<=== observer ===> "KMATTILA",\ "Mattila, K.",\ "",\ "Helsinki University Observatory",\ "Tahtitorninmaki",\ "",\ "SF-00014",\ "Helsinki",\ "Finland",\ "358 01912947",\ "358 01912952",\ "MATTILA@cc.Helsinki.FI" <=== proposal ===> "DGBE_CP1",1,2,\ {"diffuse interstellar medium",\ "dust properties","galactic structure"},\ {"Ch. Leinert","D. Lemke","R.J. Laureijs","P.G. Mezger","L. Haikala",\ "T. Liljestrom","A. Leger"} <=== title ===> Diffuse infrared emission of the Galaxy, Part 1 <=== abstract ===> SCIENTIFIC ABSTRACT We want to investigate the IR properties of the diffuse infrared emission of the galaxy using PHT and CAM. Different programs are proposed depending on the accessible sky with ISO. If the Galactic Centre is visible, PHT-S spectra are measured at selected positions along and near the galactic plane between l=-60 and l=60 degrees. An important objective for this program is to measure intensities of the UIR emission features in different parts of the galaxy as the sightlines are sufficiently bright for good PHT-S spectra. The positions are representative for the galactic radiation away from bright discrete sources. The PHT-S spectra will be complemented by PHT-P measurements. As an additional program, LINKED observations with ISOCAM are proposed. These observations are described in Part 2 of this proposal. The CAM data are coordinated with the CP proposal "Selected Area Galactic Survey with ISOCAM" (Price et al.) and are shared between the consortia of this and Price's proposal. In case Orion is visible we study the (weaker) emission of the galactic anti-centre region. We will perform raster scans in the C_200 and C_135 micron bands along selected pieces of the accessible galactic equator from l=67 to l=331. In addition, raster scans perpendicular to the galactic plane will be performed centered at the same fields and reaching from b = -0.8 to b = 2.3 degrees. These data will be utilized to investigate the distribution of cold interstellar dust and the ISRF throughout the outer Galaxy and to search for small scale structures of the very cold dust emission. The spatial changes in dust grain populations is one central open problem. With its 3' wide beam (1.5'x 1.5' pixels) ISOPHOT-C200 is ideally suited for the kind of studies suggested here. The smaller beam as compared to COBE provides the advantage to avoid discrete sources and to see the truly diffuse component of the background radiation. OBSERVATION SUMMARY In case of an autumn launch (hole in Orion) we want to take 128 seconds PHT-S spectra with AOT P40 at regular positions along the galactic plane at b=0.0, b=+/-1, and at b=+/-5 degrees. The sensitivity of PHT-S is sufficient to achieve a signal (zodiacal background subtracted) r.m.s. of 0.8 and 1.5 MJy/sr per pixel for SS and SL, respectively. The observations at b=+/-5 degrees are off-positions, therefore the PHT-S exposure time on these positions will be half the exposure time at the other latitudes. AOT P03 measurements of 32 seconds in P_3.6 and P_7.3 will be performed to calibrate the SS and SL spectra. For b=0, P03 observations in the filterbands P_25, P_60 and P100 to determine the emission in a 99" aperture. These data will be compared and cross calibrated with both the LWS (cf ISO proposal by Caux et al.) and