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 1608-52 | 243.1847 | -52.3651 | 242.223789 | -52.237385 | 251.315712 | -30.647315 | 330.96850701 | -0.81056533 | 96.6085 | 55266.077650463 | 2010-03-11 01:51:49 | 55267.0072222222 | 2010-03-12 00:10:24 | 404044010 | 34.0101 | 30 | 34.0101 | 34.0101 | 0 | 34.0101 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 30.194 | 30.194 | 80.2978 | 0 | PROCESSED | 57550.8305902778 | 2016-06-11 19:56:03 | 55647 | 2011-03-27 00:00:00 | 55279.4591666667 | 2010-03-24 11:01:12 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 041223 | The true nature of X-ray emission from neutron star X-ray binaries (NSXRBs) has not been clear for sometime and there are many possibilities for the spectral model. Recent progress has been made, but relies on RXTE data which lacks the low energy sensitivity where disk emission is most prominent. Using Suzaku we propose four 30 ksec observations of the transient 4U 1608-52 throughout an outburst. We will test how spectral parameters change with luminosity, allowing us to untangle the correct model. An essential part of this proposal is the unique ability of Suzaku to detect asymmetric broad iron emission lines in NSXRBs. We will study how the iron line varies throughout the outburst, which combined with the spectral fits will test the interaction between the accretion disk and corona. | GALACTIC POINT SOURCES | 4 | A | EDWARD CACKETT | USA | 4 | AO4-TOO | ACCRETION DISK EVOLUTION THROUGHOUT A NEUTRON STAR LMXB OUTBURST | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404044010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404044010'
Your request has been accepted.
The download will start soon automatically.