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. |
observation_id
|
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
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 300042020 | SS_CYGNI | 325.67751 | 43.58596 | 325.1865 | 43.35675 | 350.46587 | 52.65628 | 90.55863 | -7.11027 | 76.86924 | 60444.99866 | 2024-05-14 23:58:04 | 60448.29866 | 2024-05-18 07:10:04 | 158.798 | 100.000 | 158.798 | 140.806 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 2 | 31100010 | 320000A0 | 150.613 | 140.806 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2024-09-26 22:18:20 | 2025-08-31 00:00:00 | 2024-05-23 10:39:58 | 03.00.013.009 | gen20240315_xtd20240815_rsl20240815 | Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 | 000000067 | SS Cygni is one of the prototypical dwarf novae, which shows transitions between an optically quiescent state and an outburst state. In the outburst state, hard X-ray emission is thought to arise from coronae over an accretion disc, but their location is unclear. We will understand the corona geometry by measuring profiles of the coronal emission lines with the Resolve. In the quiescent state, on the other hand, it is commonly understood that the hard X-ray emission emanates from the optically thin boundary layer, yet its heating mechanism and radial profile of the BL plasma are both poorly understood. We will try to make them clear by means of spectroscopy of the emission lines from the plasma and the fluorescent iron K-alpha emission line with the Resolve. | ACCRETING WHITE DWARFS AND NOVAE | 3 | C | XRISM Collaboration | JAP | 0 | NOR-TOO | OBSERVATIONS OF SS CYGNI IN QUIESCENCE AND OUTBURST | archived | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300042020/ | WINDOW2 | WINDOW1 | 3 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '300042020'
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