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 GX 339-4 255.7297 -48.7352 254.782436 -48.66432 259.586148 -25.80756 338.99220289 -4.30584956 108.3513 54920.4773958333 2009-03-30 11:27:27 54921.5216435185 2009-03-31 12:31:10 403011030 39.6384 40 39.6633 39.6384 0 39.6633 2 2 0 2 1 0 0 35.0686 35.0686 90.186 0 PROCESSED 57545.9795601852 2016-06-06 23:30:34 55330 2010-05-14 00:00:00 54931.0610416667 2009-04-10 01:27:54 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030046 Growing evidence indicates that a relativistic jet from a black hole is produced during its transition from the "hard state" to the "soft state" through the "very high state". We propose to make TOO observations of a Galactic black hole binary in the early phase of ourburst with Suzaku in order to reveal the evolution of the accretion disk structure during ejection events. We will trigger a TOO observation upon the RXTE ASM. At the same time we organize multiwavelength observations in radio and infrared/optical bands to examine the exact relation between the ejection and state transition. GALACTIC POINT SOURCES 4 A YOSHIHIRO UEDA JAP 3 AO3-TOO MULTIWAVELENGH OBSERVATIONS OF A GALACTIC BLACK HOLE IN EARLY PHASE OF OUTBURST HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403011030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403011030'

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

Go to top of this page ⏏