! File: 1244C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:07:32:39 coverpage: title_1: NATURE OF GALAXIES WITH ANOMALOUSLY LARGE IR EMISSION sci_cat: QUASARS & AGN sci_subcat: SEYFERTS proposal_for: GTO/FOC pi_fname: F. DUCCIO pi_lname: MACCHETTO pi_inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (301) 338-4790 keywords_1: INFRARED, STARBURST, SEYFERT, IRAS hours_pri: 4.00 num_pri: 11 foc: X pi_position: CHIEF, ISB ! end of coverpage abstract: line_1: One of the most important discoveries of the IRAS Satellite has been that line_2: some galaxies have anomalously large infrared to optical emission. These line_3: predominantly interacting "Starburst" systems are probably sites of extremely line_4: vigorous star formation. IRAS has also shown that many Seyferts have strong line_5: mid-IR components which are most likely due to emission from dust in the line_6: nuclear narrow-line regions. line_8: We wish to make broad and narrow-band images of extreme-IR galaxies from line_9: both of these classes. This is a pilot study. The ultimate aim of such a line_10: program will be to (a) determine the morphologies and colour distributions of line_11: both classes of objects as a function of distance and (b) investigate possible line_12: relations between the Seyfert and starburst phenomena. ! ! end of abstract general_form_proposers: lname: MILEY fname: GEORGE mi: K. inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE country: USA esa: X ! lname: MACCHETTO fname: F. DUCCIO inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE country: USA esa: X ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: All exposures to be executed in Cycles 1-2. ! question: 13 section: 1 line_1: One of the most important discoveries of the IRAS Satellite has been that line_2: some galaxies have anomalously large infrared to optical emission. These line_3: predominantly interacting "Starburst" systems are probably sites of extremely line_4: vigorous star formation. IRAS has also shown that many seferts have strong line_5: mid-IR components which are most likely due to emission from dust in the line_6: nuclear narrow-line regions. line_8: We wish to make broad and narrow-band images of extreme-IR galaxies from line_9: both of these classes. This is a pilot study. The ultimate aim of such a line_10: program will be to (a) determine the morphologies and colour distributions of line_11: both classes of objects as a function of distance and (b) investigate possible line_12: relations between Seyfert and starburst phenomena. ! !end of general form text general_form_address: lname: MACCHETTO fname: F. DUCCIO category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: HOMEWOOD CAMPUS city: BALTIMORE state: MD zip: 21218 country: USA phone: (301) 338-4790 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: 0420+040P06 descr_1: SPIRAL WITH RADIO LOBES pos_1: RA = 04H 21M 02.7S +/- 0.1S, pos_2: DEC = +04D 01' 08" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.0462 plate_req: N ! targnum: 2 name_1: 1150-388 descr_1: STRONG H ALPHA (IR/B=18) pos_1: RA = 11H 50M 40.2S +/- 0.1S, pos_2: DEC = -38D 51' 09" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.010 plate_req: N ! targnum: 3 name_1: 1304-234P11 descr_1: SEYFERT 2 (HIGH IONIZATION) pos_1: RA = 13H 04M 23.5S +/- 0.1S, pos_2: DEC = -23D 24' 31" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.009 plate_req: N ! targnum: 4 name_1: 1318-314 descr_1: MULTIPLE SYSTEM WITH STRONG H ALPHA (IR/B= descr_2: 9) pos_1: RA = 13H 18M 07.3S +/- 0.1S, pos_2: DEC = -31D 28' 43" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.053 plate_req: N ! targnum: 5 name_1: 1319-164P11 descr_1: SEYFERT 2/N TYPE BROAD 03 pos_1: RA = 13H 19M 42.3S +/- 0.1S, pos_2: DEC = -16D 27' 53" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.017 plate_req: N ! targnum: 6 name_1: 1404+012P11 descr_1: NO EM. LINES/LONG IR/B pos_1: RA = 14H 04M 04.9S +/- 0.1S, pos_2: DEC = +01D 17' 10" +/- 1" equinox: 1950 pm_or_par: NO plate_req: N ! targnum: 7 name_1: ARP220 descr_1: GALAXY WITH IR/B=80 pos_1: RA = 15H 32M 46.92S +/- 0.1S, pos_2: DEC = +23D 40' 07.9" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.018 plate_req: N ! targnum: 8 name_1: 1840-624P11 descr_1: SEYFERT 1 pos_1: RA = 18H 40M 09.2S +/- 0.1S, pos_2: DEC = -62D 25' 02.02" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.0135 plate_req: N ! targnum: 9 name_1: 2016-527 descr_1: SEYFERT 2 pos_1: RA = 20H 16M 13.7S +/- 0.1S, pos_2: DEC = -52D 46' 47" +/- 1" equinox: 1950 pm_or_par: NO rv_or_z: Z=0.017 plate_req: N ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: ARP220 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F120M num_exp: 1 time_per_exp: 40M priority: 1 req_1: CYCLE 1 / 1-4 ! linenum: 2.000 targname: ARP220 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F165W num_exp: 1 time_per_exp: 20M priority: 1 ! linenum: 3.000 targname: ARP220 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F372M num_exp: 1 time_per_exp: 40M priority: 1 ! linenum: 4.000 targname: ARP220 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F430W num_exp: 1 time_per_exp: 20M priority: 1 ! ! end of exposure logsheet ! No scan data records found