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 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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