![[Science Operations home]](../../generic-images/sciopshomebtn.gif){kind=small}
![[NIRSPEC home]](nirspechomebtn.gif){kind=small}
Scientifically Approved NIRSPEC programs for Semester 2001B |
The approved programs for Gemini/NIRSPEC 2001B time on November 19-21, 2001 are listed below, along with the name and institution of the p.i., the countries of the p.i. and others on the proposal, and the proposal code. Because of time constraints it is likely that some of these programs will not be observed. If additional time is available other programs will be considered
| Code |
Title | P.I./Institution/countries) |
| 152s_e | He 10830 in pre-main sequence stars | S. Edwards / Smith College / USA |
| 154t_g |
Hydrocarbons in Titan | T. Geballe / Gemini |
| 156t_g | C-H stretch overtone | T. Geballe / Gemini |
| 157scb | 16O/17O in halo giants | S. Balachandran / Univ. Maryland / USA |
| 158bjh | UIR bands in protoplanetary nebulae | B.J. Hrivnak / Valparaiso Univ. / USA (+Canada) |
| 159k_n | Methane transition in brown dwarfs | K. Noll/ STScI / USA |
| 160j_m | O in metal-poor stars | J. Melendez / Inst Astron e Geofis. / Brasil |
| 162j_n | Brown dwarfs and superplanets | J. Najita / NOAO / USA |
| 165s_l | Brown dwarf secondary in a CV | S.Littlefair / UK |
| 166rih | Companion to Black hole x-ray transient | R.I. Hynes / Univ. Southampton / UK (+ Spain) |
| 168mvm | O III in lensed galaxy | M. Vilar-Martin / Univ. of Hertfordshire / UK (+ESO) |
| 170esp | Nuclear regions of the youngest AGN | E.S. Perlman / U. Maryland / USA (+Sweden) |
| 171gfl | O II in Protocluster environment | G.F. Lewis / AAO / Austr, (+ UK, USA, France) |
| 172bvc | Boron abundance | B.V. Castilho / Lab. Nac. de Astrofis / Brasil |
| 175tsb | Stellar kinematics Seyfert nuclei | T. Storchi-Bergmann / Inst de Fisica / Brasil (+USA) |
| 176a_c | 3-D structure of Mg II QSO absorber | A. Crotts / Columbia Univ. / USA |
| 177x_f | z=4.7 quasar withour UV emission | X. Fan / StScI / USA |
| 178x_f | C IV in z=5.82 quasar | X. Fan / StScI / USA |
| 179gps | Power source of active ERO's | G.P. Smith / UK |
Last update November 14, 2001 Tom Geballe