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
|
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1 | 4U 1957+11 | 299.8589 | 11.6979 | 299.267976 | 11.560536 | 304.903477 | 31.592045 | 51.30303986 | -9.34292333 | 251.3459 | 55501.8275462963 | 2010-11-01 19:51:40 | 55502.7001157407 | 2010-11-02 16:48:10 | 405057030 | 35.3491 | 35 | 35.3571 | 35.3491 | 0 | 35.3571 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 27.1697 | 27.1697 | 75.362 | 0 | PROCESSED | 57553.9520601852 | 2016-06-14 22:50:58 | 55881 | 2011-11-16 00:00:00 | 55515.3015046296 | 2010-11-15 07:14:10 | 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/ver3.0/405057030/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '405057030'
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