MilkyWay3D Dataverse

A collection of data that describe the 3D content of our Milky Way Galaxy. In 2022, the URL milkyway3d.org. will point not directly to this Dataverse, but instead to an interactive tool showing survey coverage in a 3D Milky Way. Please stay tuned!

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21 to 30 of 73 Results

Galactic Plane Infrared Polarization Survey (GPIPS) Dataverse(Harvard-Smithsonian Center for Astrophysics) Sep 5, 2016 The Galactic Plane Infrared Polarization Survey (GPIPS) covers 76 sq. deg in the Galactic midplane between 18° <= l <= 56° and -1° <= b <= +1°. It uses H-band (1.6 microns) linear polarimetry to determine magnetic field orientations in the plane of the sky near dense molecular clouds. The full GPIPS data set will contain almost 6 million stars, wit...
WISE Extended Observations: Continuum (2D) Sep 5, 2016 - Wide-Field Infrared Survey Explorer (WISE) Dataverse Edward Wright, 2016, "WISE Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/HXAXM6, Harvard Dataverse, V1 This dataset consists of mid-infrared photometric data in four bands (3.4, 4.6, 12, and 22 µm) over the entire sky. The ALLWISE image atlas contains 18,000+ four band calibrated 1.5x1.5 degree fits files, in addition to depth-of-coverage and noise maps. These atlas images were created by coadding almost 8 million single-exposure images. Individual...
WISE_Continuum_Data_Access.pdf Sep 5, 2016 - WISE Extended Observations: Continuum (2D) Adobe PDF - 27.6 KB - MD5: 3a0433e1e6818889ef0c715b91d02a44
Wide-Field Infrared Survey Explorer (WISE) Dataverse(Harvard-Smithsonian Center for Astrophysics) Sep 5, 2016 The Wide-Field Infrared Survey Explorer (WISE) maps the entire sky at mid-infrared wavelengths--3.4, 4.6, 12, and 22 microns—corresponding to an angular resolution of 6.1, 6.4, 6.5, and 12”. WISE achieves a 5σ point source sensitivity of better than 0.08, 0.11, 1, and 6 mJy for bands 1-4, which corresponds to Vega magnitudes of 16.5, 15.5, 11.2, an...
MIPSGAL Extended Observations: Continuum (2D) Sep 5, 2016 - MIPS Galactic Plane Survey (MIPSGAL) Dataverse Sean Carey, 2016, "MIPSGAL Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/BO5LL4, Harvard Dataverse, V1 This dataset consists of 24 & 70 micron maps covering latitudes -1° < b < +1° and longitudes l < 69° and l > 292°. Images are available for download via either an image cutout service (here) or by downloading the tiles directly at a specified data download link (here). In addition to the calibrated data, data products available include standard dev...
MIPSGAL_Continuum_Data_Access.pdf Sep 5, 2016 - MIPSGAL Extended Observations: Continuum (2D) Adobe PDF - 30.4 KB - MD5: c676ad3027d90ff7644ee26265c9f163
MIPS Galactic Plane Survey (MIPSGAL) Dataverse(Harvard-Smithsonian Center for Astrophysics) Sep 5, 2016 The MIPSGAL survey covers 278 sq. deg of the inner Galactic Plane at 24 μm (6” resolution) and 70 μm (18” resolution). It is meant to act as a longer wavelength component to the Spitzer-GLIMPSE Survey of the Galactic plane. Its two main science goals are to 1) identify high mass protostars and 2) probe properties of interstellar dust in the inner g...
Hi-GAL Extended Observations: Continuum (2D) Sep 5, 2016 - Herschel Infrared Galactic plane survey (Hi-GAL) Dataverse Sergio Molinari, 2016, "Hi-GAL Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/AGXXHR, Harvard Dataverse, V1 This dataset consists of photometric maps at five wavelengths: 70, 160, 250, 350 and 500μm, which combined cover the peak of the SED for dust temperatures between 8 ≤ T ≤ 50K. The first suite of Hi-GAL data was released in Spring 2016, covering 68°≥ l ≥ -70° and \|b\| ≤ 1°, with more data to come in future. The public Hi-GAL DR1 data can be retrieved...
HIGAL_Continuum_Data_Access.pdf Sep 5, 2016 - Hi-GAL Extended Observations: Continuum (2D) Adobe PDF - 28.6 KB - MD5: d1c0adaa38e46b39b1ca0acce58e49f6
Herschel Infrared Galactic plane survey (Hi-GAL) Dataverse(Harvard-Smithsonian Center for Astrophysics) Sep 5, 2016 The Herschel Infrared Galactic plane survey (Hi-GAL) is an unbiased photometric survey covering \|b\| <= 1.0°, 68 > l > -70° in five passbands between 70 and 500 μm. The nominal beam sizes range from 5-35". Its key science goals include understanding the distribution of the ISM temperature, the formation of molecular clouds, the timeline of high-mass...

