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
|
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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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