DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

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 NGC3556 167.883 55.6841 167.153795 55.95585 141.585681 45.289435 148.29932367 56.24590288 111.9355 54795.9750694444 2008-11-25 23:24:06 54797.8890162037 2008-11-27 21:20:11 803013010 84.1642 100 84.1702 84.1659 0 84.1642 2 2 0 2 1 0 0 60.3537 60.3537 165.2879 2 PROCESSED 57544.6094212963 2016-06-05 14:37:34 55175 2009-12-10 00:00:00 54811.7645717593 2008-12-11 18:20:59 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030058 We propose to observe NGC 3556, a nearby edge-on spiral galaxy, with 100 ks exposure. Galactic coronal X-ray emission in and around several spiral galaxies have been spatially resolved using Chandra and XMM instruments. The target is one of these galaxies showing relatively luminous X-ray emission. Due to limited spectral capability of these instruments, X-ray spectral properties of these diffuse emission have not yet been investigated. We use good spectral capability of the SUZAKU/XIS to investigate the temperature structure and constrain the metal abundance pattern for the first time in galactic corona. We study origin, heating mechanism, and chemical properties of these galactic corona. EXTRAGALACTIC DIFFUSE SOURCES 8 C TAKAYUKI TAMURA JAP 3 AO3 GALACTIC CORONA IN AND AROUND THE EDGE-ON GALAXY NGC 3556 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803013010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '803013010'

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