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 | 202063010 | SIGMA_GEM | 115.82683 | 28.88398 | 115.04722 | 29.00354 | 112.62545 | 7.45076 | 191.18856 | 23.27364 | 100.00138 | 60985.92991 | 2025-11-06 22:19:04 | 60988.36949 | 2025-11-09 08:52:04 | 109.076 | 100.000 | 109.076 | 112.880 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 112.880 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2025-11-14 08:15:51 | 2026-11-15 00:00:00 | 2025-11-15 08:15:52 | 03.03.015.012 | gen20241115_xtd20250915_rsl20250915 | Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 | 000021386 | Nano/micro flare heating is a promising explanation for the solar/stellar coronal heating problem. The low-ionized Fe Ka line at 6.4 keV can be a tracer of stellar nano/micro flares. High-energy-resolution spectroscopy is necessary to determine the intensity and photoionization state of the Fe Ka line accurately. The ionization parameter of the Fe Ka line depends on the flare energy scale. We propose a 100 ks Resolve observation of the RS CVn-type star Sigma Gem to reproduce the flare frequency distribution of stellar nano/micro flares and investigate whether the temperature of the Sigma Gem corona can be explained by the sum of the energies of them. We also use Xtend to determine the temperature of the quiescent corona of Sigma Gem during the Resolve observation. | STELLAR CORONAE, WINDS, AND YOUNG STARS | 2 | B | SHUN INOUE | JAP | 2 | NOR | STELLAR CORONAL HEATING PROBLEM STUDIED BY OBSERVATIONS OF THE FE KA LINE OF THE RS CVN-TYPE STAR SIGMA GEM | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202063010/ | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '202063010'
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