IRAS data. The P_3.6 and P_7.3 measurements will be obtained in a 99" aperture to obtain an S/N of at least 20 and to ensure comparison with the longer wavelength data. In case of a spring launch the camera C200 and AOT P22 configured in two filters - C_200 and C_135 - are used to scan selected pieces of 4.5 deg length at or near the galactic equator in the raster scan mode. In addition, we perform also a raster scan perpendicular to the galactic plane from -0.8 deg to +2.3 deg latitude at the central point of each galactic equator scan. The galactic coordinates of the central positions of these cross scans are: l / 67.0 90.0 118.0 165.0 240.0 275.0 301.0 degrees. b / 0.3 0.5 0.5 0.0 -0.5 -0.5 -0.2 degrees These positions have been selected in such a way that they avoid the bright hot dust areas around HII regions. The positions are not exactly at the galactic equator but follow the ridge of maximum FIR emission as determined from the IRAS 100 micron data. This optimizes the detection possibilities of very cold dust. Each set of measurements consists of ten concatenated linear raster scans - five in each of the two filters - of 32 positions with 180" spacing. The integration time is 10 sec per raster position. For a typical brightness in the outer galactic plane of 50 MJy/sr we reach a S/N of better than 500, i.e. features as weak as 0.5 can be measured with S/N = 5 in the single-pixel mode. <=== scientific_justification ===> FIXED TIME (part 1 autumn launch program): Each set of five positions (b=+5,+1,0,-1,-5 deg) at a given longitude is to be observed during the same orbit in order to enable us to subtract the zodiacal foreground emission from the ON-positions (b=+1,0,-1 deg) using the appropriate OFF- positions (b=+5,-5 deg). An even better zodiacal foreground subtraction is achieved when two or several sets of constant- longitude strips are observed during the same orbit. Suitable epochs determined from the SKY COVERAGE PLOTS (as provided to us by the SOT) are: Gal. longitude Orbit No. -60 -45 -30 90+-10 280+-5 -15 -5 0 +5 +15 110+-10 300+-5 +30 +45 +60 130+-10 320+-5 CONCATENATION (autumn launch program): Each pair of PHT-S and PHT-P observations at the same position is concatenated in order to have the same zodiacal foreground for both the PHT-S and PHT-P observations, and to improve the observational efficiency. The PHT-P1 observations must be performed after the PHT-S measurements in order to give the P1 detector some time to settle thereby improving the photometry. (spring launch program): Ten linear raster scans - five in each of the two filters - are concatenated at each one of the seven measuring areas. The central positions of all the scans are selected within a radius of 3 deg diameter. Thus we can perform scans of about 4.5 deg length along the galactic plane. Concatenation is essential for three reasons: (1) it improves the observing efficiency; (2) it provides longer interconnected scans; (3) it provides the possibility to measure the same positions with the same detector orientation in the two filters - essential for accurate colour determination. Time distribution for autumn launch main target list top 40 % second 30 % last 30 % total ___________________________________________________________________ PHT 10020 