YSOVAR
Young Stellar Object VARiability: Mid-Infrared Clues to Accretion Disk Physics and Protostar Rotational Evolution
YSOVAR
Young Stellar Object VARiability: Mid-Infrared Clues to Accretion Disk Physics and Protostar Rotational Evolution
Internal Team Page
YSOVAR Calendars
Spitzer Visibility Windows
Spitzer Scheduled Observations
Ground-based Observing Runs
Proposal Deadlines
Conferences and Meetings of Interest
Spitzer Visibility Windows Calendar
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Spitzer Scheduled Observations Calendar
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Ground-Based Observing Runs Calendar
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Proposal Deadlines
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Links of Interest:
NOAO Telescope list
Conferences and Meetings of Interest
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YSOVAR Team Members
Principal Investigator: John StaufferInstitution: Spitzer Science Center
Electronic mail: stauffer AT ipac DOT caltech DOT edu
Technical Contact: Luisa Rebull, Spitzer Science Center
Co-Investigators:
Rachel Akeson, NExScI
Lori Allen, CfA/NOAO
David Ardila, NHSC
David Barrado, LAEFF
Amelia Bayo, LAEFF
Jerome Bouvier, Obs. de Grenoble
Sean Carey, SSC
Nuria Calvet, Univ. Michigan
John Carpenter, Caltech
David Ciardi, NExScI
Kevin Covey, CfA
Fabio Favata, ESA
Kevin Flaherty, U. Arizona
Jan Forbrich, CfA
Sylvain Guieu, SSC
Rob Gutermuth, Smith College
Lee Hartmann, U. Michigan
Lynne Hillenbrand, Caltech
Joe Hora, CfA
David James, U. Hawaii
Mark McCaughrean, Exeter
Tom Megeath, U. Toledo
Giusi Micela, INAF
Maria Morales-Calderon, LAEFF
James Muzerolle, U. Arizona
Peter Plavchan, NExScI
Luisa Rebull, SSC
George Rieke, U. Arizona
Howard Smith, CfA
Mike Skrutskie, U. Virginia
Inseok Song, U. Georgia
Karl Stapelfeldt, JPL
Hwankyung Sung, SSC
Susan Terebey, CSULA
Fred Vrba, USNO
Alan Watson, UNAM
Mike Werner, JPL
Barbara Whitney, Space Science Institute
Elaine Winston, CfA
Kenny Wood, University of St. Andrews
Data Products
Observations of IC 1396 and Orion are being taken in Fall 2009About YSOVAR
YSOVAR is an Exploration Science program being conducted by the Spitzer Space Telescope during its warm mission with the InfraRed Array Camera (IRAC).Abstract from Proposal:
Spitzer/IRAC in the warm mission is the only facility now existing or planned capable of carrying out an extensive, accurate time series photometric monitoring survey of star-forming regions in the thermal infrared. The demonstrated sensitivity and stability of IRAC allows measurement of the relative fluxes of YSO's down to the substellar mass limit to 1-2% accuracy in star-forming regions out to >500 pc. We propose a time series monitoring exploration science survey of the Orion Nebula Cluster and 11 very young, populous embedded star-forming cores which will provide >= 80 epochs of data for > 1500 YSO's. We will complement these observations with contemporaneous optical and near-IR monitoring data in order to allow comparison of the phase, amplitude and light-curve shape as a function of wavelength. These data will allow us to:
(a) provide otherwise unobtainable constraints on the structure of the inner disks in Class I and II YSOs - and hence, perhaps, provide clues to the formation and migration of planets at young ages;
(b) measure the short and long-term stability of hot spots on the surfaces of YSO's of all evolutionary stages; and
(c) determine rotational periods for the largest sample to date of Class I YSO's and hence obtain the best measure of the initial angular momentum distribution of young stars.
The home page background image is used courtesy of NASA, JPL-Caltech, and L. Allen (Harvard-Smithsonian CfA).
Cluster Coordinates
IRAC arrays are ~5'x5', and these coordinates refer to the center of the IRAC field of view.| PID | Cluster | Center | Notes |
| 60014 | AFGL 490 | 03:27:24 +58:44:00 | two FOVs, 3h27m08.00s,+58d44m55.0s and 3h27m17.00s,+58d50m40.0s |
| 61020 | Ceph-C | 23:05:51 +62:30:55 | one FOV |
| 61021 | GGD 12-15 | 06:10:48 -06:12:30 | two FOVs, 6h10m45.00s,-6d12m30.0s and 6h10m58.00s,-6d10m00.0s |
| 61022 | IC1396 | 21:36:29.81 +57:29:48.2 | one FOV |
| 61023 | IRAS 20050+2720 | 20:07:04 +27:29:14.0 | one FOV |
| 61024 | L1688 | 16:27:10 -24:37:30 | three FOVs, 16h26m28.00s,-24d23m05.0s and 16h27m29.10s,-24d40m56.0s, and 16h27m25.00s,-24d27m54.4s |
| 61025 | Mon R2 | 06:07:48 -06:25:00 | one FOV. |
| 61026 | NGC 1333 | 03:29:05.75 +31:19:30 | one FOV. |
| 61027 | NGC2264-IRAS12 | 06:41:04 +09:35:10 | one FOV. |
| 61028 | Orion | 05:35:15 -05:21:00 | very big map; see AORs |
| 61029 | Serpens Main | 18:29:59 +01:13:53 | one FOV |
| 61030 | Serpens South | 18:30:03.7 -02:02:05.0 | one FOV |