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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http://www.google.com/calendar/ical/omd8c03mppcl66der6js58v4nc%40group.calendar.google.com/public/basic.ics

Spitzer Scheduled Observations Calendar

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http://www.google.com/calendar/ical/hehldlqc0f6kvam8l0f7jkoiu0%40group.calendar.google.com/public/basic.ics

Ground-Based Observing Runs Calendar

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http://www.google.com/calendar/ical/2umveo5dlombvkdhqd9kve75lk%40group.calendar.google.com/public/basic.ics

Proposal Deadlines

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http://www.google.com/calendar/ical/hkid79pbume96cdf5tbeiti9s4%40group.calendar.google.com/public/basic.ics

Links of Interest:

NOAO Telescope list

Conferences and Meetings of Interest

To add this calendar to your iCal utility, please subscribe to it using this URL address that you need to cut and paste into your subscribe box:
http://www.google.com/calendar/ical/572afh6220p8fgdvcqlcmm9ias%40group.calendar.google.com/public/basic.ics

YSOVAR Team Members

Principal Investigator: John Stauffer
Institution: 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 2009

About 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.
PIDClusterCenterNotes
60014AFGL 49003:27:24 +58:44:00two FOVs, 3h27m08.00s,+58d44m55.0s and 3h27m17.00s,+58d50m40.0s
61020Ceph-C23:05:51 +62:30:55one FOV
61021GGD 12-1506:10:48 -06:12:30two FOVs, 6h10m45.00s,-6d12m30.0s and 6h10m58.00s,-6d10m00.0s
61022IC139621:36:29.81 +57:29:48.2one FOV
61023IRAS 20050+272020:07:04 +27:29:14.0one FOV
61024L168816:27:10 -24:37:30three FOVs, 16h26m28.00s,-24d23m05.0s and 16h27m29.10s,-24d40m56.0s, and 16h27m25.00s,-24d27m54.4s
61025Mon R206:07:48 -06:25:00one FOV.
61026NGC 133303:29:05.75 +31:19:30one FOV.
61027NGC2264-IRAS1206:41:04 +09:35:10one FOV.
61028Orion05:35:15 -05:21:00very big map; see AORs
61029Serpens Main18:29:59 +01:13:53one FOV
61030Serpens South18:30:03.7 -02:02:05.0one FOV