eHOPS Aquila SED Data Catalog
Short Name:
eHOPSAquilaPhot
Date:
01 Apr 2023 01:07:05
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Extension of HOPS Out to 500 ParSecs (eHOPS) project used archival data to survey all the major star forming molecular clouds within 500 pc of the Sun, except Orion (which was surveyed by HOPS). The first eHOPS data release covers the Aquila molecular clouds (d ~ 436 pc). For every source detected in the Herschel/PACS bands, the eHOPS-Aquila catalog contains 1-850 micron SEDs assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data. A total of 172 protostars are found in Aquila, tightly concentrated in the molecular filaments that thread the clouds. Of these, 72 (42%) are Class 0 protostars, 53 (31%) Class I protostars, 43 (25%) are flat-spectrum protostars, and 4 (2%) are Class II sources. Ten of the Class 0 protostars are young PACS Bright Red Sources similar to those discovered in Orion. eHOPS compares the SEDs to a grid of radiative transfer models to constrain the luminosities, envelope densities, and envelope masses of the protostars.
97. eHOPS Aquila SED Fits Catalog
ID:
ivo://irsa.ipac/Herschel/Catalog/eHOPS/eHOPSAquilaFits
Title:
eHOPS Aquila SED Fits Catalog
Short Name:
eHOPSAquilaFits
Date:
01 Apr 2023 01:07:05
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Extension of HOPS Out to 500 ParSecs (eHOPS) project used archival data to survey all the major star forming molecular clouds within 500 pc of the Sun, except Orion (which was surveyed by HOPS). The first eHOPS data release covers the Aquila molecular clouds (d ~ 436 pc). For every source detected in the Herschel/PACS bands, the eHOPS-Aquila catalog contains 1-850 micron SEDs assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data. A total of 172 protostars are found in Aquila, tightly concentrated in the molecular filaments that thread the clouds. Of these, 72 (42%) are Class 0 protostars, 53 (31%) Class I protostars, 43 (25%) are flat-spectrum protostars, and 4 (2%) are Class II sources. Ten of the Class 0 protostars are young PACS Bright Red Sources similar to those discovered in Orion. eHOPS compares the SEDs to a grid of radiative transfer models to constrain the luminosities, envelope densities, and envelope masses of the protostars.
98. Euclid ERO
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.
99. Eureka LBNL Far-IR Lockman Hole (ELFLock) Maps
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.
100. Evolution of Interstellar Dust
ID:
ivo://irsa.ipac/Herschel/Images/SAG-4
Title:
Evolution of Interstellar Dust
Short Name:
SAG-4
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The goal of the "Evolution of interstellar dust" guaranteed time key project (PI: A. Abergel & A. Zavagno) is to explore with Herschel the far-infrared (FIR) to submillimeter (submm) emission properties of dust particles in a wide range of regions within our Galaxy, from very diffuse clouds to sites of star formation and proto-stars. Photometric data taken with SPIRE and PACS are complemented with spectroscopy using the FTS of SPIRE and PACS to derive the physical conditions of the gas from the lines of [CI], the high-level rotational lines of CO, and the major cooling lines of [CII] and [OI].