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 | CYGNUS X-1 | 299.5796 | 35.2119 | 299.109658 | 35.075474 | 313.654707 | 54.262131 | 71.33922039 | 3.07967202 | 58.5817 | 56796.2767476852 | 2014-05-19 06:38:31 | 56799.3266203704 | 2014-05-22 07:50:20 | 409049010 | 14.5127 | 30 | 0 | 14.5127 | 0 | 0 | 0 | 3 | 0 | 0 | 1 | 0 | 0 | 113.8259 | 113.8259 | 263.4619 | 1 | PROCESSED | 57615.2053703704 | 2016-08-15 04:55:44 | 57180 | 2015-06-07 00:00:00 | 56811.8023958333 | 2014-06-03 19:15:27 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 091241 | We propose for a 30 ks observation of the accreting black hole Cygnus X-1 to occur simultaneously with NuSTAR. In mid-2012, we obtained a joint Suzaku/NuSTAR observation of Cyg X-1 in the soft state, and we clearly see reflection features with a relativistically broadened iron line that we have used to constrain the geometry of the accretion disk, including finding possible evidence for a warped accretion disk, and the black hole spin. This TOO proposal is to observe the source in the hard state to constrain how the accretion geometry changes between states. The combination of Suzaku and NuSTAR covers, with very good energy resolution and throughput, the thermal component, the iron line complex, the iron absorption edge, and the hard X-ray reflection hump. | GALACTIC POINT SOURCES | 4 | A | JOHN TOMSICK | USA | 9 | AO9-TOO | CYGNUS X-1 IN THE HARD STATE WITH SUZAKU AND NUSTAR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409049010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '409049010'
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