# TESS Program G03147 Title: Asteroseismology Of Pre-Main Sequence Delta Scuti Stars PI: Zwintz, Konstanze - Universitat Innsbruck Type: SMALL Summary: Before TESS data became available, the field of asteroseismology was revolutionized by the high precision photometric time series obtained by the space missions MOST, CoRoT and Kepler. The main focus was lying on main sequence (MS) and post-MS stars, but first promising results were also achieved for the pre-MS stages. For a successful application of pre-MS asteroseismology we require the observational detection, resolution and identification of individual pulsation modes, and accurate theories of stellar structure and evolution. For many pre-MS delta Scuti stars, TESS is now the first space mission delivering high-quality, uninterrupted photometric time series which allows to tackle some of the open questions of early stellar evolution theory. # Sector 032 targets observed (2 min: 5, 20 s: 0) 11199521,84.5219,-1.256,9.51,G03147;G03255;G03252 264460023,81.1784,1.7301,9.9,G03147;G03252 24344701,79.002,-9.8098,9.74,G03147;G03255;G03252 332856261,84.4462,-6.7084,7.38,G03147;G03252 270577175,86.8212,-51.066,3.7,G03147;G03156;G03255;G03106;G03252;G_NONSTANDARDMASK;G_NOPHOTOMETRY;G_SPECIAL_APERTURE_25_25 # Sector 033 targets observed (2 min: 9, 20 s: 0) 234834875,97.7871,4.7909,10.38,G03147;G03252 234881632,98.0796,4.8158,11.89,G03147;G03252 220281554,99.8686,9.7011,9.96,G03147;G03255 220313579,100.0675,9.2869,11.4,G03147;G03252 220314268,100.0894,9.6974,10.39,G03147;G03252 220322393,100.2064,9.8897,11.23,G03147;G03252 220338578,100.3137,9.5211,9.62,G03147;G03252 231148059,100.4584,9.2658,11.0,G03147;G03255 270577175,86.8212,-51.066,3.7,G03147;G03156;G03255;G03106;G03252;G_NONSTANDARDMASK;G_NOPHOTOMETRY;G_SPECIAL_APERTURE_25_25 # Sector 034 targets observed (2 min: 2, 20 s: 0) 412746911,111.2047,-20.9797,14.75,G03147 270577175,86.8212,-51.066,3.7,G03147;G03156;G03255;G03106;G03252;G_NONSTANDARDMASK;G_NOPHOTOMETRY;G_SPECIAL_APERTURE_25_25 # Sector 035 targets observed (2 min: 4, 20 s: 0) 141905922,130.1275,-47.7397,11.1,G03147 93999747,130.6902,-48.0865,11.32,G03147;G03186 93999782,130.6933,-48.0904,9.4,G03147;G03186 180666191,129.3872,-39.5505,11.67,G03147 # Sector 036 targets observed (2 min: 6, 20 s: 0) 458429271,160.0046,-59.1794,14.54,G03147 463307248,153.396,-54.6047,10.62,G03147;G03255 464732841,156.8981,-57.6411,14.32,G03147 141905922,130.1275,-47.7397,11.1,G03147 93999747,130.6902,-48.0865,11.32,G03147;G03186 93999782,130.6933,-48.0904,9.4,G03147;G03186 # Sector 037 targets observed (2 min: 6, 20 s: 0) 436267771,193.4037,-60.4242,12.07,G03147 467279740,168.224,-60.7799,14.45,G03147 458429271,160.0046,-59.1794,14.54,G03147 463307248,153.396,-54.6047,10.62,G03147;G03255 323246150,130.4353,-79.048,7.25,G03147;G03255;G03202 323292655,130.8,-79.0699,5.83,G03147;G03265;G03255;G03251;G03252 # Sector 038 targets observed (2 min: 9, 20 s: 0) 436267771,193.4037,-60.4242,12.07,G03147 259722519,223.7606,-66.208,9.29,G03147 260721077,225.8077,-65.8917,11.01,G03147 455329806,228.854,-60.7589,12.24,G03147 357040880,180.0201,-78.193,6.35,G03147;G03255;G03251;G03252 357165560,181.7718,-78.7412,7.23,G03164;G03147;G03255;G03252 454961439,179.6457,-77.8255,6.56,G03147;G03255;G03251;G03252 323246150,130.4353,-79.048,7.25,G03147;G03255;G03202 323292655,130.8,-79.0699,5.83,G03147;G03265;G03255;G03251;G03252 # Sector 039 targets observed (2 min: 11, 20 s: 0) 70032020,241.6383,-39.2597,7.83,G03147;G03255;G03252 217302172,260.2108,-45.4211,7.2,G03147;G03252 102643324,263.7296,-32.5919,11.74,G03147;G03252 102643765,263.7021,-32.6226,12.11,G03147;G03252 259722519,223.7606,-66.208,9.29,G03147 260721077,225.8077,-65.8917,11.01,G03147 357040880,180.02,-78.193,6.35,G03147;G03255;G03251;G03252 357165560,181.7718,-78.7412,7.23,G03164;G03147;G03255;G03252 454961439,179.6457,-77.8255,6.56,G03147;G03255;G03251;G03252 323246150,130.4353,-79.048,7.25,G03147;G03255;G03202 323292655,130.8,-79.0699,5.83,G03147;G03265;G03255;G03251;G03252