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 ESO 511-G030 214.8456 -26.6457 214.126189 -26.416188 221.40386 -12.022179 326.23004886 32.21661925 292.391 56156.7622337963 2012-08-17 18:17:37 56157.7960416667 2012-08-18 19:06:18 707023030 51.9172 270 51.9252 51.9252 0 51.9172 3 2 0 2 1 0 0 52.011 52.011 89.3158 3 PROCESSED 57606.8813194444 2016-08-06 21:09:06 56640 2013-12-14 00:00:00 56272.6998148148 2012-12-11 16:47:44 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071413 The study of "bare" Seyfert 1 AGN is essential to measure the true properties of the inner regions of the accretion disk. The nearby Seyfert ESO 511-G30 is a prime candidate for fulfilling this role due to its broad Fe K component and lack of any intrinsic warm absorption. It is also one of the X-ray brightest bare Seyferts featured in the Swift 58 month BAT catalogue as yet unobserved with Suzaku. We propose a 270 ks Suzaku observation of ESO 511-G30 to unambiguously constrain the properties of the accretion disk and subsequently the black hole spin. In addition, the HXD data will allow us to measure the Compton reflection hump, while the excellent soft X-ray spectral resolution of XIS will allow the origin of the soft excess to be determined. EXTRAGALACTIC COMPACT SOURCES 7 A JAMES REEVES USA 7 AO7 MEASURING THE ACCRETION DISK AND BLACK HOLE PROPERTIES OF ESO 511-G30 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707023030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707023030'

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

Go to top of this page ⏏