Galactic Plane Infrared Polarization Survey (GPIPS) Dataverse(Harvard-Smithsonian Center for Astrophysics)

Sep 5, 2016

The Galactic Plane Infrared Polarization Survey (GPIPS) covers 76 sq. deg in the Galactic midplane between 18° <= l <= 56° and -1° <= b <= +1°. It uses H-band (1.6 microns) linear polarimetry to determine magnetic field orientations in the plane of the sky near dense molecular clouds. The full GPIPS data set will contain almost 6 million stars, wit...

WISE Extended Observations: Continuum (2D)

Sep 5, 2016 - Wide-Field Infrared Survey Explorer (WISE) Dataverse

Edward Wright, 2016, "WISE Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/HXAXM6, Harvard Dataverse, V1

This dataset consists of mid-infrared photometric data in four bands (3.4, 4.6, 12, and 22 µm) over the entire sky. The ALLWISE image atlas contains 18,000+ four band calibrated 1.5x1.5 degree fits files, in addition to depth-of-coverage and noise maps. These atlas images were created by coadding almost 8 million single-exposure images. Individual...

WISE_Continuum_Data_Access.pdf

Sep 5, 2016 - WISE Extended Observations: Continuum (2D)

Adobe PDF - 27.6 KB -

Wide-Field Infrared Survey Explorer (WISE) Dataverse(Harvard-Smithsonian Center for Astrophysics)

Sep 5, 2016

The Wide-Field Infrared Survey Explorer (WISE) maps the entire sky at mid-infrared wavelengths--3.4, 4.6, 12, and 22 microns—corresponding to an angular resolution of 6.1, 6.4, 6.5, and 12”. WISE achieves a 5σ point source sensitivity of better than 0.08, 0.11, 1, and 6 mJy for bands 1-4, which corresponds to Vega magnitudes of 16.5, 15.5, 11.2, an...

MIPSGAL Extended Observations: Continuum (2D)

Sep 5, 2016 - MIPS Galactic Plane Survey (MIPSGAL) Dataverse

Sean Carey, 2016, "MIPSGAL Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/BO5LL4, Harvard Dataverse, V1

This dataset consists of 24 & 70 micron maps covering latitudes -1° < b < +1° and longitudes l < 69° and l > 292°. Images are available for download via either an image cutout service (here) or by downloading the tiles directly at a specified data download link (here). In addition to the calibrated data, data products available include standard dev...

MIPSGAL_Continuum_Data_Access.pdf

Sep 5, 2016 - MIPSGAL Extended Observations: Continuum (2D)

Adobe PDF - 30.4 KB -

MIPS Galactic Plane Survey (MIPSGAL) Dataverse(Harvard-Smithsonian Center for Astrophysics)

Sep 5, 2016

The MIPSGAL survey covers 278 sq. deg of the inner Galactic Plane at 24 μm (6” resolution) and 70 μm (18” resolution). It is meant to act as a longer wavelength component to the Spitzer-GLIMPSE Survey of the Galactic plane. Its two main science goals are to 1) identify high mass protostars and 2) probe properties of interstellar dust in the inner g...

Hi-GAL Extended Observations: Continuum (2D)

Sep 5, 2016 - Herschel Infrared Galactic plane survey (Hi-GAL) Dataverse

Sergio Molinari, 2016, "Hi-GAL Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/AGXXHR, Harvard Dataverse, V1

This dataset consists of photometric maps at five wavelengths: 70, 160, 250, 350 and 500μm, which combined cover the peak of the SED for dust temperatures between 8 ≤ T ≤ 50K. The first suite of Hi-GAL data was released in Spring 2016, covering 68°≥ l ≥ -70° and |b| ≤ 1°, with more data to come in future. The public Hi-GAL DR1 data can be retrieved...

HIGAL_Continuum_Data_Access.pdf

Sep 5, 2016 - Hi-GAL Extended Observations: Continuum (2D)

Adobe PDF - 28.6 KB -

Herschel Infrared Galactic plane survey (Hi-GAL) Dataverse(Harvard-Smithsonian Center for Astrophysics)

Sep 5, 2016

The Herschel Infrared Galactic plane survey (Hi-GAL) is an unbiased photometric survey covering |b| <= 1.0°, 68 > l > -70° in five passbands between 70 and 500 μm. The nominal beam sizes range from 5-35". Its key science goals include understanding the distribution of the ISM temperature, the formation of molecular clouds, the timeline of high-mass...

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