Extragalactic abstracts - IRSA - California Institute of Technology

More documents

Recommendations

Info

Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 235/742 Spitzer Space Telescope − General Observer Proposal #20389 The Environmental Dependence of Galaxy Star Formation Rates Principal Investigator: Vandana Desai Institution: Caliornia Institue of Technology Technical Contact: Vandana Desai, Caliornia Institue of Technology Co−Investigators: Alfonso Aragon−Salamanca, University of Nottingham Philip Best, Royal Observatory Edinburgh Douglas Clowe, Steward Observatory Julianne Dalcanton, University of Washington Gabriella De Lucia, Max−Planck Institut fuer Astrophysik Rose Finn, University of Massachusetts Claire Halliday, Max−Planck Institut fuer Astrophysik Pascale Jablonka, GEPI, Observatoire de Paris−Meudon Bo Milvang−Jensen, Max Planck Institute fur extraterrestrische Physik Bianca Poggianti, Osservatorio Astronomico di Padova Gregory Rudnick, NOAO Charlot Stephane, Max−Planck Institut fuer Astrophysik Dennis Zaritsky, Steward Observatory Science Category: high−z galaxies (z>0.5) Observing Modes: MipsScan Hours Approved: 7.4 Abstract: We are requesting 29.6 hours of observations with MIPS in order to study the star formation rates of galaxies out to the infall regions (30’x30’) of 4 well−studied high redshift (z = 0.8) clusters from the ESO Distant Cluster Survey (EDisCS). These observations will provide star formation rates that are unbiased by dust for galaxies in a wide range of local environments, and for clusters with a variety of masses. Our goals are to establish the dependence of galaxy star formation rates on local galaxy density at z=0.8, determine whether there are environments where the star formation is enhanced over the field, and understand how dust obscuration depends upon environment. Spitzer_Approved_Extragalactic Printed_by_SSC Mar 25, 10 16:24 Page 236/742 Spitzer Space Telescope − General Observer Proposal #50581 Spitzer South Ecliptic Pole Survey Principal Investigator: Mark Devlin Institution: University of Pennsylvania Technical Contact: Mark Devlin, University of Pennsylvania Co−Investigators: Colin Borys, Caltech/IPAC Edward Chapin, University of British Columbia Joshua Gundersen, University of Miami Mark Halpern, University of British Columbia Jeff Klein, University of Pennsylvania Barth Netterfield, University of Toronto Marie Rex, University of Pennsylvania Douglas Scott, University of British Columbia Matthew Truch, University of Pennsylvania Gregory Tucker, Brown University Shuji Matsuura, ISAS/JAXA David Hughes, INAOE Sophia Kahn, ALMA Chris Pearson, ESA Mai Shirahata, ISAS/JAXA Science Category: high−z galaxies (z>0.5) Observing Modes: MipsScan Hours Approved: 91.6 Abstract: The Balloon−borne Large Aperture Submillimeter Telescope, a precursor to Herschel−SPIRE, had a very successful long duration flight from Antarctica in December 2006. Two extragalactic fields were mapped in exquisite detail, discovering more submillimeter sources than all of the ground−based "blank sky" surveys put together. One deep field, centered on GOODS−S, already has extensive Spitzer imaging, and here we request MIPS time for the second field, a strip of ~10 square degrees centered near the South Ecliptic Pole. This is a unique extragalactic survey field because of the combination of BLAST 250, 350 and 500 micron maps with deep mutli−band mid− and far−IR imaging from the Akari satellite. The addition of Spitzer data at 24 and 70 microns will enable us to pursue several inter−related science goals. Firstly, we can construct detailed spectral energy distributions for many galaxies, which can then be used as templates for studying the fainter, higher redshift population. Secondly, our proposed MIPS depths of 1 sigma = 56 (3600) micro−Jy at 24 (70) microns, should be sufficient to yield identifications for the bulk of BLAST sources, enabling detailed studies of the evolution of LIRGs and ULIRGs in the crucial z=1−3 range. And thirdly, careful stacking of the MIPS 24 micron sources on the BLAST maps should allow us to resolve most of the far−IR background, and study the populations which are responsible for making it. The SEP field has existing or planned coverage for many ground−based observatories, and is also part of the Herschel HERMES Guaranteed Time project, as well as being ideally placed for ALMA follow−up. The missing ingredient is the deep mid−IR imaging which only MIPS can provide. Thursday March 25, 2010 xgal_covers.txt 118/371
Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 237/742 Spitzer Space Telescope − Legacy General Observer Proposal #169 Great Observatories Origins Deep Survey (GOODS) Principal Investigator: Mark Dickinson Institution: NOAO Technical Contact: Peter Eisenhardt, JPL Co−Investigators: Jacqueline Bergeron, ESO Stefano Casertano, STScI Catherine Cesarsky, ESO Ranga−Ram Chary, UC Santa Cruz Stefano Cristiani, ESO Peter Eisenhardt, JPL/Caltech David Elbaz, CEA Saclay/UC Santa Cruz Michael Fall, STScI Henry Ferguson, STScI Robert Fosbury, ST−ECF Riccardo Giacconi, JHU/AUI Mauro Giavalisco, STScI Norman Grogin, STScI Robert Hanisch, STScI Michael Hauser, STScI Richard Hook, ST−ECF Inger Jorgensen, Gemini Obs Anton Koekemoer, STScI Michael Ledlow, Gemini Obs Mario Livio, STScI Bahram Mobasher, STScI Paolo Padovani, STScI Casey Papovich, STScI/JHU William Reach, SSC/Caltech Alvio Renzini, ESO Marcia Rieke, U. Arizona Piero Rosati, ESO Katherine Roth, Gemini Obs Jean−Rene Roy, U. Laval Ethan Schreier, STScI Daniel Stern, JPL/Caltech Massimo Stiavelli, STScI Marianne Takamiya, Gemini Obs Eric Tollestrup, Boston U. Megan Urry, STScI Robert Williams, STScI Claudia Winge, Gemini Obs Edward Wright, UCLA Science Category: high−z galaxies (z>0.5) Observing Modes: IracMap MipsPhot Hours Approved: 647.0 Abstract: We propose a SIRTF Legacy Project, the Great Observatories Origins Deep Survey, to study galaxy formation and evolution over a wide range of redshift and cosmic lookback time. The survey will determine the galaxies’ mass assembly history, stellar populations, and energetic output from star formation (SF) and AGN. By observing at lambda >3um, SIRTF measures the rest−frame near− and mid−IR light from objects at 1
Page 1 and 2:
Spitzer_Approved_Extragalactic Mar
Page 3 and 4:
Page 5 and 6:
Page 7 and 8:
Page 9 and 10:
Page 11 and 12:
Page 13 and 14:
Page 15 and 16:
Page 17 and 18:
Page 19 and 20:
Page 21 and 22:
Page 23 and 24:
Page 25 and 26:
Page 27 and 28:
Page 29 and 30:
Page 31 and 32:
Page 33 and 34:
Page 35 and 36:
Page 37 and 38:
Page 39 and 40:
Page 41 and 42:
Page 43 and 44:
Page 45 and 46:
Page 47 and 48:
Page 49 and 50:
Page 51 and 52:
Page 53 and 54:
Page 55 and 56:
Page 57 and 58:
Page 59 and 60:
Page 61 and 62:
Page 63 and 64:
Page 65 and 66:
Page 67 and 68: Spitzer_Approved_Extragalactic Mar
Page 117: Spitzer_Approved_Extragalactic Mar
Page 121 and 122: Mar 25, 10 16:24 Spitzer_Approved_E
Page 165 and 166: Mar 25, 10 16:24 Spitzer_Approved_E
Page 169 and 170:
Page 171 and 172:
Page 173 and 174:
Page 175 and 176:
Page 177 and 178:
Page 179 and 180:
Page 181 and 182:
Page 183 and 184:
Page 185 and 186:
Page 187 and 188:
Page 189 and 190:
Page 191 and 192:
Page 193 and 194:
Page 195 and 196:
Page 197 and 198:
Page 199 and 200:
Page 201 and 202:
Page 203 and 204:
Page 205 and 206:
Page 207 and 208:
Page 209 and 210:
Page 211 and 212:
Page 213 and 214:
Page 215 and 216:
Page 217 and 218:
Page 219 and 220:
Page 221 and 222:
Page 223 and 224:
Page 225 and 226:
Page 227 and 228:
Page 229 and 230:
Page 231 and 232:
Page 233 and 234:
Page 235 and 236:
Page 237 and 238:
Page 239 and 240:
Page 241 and 242:
Page 243 and 244:
Page 245 and 246:
Page 247 and 248:
Page 249 and 250:
Page 251 and 252:
Page 253 and 254:
Page 255 and 256:
Page 257 and 258:
Page 259 and 260:
Page 261 and 262:
Page 263 and 264:
Page 265 and 266:
Page 267 and 268:
Page 269 and 270:
Page 271 and 272:
Page 273 and 274:
Page 275 and 276:
Page 277 and 278:
Page 279 and 280:
Page 281 and 282:
Page 283 and 284:
Page 285 and 286:
Page 287 and 288:
Page 289 and 290:
Page 291 and 292:
Page 293 and 294:
Page 295 and 296:
Page 297 and 298:
Page 299 and 300:
Page 301 and 302:
Page 303 and 304:
Page 305 and 306:
Page 307 and 308:
Page 309 and 310:
Page 311 and 312:
Page 313 and 314:
Page 315 and 316:
Page 317 and 318:
Page 319 and 320:
Page 321 and 322:
Page 323 and 324:
Page 325 and 326:
Page 327 and 328:
Page 329 and 330:
Page 331 and 332:
Page 333 and 334:
Page 335 and 336:
Page 337 and 338:
Page 339 and 340:
Page 341 and 342:
Page 343 and 344:
Page 345 and 346:
Page 347 and 348:
Page 349 and 350:
Page 351 and 352:
Page 353 and 354:
Page 355 and 356:
Page 357 and 358:
Page 359 and 360:
Page 361 and 362:
Page 363 and 364:
Page 365 and 366:
Page 367 and 368:
Page 369 and 370:
Page 371:
show all

Extragalactic abstracts - IRSA - California Institute of Technology

Create successful ePaper yourself

Delete template?

Save as template?