- Home
- Search Results
- Page 1 of 1
Search for: All records
-
Total Resources2
- Resource Type
-
0000000002000000
- More
- Availability
-
20
- Author / Contributor
- Filter by Author / Creator
-
-
Beane, Angus (1)
-
Bonaca, Ana (1)
-
Cargile, Phillip A (1)
-
Conroy, Charlie (1)
-
Dotter, Aaron (1)
-
Eadie, Gwendolyn (1)
-
Eisenstein, Daniel J (1)
-
El-Badry, Kareem (1)
-
Finkbeiner, Douglas P (1)
-
Goodman, Alyssa A (1)
-
Green, Gregory M (1)
-
Han, Jiwon Jesse (1)
-
Hawkins, Keith (1)
-
Ji, Alexander (1)
-
Johnson, Benjamin D (1)
-
Kamdar, Harshil (1)
-
Kamdar, Harshil M (1)
-
Naidu, Rohan (1)
-
Nelson, Tyler (1)
-
Rix, Hans-Walter (1)
-
- Filter by Editor
-
-
& Spizer, S. M. (0)
-
& . Spizer, S. (0)
-
& Ahn, J. (0)
-
& Bateiha, S. (0)
-
& Bosch, N. (0)
-
& Brennan K. (0)
-
& Brennan, K. (0)
-
& Chen, B. (0)
-
& Chen, Bodong (0)
-
& Drown, S. (0)
-
& Ferretti, F. (0)
-
& Higgins, A. (0)
-
& J. Peters (0)
-
& Kali, Y. (0)
-
& Ruiz-Arias, P.M. (0)
-
& S. Spitzer (0)
-
& Sahin. I. (0)
-
& Spitzer, S. (0)
-
& Spitzer, S.M. (0)
-
(submitted - in Review for IEEE ICASSP-2024) (0)
-
-
Have feedback or suggestions for a way to improve these results?
!
Note: When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher.
Some full text articles may not yet be available without a charge during the embargo (administrative interval).
What is a DOI Number?
Some links on this page may take you to non-federal websites. Their policies may differ from this site.
-
Abstract We presentAugustus, a catalog of distance, extinction, and stellar parameter estimates for 170 million stars from 14 mag <r< 20 mag and with ∣b∣ > 10° drawing on a combination of optical to near-infrared photometry from Pan-STARRS, 2MASS, UKIDSS, and unWISE along with parallax measurements from Gaia DR2 and 3D dust extinction maps. After applying quality cuts, we find 125 million objects have “high-quality” posteriors with statistical distance uncertainties of ≲10% for objects with well-constrained stellar types. This is a substantial improvement over the distance estimates derived from Gaia parallaxes alone and in line with the recent results from Anders et al. We find the fits are able to reproduce the dereddened Gaia color–magnitude diagram accurately, which serves as a useful consistency check of our results. We show that we are able to detect large, kinematically coherent substructures in our data clearly relative to the input priors, including the Monoceros Ring and the Sagittarius Stream, attesting to the quality of the catalog. Our results are publicly available at doi:10.7910/DVN/WYMSXV. An accompanying interactive visualization can be found athttp://allsky.s3-website.us-east-2.amazonaws.com.more » « less
-
Nelson, Tyler; Ting, Yuan-Sen; Hawkins, Keith; Ji, Alexander; Kamdar, Harshil; El-Badry, Kareem (, The Astrophysical Journal)
An official website of the United States government

Full Text Available