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 CYG X-2 326.1609 38.3293 325.643028 38.098792 346.688554 47.972011 87.3271497 -11.30495752 51.1203 54648.0669097222 2008-07-01 01:36:21 54650.6154398148 2008-07-03 14:46:14 403063010 72.4308 100 102.6922 72.4308 0 89.8144 1 1 0 2 1 0 0 88.1331 88.1331 220.1678 0 PROCESSED 57527.0641319444 2016-05-19 01:32:21 55031 2009-07-19 00:00:00 54665.3170601852 2008-07-18 07:36:34 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031165 The nature of ultra-dense matter in neutron stars remains enigmatic. To probe this requires accurate neutron star radii and masses. We recently showed that broad iron lines in neutron star low-mass X-ray binaries (LMXBs) constrain the neutron star radius. LMXBs also provide us with another tool, kHz quasi-periodic oscillations (QPOs). Combining the inner disk velocity (from modeling the iron line) and the frequency of the kHz QPOs gives a method to measure the neutron star mass. We propose a 100 ks observation of Cyg X-2 with Suzaku to provide a detailed iron line profile. Combined with simultaneous observations with RXTE to determine the kHz QPO frequency, we will measure the neutron star mass. Cyg X-2 is the perfect test case as it already has a known mass from optical observations. GALACTIC POINT SOURCES 4 B EDWARD CACKETT USA 3 AO3 MEASURING NEUTRON STAR MASSES USING BROAD IRON LINES AND KHZ QPOS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403063010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403063010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