DARTS/Astro Query System - SQL Search -

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No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 ETA CARINAE 161.2814 -59.6826 160.794718 -59.419235 202.159659 -58.914636 287.60335194 -0.62397837 335.8837 56875.8359259259 2014-08-06 20:03:44 56876.6961111111 2014-08-07 16:42:24 409028010 21.5455 30 21.5455 21.5455 0 21.5455 2 2 0 2 1 0 0 9.9582 9.9582 22.028 0 PROCESSED 57616.4668518518 2016-08-16 11:12:16 57264 2015-08-30 00:00:00 56898.441875 2014-08-29 10:36:18 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 091202 Eta Carinae is an extremely massive binary system whose strong winds produce a variety of high-energy X-ray and possibly gamma-ray emission. Earlier XMM-Newton, Suzaku and INTEGRAL observations found interesting features in the extremely hard X-ray band: i) a flat spectral component above 9 keV toward the flux maximum; ii) strong 15-20 keV emission during an occultation of the wind-wind colliding plasma; iii) stable power-law emission above 25 keV. These features are signs of the highest energy processes yet detected in any colliding wind binary. Broad band X-ray observations around periastron are essential to understanding those features. We therefore propose Suzaku observations at 5 key phases around the next periastron passage of eta Carinae in 2014.6. GALACTIC POINT SOURCES 4 A KENJI HAMAGUCHI USA 9 AO9 PROBING THE HIGHEST ENERGY PHENOMENA OF ETA CARINAE AROUND PERIASTRON IN 2014 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409028010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '409028010'

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