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.

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1 to 10 of 59 Results
The Radcliffe Wave Is Oscillating(Harvard University)
Feb 20, 2024MilkyWay3D Dataverse
SMOG_CfA Dataverse(Center for Astrophysics | Harvard & Smithsonian)
Aug 8, 2019
CfA OIR project on the Spitzer Mapping of the Outer Galaxy (SMOG) field related to paper: A Census of Star Formation in the Outer Galaxy: The SMOG Field by E Winston, J Hora, R Gutermuth, V Tolls, ApJ, 2019, 880, 9 https://iopscience.iop.org/article/10.3847/1538-4357/ab27c8/pdf We include here the 7x3 degree mosaics of the full SMOG field for IRAC...
Cepheus-L1251 Dataverse(University of Victoria)
Oct 16, 2017Green Bank Ammonia Survey Dataverse
GAS DR1 Dataverse(University of Toronto)
Mar 24, 2017Green Bank Ammonia Survey Dataverse
GBT NH3 maps for L1495-B218 Dataverse(MPE)
Oct 12, 2016Green Bank Ammonia Survey Dataverse
These are the data used in Seo et al. (2015, http://adsabs.harvard.edu/abs/2015ApJ...805..185S)
Bar And Spiral Structure Legacy (BeSSeL) Survey Dataverse(Harvard-Smithsonian Center for Astrophysics)
Sep 25, 2016MilkyWay3D Dataverse
The BeSSeL Survey is a Very Long Baseline Array (VLBA) key science project whose goal is to study the kinematics and spiral structure of the Milky Way Galaxy. They do this by measuring the trigonometric parallaxes and proper motions of masers associated with high-mass star forming regions throughout the Galaxy. The main maser emission lines include...
The Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) Dataverse(Harvard-Smithsonian Center for Astrophysics)
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...
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...
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...
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...
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