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 | NGC6946 | 308.6989 | 60.1968 | 308.436769 | 60.023263 | 358.020745 | 71.889708 | 95.74917907 | 11.70533663 | 79.9968 | 56060.7040393518 | 2012-05-13 16:53:49 | 56063.8903935185 | 2012-05-16 21:22:10 | 807035010 | 198.879 | 200 | 198.879 | 198.8958 | 0 | 198.8948 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 182.1955 | 182.1955 | 275.2756 | 3 | PROCESSED | 57605.4921296296 | 2016-08-05 11:48:40 | 56442 | 2013-05-30 00:00:00 | 56075.3809027778 | 2012-05-28 09:08:30 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070098 | Hot X-ray emitting interstellar medium (ISM) carries important information about the history of star formation and evolution of galaxies. However, the origin of hot ISM is still unclear. We investigate the property of hot ISM according to luminosity of infrared emission, which is good tracer of star formation rate. If the hot ISM depend on the present activity of star formation, there are correlation between hot ISM and infrared emission. We propose the observation of the spiral galaxy NGC 6946. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | SAORI KONAMI | JAP | 7 | AO7 | CLARIFICATION OF THE ORIGIN OF HOT ISM IN SPIRAL GALAXIES | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807035010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807035010'
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