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 161.2769 -59.635 160.789962 -59.371642 202.089433 -58.883736 287.57915278 -0.58292483 99.9027 54810.21125 2008-12-10 05:04:12 54811.2084953704 2008-12-11 05:00:14 403036010 48.5016 30 48.5016 48.5016 0 48.5016 2 2 0 2 1 0 0 42.4259 42.4259 86.1518 2 PROCESSED 57544.6853125 2016-06-05 16:26:51 55198 2010-01-02 00:00:00 54828.3640972222 2008-12-28 08:44:18 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031124 X-ray observations of Eta Carinae near the 2003 periastron passage confirmed that the X-ray emission primarily arises from collision of winds in a binary system, but raised fundamental questions about the cause of the 3 month-long X-ray minimum and an excess above ~10 keV (possibly up to 50 keV) in addition to the thermal emission with kT ~3-5 keV. These features would originate from plasma extremely embedded in the primary winds and acceleration of high energy particles at the wind colliding region. To resolve these features clearly, broad band Suzaku observations around the periastron passage are crucial. We propose four 30 ksec Suzaku observations of Eta Carinae during AO3, which will cover the next X-ray maximum (in late 2008) and minimum (in early 2009). GALACTIC POINT SOURCES 4 A KENJI HAMAGUCHI USA 3 AO3 X-RAY EMISSION FROM ETA CARINAE DURING THE X-RAY MAXIMUM AND MINIMUM HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403036010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403036010'

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