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 X1630-472 248.5414 -47.3441 247.620794 -47.24014 254.106628 -25.078548 336.96314137 0.26612574 120.5775 53802.0758796296 2006-03-08 01:49:16 53802.7300231482 2006-03-08 17:31:14 400010040 21.2481 200 21.2481 21.2499 21.2499 21.2499 3 3 3 3 1 0 0 20.4778 20.4778 56.512 0 PROCESSED 57533.1620486111 2016-05-25 03:53:21 54247 2007-05-27 00:00:00 54041.7698726852 2006-11-02 18:28:37 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001058 We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. GALACTIC POINT SOURCES 4 A JEAN COTTAM JAP 0 SWG-TOO FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '400010040'

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