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 4U 1957+11 299.8426 11.72 299.251782 11.582704 304.891281 31.61725 51.31417386 -9.31797438 71.6227 55320.4377777778 2010-05-04 10:30:24 55321.4168055556 2010-05-05 10:00:12 405057010 35.796 35 35.804 35.804 0 35.796 2 2 0 2 1 0 0 30.8692 30.8692 84.58 0 PROCESSED 57551.4086226852 2016-06-12 09:48:25 55741 2011-06-29 00:00:00 55375.7567013889 2010-06-28 18:09:39 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051254 We propose three observations of the black hole candidate 4U 1957+11. It is one of only two persistently soft state BHC, and has the highest fitted temperature, and highest fitted spin parameter, of any observed BHC. The question arises of whether this high spin is a good estimate of the true spin, or whether this high temperature is evidence of a low level or corona or wind. The multiple Suzaku observations will allow us to track how the disk parameters change, and offer us a 40% chance of observing a state with a large coronal component. The latter might be indicative of launching of a disk wind. GALACTIC POINT SOURCES 4 B MICHAEL NOWAK USA 5 AO5 4U1957+11: THE MOST RAPIDLY SPINNING BLACK HOLE? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405057010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '405057010'

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