Development of the WFIRST Exoplanet Mass Measurement Method
This data set contains NIRC2 mosaics and photometry obtained during the KSMS Program “Development of the WFIRST Exoplanet Mass Measurement Method” lead by D. Bennett. These adaptive optics observations are follow-up images of the exoplanet host stars found by various microlensing surveys.
The tables below provide the information about each of the mosaic, as well as links to the papers in which they were used. For each mosaic (i.e., each row of a table) you can download the mosaic (mosaic link), a raw file that was used in the mosaic for getting any metadata information missing from the head of the mosaic file (raw file link), photometry of sources in the mosaic (photometry link). Clicking on the date of the mosaic queries KOA for all raw file observed for the relevant program on that night. The gzipped tar files under the data references contains the files link to in the Data column of the tables as well as ancillary data obtained from other telescopes.
OGLE-2005-BLG-071
Bennett et al 2020, AJ, 159, 68
Data Download (includes ancillary data): OB05071_data_products.tar.gz (17.2 MB)
| UT Date (Search) |
Program ID | Program PI | Filter | Camera | Mosaic Total Exp. Time (sec) | Data |
|---|---|---|---|---|---|---|
| 20190528 | N021 | Bennett | Ks | wide | 56 | mosaic raw file photometry |
| 20190528 | N021 | Bennett | Ks | narrow | 1380 | mosaic raw file photometry |
OGLE-2012-BLG-0950
Bhattacharya et al 2018, AJ, 156, 298
Data Download (includes ancillary data): OB120950_data_products.tar.gz (8.1 MB)
| UT Date (Search) |
Program ID | Program PI | Filter | Camera | Mosaic Total Exp. Time (sec) | Data |
|---|---|---|---|---|---|---|
| 20180523 | N027 | Bennett | Ks | narrow | 2280 | mosaic raw file photometry |
Macho 97-BLG-28
Blackman et al. 2020, ApJ, 890, 87
Data Download (includes ancillary data): Macho9728_data_products.tar.gz (27.7 MB)
| UT Date (Search) |
Program ID | Program PI | Filter | Camera | Mosaic Total Exp. Time (sec) | Data |
|---|---|---|---|---|---|---|
| 20130717 | N301N2L | Batista | J | narrow | 400 | mosaic raw file photometry |
| 20130717 | N301N2L | Batista | Ks | narrow | 400 | mosaic raw file photometry |
OGLE-2017-BLG-1434
Blackman et al. 2021, AJ, 161, 279
Data Download (includes ancillary data): OB171434_data_products.tar.gz (10.9 MB)
| UT Date (Search) |
Program ID | Program PI | Filter | Camera | Mosaic Total Exp. Time (sec) | Data |
|---|---|---|---|---|---|---|
| 20180807 | N139 | Bennett | Ks | wide | 450 | mosaic raw file photometry |
MOA-2010-BLG-477
Blackman et al. 2021, Nature, 598, 272
Data Download (includes ancillary data): MB10477_data_products.tar.gz (34.3 MB)
| UT Date | Program ID | Program PI | Filter | Camera | Mosaic Total Exp. Time (sec) | Data |
|---|---|---|---|---|---|---|
| 20150727 | N169N2L | Bennett | H | narrow | 300 | mosaic raw file photometry |
| 20150727 | N169N2L | Bennett | H | wide | 150 | mosaic raw file photometry |
| 20160805 | N067N2L | Bennett | H | narrow | 150 | mosaic raw file photometry |
| 20180523 | N027 | Bennett | H | narrow | 480 | mosaic raw file photometry |
| 20180523 | N027 | Bennett | Ks | narrow | 960 | mosaic raw file photometry |
MOA-2013-BLG-220
Vandorou et al. 2020, AJ, 160, 121
Data Download (includes ancillary data): MB13220_data_products.tar.gz (15 MB)
| UT Date | Program ID | Program PI | Filter | Camera | Mosaic Total Exp. Time (sec) | Data |
|---|---|---|---|---|---|---|
| 20130718 | N301N2L | Batista | Ks | wide | 660 | mosaic photometry |
| 20190527 | N021 | Bennett | Ks | narrow | 630 | mosaic photometry |
Please acknowledge the use of KOA by including this text in your publications:
This research has made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration.
Please also acknowledge the PI(s) of datasets that have been obtained through KOA, and please contact the KOA Help Desk if you publish archival data.
If your research uses data reduced by the DEIMOS, KCWI, MOSFIRE, or NIRES PypeIt DRP, please use the PypeIt Citation.
If your research uses data reduced by the KPF DRP, please use the citation as described in the README.md.
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