6192 3666 5.52 h SOT 4540 2800 1660 2.50 h ------------------------------------------------------------------- Total 14560 8992 5326 8.02 h Time distribution for autumn launch CAM target list top 40 % second 30 % last 30 % total ___________________________________________________________________ SOT 21560 0 0 6 h ------------------------------------------------------------------- Total 21560 0 0 6 h Time distribution for spring launch target list top 40 % second 30 % last 30 % total ___________________________________________________________________ PHT 9706 5450 4336 5.42 h SOT 4550 2470 1980 2.50 h PHT/SOT 9924 8200 9804 7.75 h ------------------------------------------------------------------- Total 24180 16120 16120 15.67 h <=== autumn_launch_targets ===> 1, "PHT40", 3.0, "N", "SA -60 +05 ", 12.17519, -57.05133, 1950, 0.000, 0.000, 330, 2 2, "PHT03", 3.0, "N", "SA -60 +05 ", 12.17519, -57.05133, 1950, 0.000, 0.000, 168, 0 3, "PHT40", 3.0, "N", "SA -60 +01 ", 12.10983, -61.16722, 1950, 0.000, 0.000, 394, 4 4, "PHT03", 3.0, "N", "SA -60 +01 ", 12.10983, -61.16722, 1950, 0.000, 0.000, 168, 0 5, "PHT40", 3.0, "N", "SA -60 +00 ", 12.07749, -61.93811, 1950, 0.000, 0.000, 394, 6 6, "PHT03", 3.0, "N", "SA -60 +00 ", 12.07749, -61.93811, 1950, 0.000, 0.000, 430, 0 7, "PHT40", 3.0, "N", "SA -60 -05 ", 11.94203, -68.55083, 1950, 0.000, 0.000, 330, 8 8, "PHT03", 3.0, "N", "SA -60 -05 ", 11.94203, -68.55083, 1950, 0.000, 0.000, 168, 0 9, "PHT40", 1.0, "N", "SA -45 +05 ", 14.25514, -55.38917, 1950, 0.000, 0.000, 330, 10 10, "PHT03", 1.0, "N", "SA -45 +05 ", 14.25514, -55.38917, 1950, 0.000, 0.000, 168, 0 11, "PHT40", 2.0, "N", "SA -45 +01 ", 14.48364, -59.18833, 1950, 0.000, 0.000, 394, 12 12, "PHT03", 2.0, "N", "SA -45 +01 ", 14.48364, -59.18833, 1950, 0.000, 0.000, 168, 0 13, "PHT40", 1.0, "N", "SA -45 +00 ", 14.52005, -60.15806, 1950, 0.000, 0.000, 394, 14 14, "PHT03", 1.0, "N", "SA -45 +00 ", 14.52005, -60.15806, 1950, 0.000, 0.000, 430, 0 15, "PHT40", 2.0, "N", "SA -45 -01 ", 14.58431, -61.00528, 1950, 0.000, 0.000, 394, 16 16, "PHT03", 2.0, "N", "SA -45 -01 ", 14.58431, -61.00528, 1950, 0.000, 0.000, 168, 0 17, "PHT40", 1.0, "N", "SA -45 -05 ", 14.81219, -64.74917, 1950, 0.000, 0.000, 330, 18 18, "PHT03", 1.0, "N", "SA -45 -05 ", 14.81219, -64.74917, 1950, 0.000, 0.000, 168, 0 19, "PHT40", 1.0, "N", "SA -30 +05 ", 15.69111, -48.45722, 1950, 0.000, 0.000, 330, 20 20, "PHT03", 1.0, "N", "SA -30 +05 ", 15.69111, -48.45722, 1950, 0.000, 0.000, 168, 0 21, "PHT40", 2.0, "N", "SA -30 +01 ", 15.94756, -51.45444, 1950, 0.000, 0.000, 394, 22 22, "PHT03", 2.0, "N", "SA -30 +01 ", 15.94756, -51.45444, 1950, 0.000, 0.000, 168, 0 23, "PHT40", 1.0, "N", "SA -30 +00 ", 15.99728, -52.17395, 1950, 0.000, 0.000, 394, 24 24, "PHT03", 1.0, "N", "SA -30 +00 ", 15.99728, -52.17395, 1950, 0.000, 0.000, 430, 0 25, "PHT40", 2.0, "N", "SA -30 -01 ", 16.08383, -53.03667, 1950, 0.000, 0.000, 394, 26 26, "PHT03", 2.0, "N", "SA -30 -01 ", 16.08383, -53.03667, 1950, 0.000, 0.000, 168, 0 27, "PHT40", 1.0, "N", "SA -30 -05 ", 16.38932, -56.06761, 1950, 0.000, 0.000, 330, 28 28, "PHT03", 1.0, "N", "SA -30 -05 ", 16.38932, -56.06761, 1950, 0.000, 0.000, 168, 0 29, "PHT40", 1.0, "N", "SA -15 +05 ", 16.67208, -38.16031, 1950, 0.000, 0.000, 330, 30 30, "PHT03", 1.0, "N", "SA -15 +05 ", 16.67208, -38.16031, 1950, 0.000, 0.000, 168, 0 31, "PHT40", 2.0, "N", "SA -15 +01 ", 16.95986, -40.73925, 1950, 0.000, 0.000, 394, 32 32, "PHT03", 2.0, "N", "SA -15 +01 ", 16.95986, -40.73925, 1950, 0.000, 0.000, 168, 0 33, "PHT40", 1.0, "N", "SA -15 +00 ", 17.02858, -41.05942, 1950, 0.000, 0.000, 394, 34 34, "PHT03", 1.0, "N", "SA -15 +00 ", 17.02858, -41.05942, 1950, 0.000, 0.000, 430, 0 35, "PHT40", 2.0, "N", "SA -15 -01 ", 17.07167, -41.90722, 1950, 0.000, 0.000, 394, 36 36, "PHT03", 2.0, "N", "SA -15 -01 ", 17.07167, -41.90722, 1950, 0.000, 0.000, 168, 0 37, "PHT40", 1.0, "N", "SA -15 -05 ", 17.39814, -44.08889, 1950, 0.000, 0.000, 330, 38 38, "PHT03", 1.0, "N", "SA -15 -05 ", 17.39814, -44.08889, 1950, 0.000, 0.000, 168, 0 39, "PHT40", 1.0, "N", "SA -05 +05 ", 17.19547, -29.68417, 1950, 0.000, 0.000, 330, 40 40, "PHT03", 1.0, "N", "SA -05 +05 ", 17.19547, -29.68417, 1950, 0.000, 0.000, 168, 0 41, "PHT40", 2.0, "N", "SA -05 +00 ", 17.49369, -33.14167, 1950, 0.000, 0.000, 394, 42 42, "PHT03", 2.0, "N", "SA -05 +00 ", 17.49369, -33.14167, 1950, 0.000, 0.000, 168, 0 43, "PHT40", 1.0, "N", "SA -05 +01 ", 17.43961, -32.65528, 1950, 0.000, 0.000, 394, 44 44, "PHT03", 1.0, "N", "SA -05 +01 ", 17.43961, -32.65528, 1950, 0.000, 0.000, 430, 0 45, "PHT40", 2.0, "N", "SA -05 -01 ", 17.57237, -33.59522, 1950, 0.000, 0.000, 394, 46 46, "PHT03", 2.0, "N", "SA -05 -01 ", 17.57237, -33.59522, 1950, 0.000, 0.000, 168, 0 47, "PHT40", 1.0, "N", "SA -05 -05 ", 17.90039, -34.64728, 1950, 0.000, 0.000, 330, 48 48, "PHT03", 1.0, "N", "SA -05 -05 ", 17.90039, -34.64728, 1950, 0.000, 0.000, 168, 0 49, "PHT40", 1.0, "N", "SA +05 +05 ", 17.53783, -21.00667, 1950, 0.000, 0.000, 330, 50 50, "PHT03", 1.0, "N", "SA +05 +05 ", 17.53783, -21.00667, 1950, 0.000, 0.000, 168, 0 51, "PHT40", 2.0, "N", "SA +05 +01 ", 17.73301, -26.34897, 1950, 0.000, 0.000, 394, 52 52, "PHT03", 2.0, "N", "SA +05 +01 ", 17.73301, -26.34897, 1950, 0.000, 0.000, 168, 0 53, "PHT40", 1.0, "N", "SA +05 +00 ", 17.84489, -25.85528, 1950, 0.000, 0.000, 394, 54 54, "PHT03", 1.0, "N", "SA +05 +00 ", 17.84489, -25.85528, 1950, 0.000, 0.000, 430, 0 55, "PHT40", 2.0, "N", "SA +05 -01 ", 17.89054, -26.89353, 1950, 0.000, 0.000, 394, 56 56, "PHT03", 2.0, "N", "SA +05 -01 ", 17.89054, -26.89353, 1950, 0.000, 0.000, 168, 0 57, "PHT40", 1.0, "N", "SA +05 -05 ", 18.18914, -29.31611, 1950, 0.000, 0.000, 330, 58 58, "PHT03", 1.0, "N", "SA +05 -05 ", 18.18914, -29.31611, 1950, 0.000, 0.000, 168, 0 59, "PHT40", 1.0, "N", "SA +15 +05 ", 17.79984, -15.18008, 1950, 0.000, 0.000, 330, 60 60, "PHT03", 1.0, "N", "SA +15 +05 ", 17.79984, -15.18008, 1950, 0.000, 0.000, 168, 0 61, "PHT40", 2.0, "N", "SA +15 +00 ", 18.27373, -15.29581, 1950, 0.000, 0.000, 394, 62 62, "PHT03", 2.0, "N", "SA +15 +00 ", 18.27373, -15.29581, 1950, 0.000, 0.000, 168, 0 63, "PHT40", 1.0, "N", "SA +15 +01 ", 18.20947, -14.79167, 1950, 0.000, 0.000, 394, 64 64, "PHT03", 1.0, "N", "SA +15 +01 ", 18.20947, -14.79167, 1950, 0.000, 0.000, 430, 0 65, "PHT40", 2.0, "N", "SA +15 -01 ", 18.34061, -15.53972, 1950, 0.000, 0.000, 394, 66 66, "PHT03", 2.0, "N", "SA +15 -01 ", 18.34061, -15.53972, 1950, 0.000, 0.000, 168, 0 67, "PHT40", 1.0, "N", "SA +15 -05 ", 18.72307, -15.99325, 1950, 0.000, 0.000, 330, 68 68, "PHT03", 1.0, "N", "SA +15 -05 ", 18.72307, -15.99325, 1950, 0.000, 0.000, 168, 0 69, "PHT40", 1.0, "N", "SA +30 +05 ", 18.41393, -0.79525, 1950, 0.000, 0.000, 330, 70 70, "PHT03", 1.0, "N", "SA +30 +05 ", 18.41393, -0.79525, 1950, 0.000, 0.000, 168, 0 71, "PHT40", 2.0, "N", "SA +30 +01 ", 18.63167, -3.53500, 1950, 0.000, 0.000, 394, 72 72, "PHT03", 2.0, "N", "SA +30 +01 ", 18.63167, -3.53500, 1950, 0.000, 0.000, 168, 0 73, "PHT40", 1.0, "N", "SA +30 +00 ", 18.65869, -4.57192, 1950, 0.000, 0.000, 394, 74 74, "PHT03", 1.0, "N", "SA +30 +00 ", 18.65869, -4.57192, 1950, 0.000, 0.000, 430, 0 75, "PHT40", 2.0, "N", "SA +30 -01 ", 18.72050, -4.97408, 1950, 0.000, 0.000, 394, 76 76, "PHT03", 2.0, "N", "SA +30 -01 ", 18.72050, -4.97408, 1950, 0.000, 0.000, 168, 0 77, "PHT40", 1.0, "N", "SA +30 -05 ", 18.94223, -7.26006, 1950, 0.000, 0.000, 330, 78 78, "PHT03", 1.0, "N", "SA +30 -05 ", 18.94223, -7.26006, 1950, 0.000, 0.000, 168, 0 79, "PHT40", 1.0, "N", "SA +45 +05 ", 18.82609, 11.16108, 1950, 0.000, 0.000, 330, 80 80, "PHT03", 1.0, "N", "SA +45 +05 ", 18.82609, 11.16108, 1950, 0.000, 0.000, 168, 0 81, "PHT40", 2.0, "N", "SA +45 +01 ", 19.16099, 11.99239, 1950, 0.000, 0.000, 394, 82 82, "PHT03", 2.0, "N", "SA +45 +01 ", 19.16099, 11.99239, 1950, 0.000, 0.000, 168, 0 83, "PHT40", 1.0, "N", "SA +45 +00 ", 19.18692, 10.56311, 1950, 0.000, 0.000, 394, 84 84, "PHT03", 1.0, "N", "SA +45 +00 ", 19.18692, 10.56311, 1950, 0.000, 0.000, 430, 0 85, "PHT40", 2.0, "N", "SA +45 -01 ", 19.30282, 11.56853, 1950, 0.000, 0.000, 394, 86 86, "PHT03", 2.0, "N", "SA +45 -01 ", 19.30282, 11.56853, 1950, 0.000, 0.000, 168, 0 87, "PHT40", 1.0, "N", "SA +45 -05 ", 19.47201, 7.94144, 1950, 0.000, 0.000, 330, 88 88, "PHT03", 1.0, "N", "SA +45 -05 ", 19.47201, 7.94144, 1950, 0.000, 0.000, 168, 0 89, "PHT40", 3.0, "N", "SA +60 +05 ", 19.42883, 27.38680, 1950, 0.000, 0.000, 330, 90 90, "PHT03", 3.0, "N", "SA +60 +05 ", 19.42883, 27.38680, 1950, 0.000, 0.000, 168, 0 91, "PHT40", 3.0, "N", "SA +60 +01 ", 19.66785, 25.16072, 1950, 0.000, 0.000, 394, 92 92, "PHT03", 3.0, "N", "SA +60 +01 ", 19.66785, 25.16072, 1950, 0.000, 0.000, 168, 0 93, "PHT40", 3.0, "N", "SA +60 +00 ", 19.71197, 24.19167, 1950, 0.000, 0.000, 394, 94 94, "PHT03", 3.0, "N", "SA +60 +00 ", 19.71197, 24.19167, 1950, 0.000, 0.000, 430, 0 95, "PHT40", 3.0, "N", "SA +60 -05 ", 20.05239, 22.22619, 1950, 0.000, 0.000, 330, 96 96, "PHT03", 3.0, "N", "SA +60 -05 ", 20.05239, 22.22619, 1950, 0.000, 0.000, 168, 0 97, "PHT40", 3.0, "N", "SA +60 -01 ", 19.76242, 23.25714, 1950, 0.000, 0.000, 394, 98 98, "PHT03", 3.0, "N", "SA +60 -01 ", 19.76242, 23.25714, 1950, 0.000, 0.000, 168, 0 <=== spring_launch_targets ===> 1, "PHT22", 1.0, "N", "g67_0_-1 C200 ", 19.88833, 28.69056, 1950, 0.000, 0.000, 948, 2 2, "PHT22", 1.0, "N", "g67_0_0 C200 ", 19.94667, 29.92472, 1950, 0.000, 0.000, 788, 3 3, "PHT22", 1.0, "N", "g67_0_1 C200 ", 20.00611, 31.15306, 1950, 0.000, 0.000, 788, 4 4, "PHT22", 1.0, "N", "g67_0_0 C200 ", 19.94667, 29.92472, 1950, 0.000, 0.000, 788, 5 5, "PHT22", 1.0, "N", "g67_1_0 C200 ", 19.85111, 30.68250, 1950, 0.000, 0.000, 788, 6 6, "PHT22", 1.0, "N", "g67_0_-1 C135 ", 19.88833, 28.69056, 1950, 0.000, 0.000, 792, 7 7, "PHT22", 1.0, "N", "g67_0_0 C135 ", 19.94667, 29.92472, 1950, 0.000, 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