This is the Astronomy data repository at Harvard. It is currently open to all scientific data from astronomical institutions worldwide. Administration and support is provided by the Harvard-Smithsonian Center for Astrophysics (CfA) in collaboration with Harvard Library (HL) and the Institute for Quantitative Social Science (IQSS). Infrastructure is provided by Harvard University Information Technology Services.

The Astronomy Dataverse Network plays an important role in fulfilling your Data Management Plan requirements (e.g. as mandated by NSF), and for providing data re-use and citation opportunities. Find out more about our team by exploring the Seamless Astronomy and Wolbach Library teams at the CfA. We are also connecting the Astronomy Dataverse to the indexing services provided by the SAO/NASA Astrophysical Data Service (ADS).
Featured Dataverses

In order to use this feature you must have at least one published or linked dataverse.

Publish Dataverse

Are you sure you want to publish your dataverse? Once you do so it must remain published.

Publish Dataverse

This dataverse cannot be published because the dataverse it is in has not been published.

Delete Dataverse

Are you sure you want to delete your dataverse? You cannot undelete this dataverse.

Advanced Search

31 to 40 of 215 Results
Sep 5, 2016MilkyWay3D Dataverse
The Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) is composed of several individual surveys and together they provide almost complete longitudinal coverage of the Galactic plane at |b| <= 1.0°. Most of the plane is imaged at a spatial resolution of <2” at wavelengths of 3.6, 4.5, 5.8, and 8.0 μm; however, certain longitudes in...
Sep 5, 2016 - UKIRT Infrared Deep Sky Galactic Plane Survey (UKIDSS-GPS) Dataverse
Phil Lucas, 2016, "UKIDSS-GPS Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/G43KCK, Harvard Dataverse, V1
This dataset consists of near-infrared photometric maps (J, H, and K bands) in a wide strip covering all the first quadrant and sections of both the second and third quadrants. As of Summer 2016, the most recent publicly available data release is UKIDSS DR10, with more data to become available in future. The cutout service includes the option to ex...
UKIRT Infrared Deep Sky Galactic Plane Survey (UKIDSS-GPS) Dataverse(Harvard-Smithsonian Center for Astrophysics)
Sep 5, 2016MilkyWay3D Dataverse
The UKIRT Infrared Deep Sky Galactic Plane Survey (UKIDSS-GPS) is a near infrared survey which will map over 1800 square degrees of the Galactic plane in J,H,K bands (1-3 μm) to a depth of 19 magnitudes. It is a successor to the 2MASS survey, probing 3 magnitudes deeper. The GPS plans to map half the plane over the following regions: 141° < l < 230...
Sep 5, 2016 - Galactic Plane Infrared Polarization Survey (GPIPS) Dataverse
Dan Clemens, 2016, "GPIPS Extended Observations: Polarimetry (2D)", https://doi.org/10.7910/DVN/QYVXUP, Harvard Dataverse, V1
This dataset consists of 76 sq. deg. of H-band (1.6 μm) linear polarimetry observations, which are able to reveal the plane-of-the-sky magnetic field orientations. Data products include 3237 overlapping 10 × 10 arcmin fields, which are downloadable in 1.7 GB zip files here.
Galactic Plane Infrared Polarization Survey (GPIPS) Dataverse(Harvard-Smithsonian Center for Astrophysics)
Sep 5, 2016MilkyWay3D Dataverse
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...
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...
Wide-Field Infrared Survey Explorer (WISE) Dataverse(Harvard-Smithsonian Center for Astrophysics)
Sep 5, 2016MilkyWay3D Dataverse
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...
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...
MIPS Galactic Plane Survey (MIPSGAL) Dataverse(Harvard-Smithsonian Center for Astrophysics)
Sep 5, 2016MilkyWay3D Dataverse
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...
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...
Add Data

Sign up or log in to create a dataverse or add a dataset.

Share Dataverse

Share this dataverse on your favorite social media networks.

Link Dataverse
Reset Modifications

Are you sure you want to reset the selected metadata fields? If you do this, any customizations (hidden, required, optional) you have done will no longer appear.