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 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'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