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 | GX 301-2 | 186.5611 | -62.8021 | 185.862176 | -62.525248 | 221.491572 | -52.675278 | 300.05773343 | -0.07103063 | 326.712 | 54703.5522800926 | 2008-08-25 13:15:17 | 54704.0036689815 | 2008-08-26 00:05:17 | 403044010 | 11.4275 | 60 | 11.4292 | 11.4306 | 0 | 11.4275 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 10.7148 | 10.7148 | 38.9939 | 0 | PROCESSED | 57543.3977546296 | 2016-06-04 09:32:46 | 55218 | 2010-01-22 00:00:00 | 54720.435462963 | 2008-09-11 10:27:04 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031152 | We propose the first observation of the bright neutron star GX 301-2 with Suzaku. The aim of the proposed 60 ks observation is a study of the broadband spectrum of the source in unprecedented detail and quality. This will allow us to analyze the structure (including density and clumpiness) of the intense wind of the optical companion and the gas stream flowing from Wray 977 to the neutron star. Spectral data will be used to study the evolution of nH and the iron line with very high time resolution. Furthermore, we will perform phase resolved spectroscopy to study the spectral variation of the cyclotron line with pulse phase. | GALACTIC POINT SOURCES | 4 | A | RICHARD ROTHSCHILD | USA | 3 | AO3 | BROAD-BAND STUDY OF GX 301-2 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403044010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403044010'
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