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 339-4 255.7085 -48.7866 254.760711 -48.715619 259.576938 -25.860175 338.94274721 -4.32598042 275.4008 56526.5726967593 2013-08-22 13:44:41 56529.3592476852 2013-08-25 08:37:19 408034010 101.0196 100 101.0196 101.0196 0 101.0196 2 2 0 2 1 0 0 90.3169 90.3169 240.7097 1 PROCESSED 57612.5083680556 2016-08-12 12:12:03 56956 2014-10-26 00:00:00 56588.9590046296 2013-10-23 23:00:58 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081242 Due to the presence of a steady jet, constraining the properties of black hole systems in their hard state is important for understanding accretion disks and jets. Along with radio observations, Suzaku is constraining theoretical models by answering the following questions: Does the inner edge of the accretion disk recede in the hard state? How is the location of the disk's inner edge related to the presence of a jet? This proposal includes the use of Suzaku, NuSTAR, and radio observations to address these questions. A main diagnostic of the accretion geometry is the Compton reflection component, and the combination of Suzaku and NuSTAR covers, with very good energy resolution and sensitivity, the iron emission line, the absorption edges, and the hard X-ray reflection bump. GALACTIC POINT SOURCES 4 A JOHN TOMSICK USA 8 AO8-TOO CONSTRAINING THE HARD STATE ACCRETION GEOMETRY FOR BLACK HOLE BINARIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408034010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '408034010'

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

Go to top of this page ⏏